Does back reaction enforce the averaged null energy condition in semiclassical gravity?
Open accessAbstract
The expectation value $〈{T}_{\mathrm{ab}}〉$ of the renormalized stress-energy tensor of quantum fields generically violates the classical, local positive energy conditions of general relativity. Nevertheless, it is possible that $〈{T}_{\mathrm{ab}}〉$ may still satisfy some nonlocal positive energy conditions. Most prominent among these nonlocal conditions is the averaged null energy condition (ANEC), which states that $\ensuremath{\int}〈{T}_{\mathrm{ab}}〉{k}^{a}{k}^{b}d\ensuremath{\lambda}>~0$ along any complete null geodesic, where ${k}^{a}$ denotes the geodesic tangent, with affine parameter $\ensuremath{\lambda}$. If the ANEC holds, then traversable wormholes cannot occur. However, although the ANEC holds in Minkowski spacetime, it is known that the ANEC can be violated in curved spacetimes if one is allowed to choose the spacetime and quantum state arbitrarily, without imposition of the semiclassical Einstein equation, ${G}_{\mathrm{ab}}=8\ensuremath{\pi}〈{T}_{\mathrm{ab}}〉$. In this paper, we investigate whether the ANEC holds for self-consistent solutions of the semiclassical Einstein equation. We study a free, linear, massless scalar field with arbitrary curvature coupling in the context of perturbation theory about the flat spacetime/vacuum solution, and we modify the perturbed semiclassical equations by the "reduction of order" procedure to eliminate spurious solutions. We also restrict attention to the limit in which the length scales determined by the state and metric are much larger than the Planck length. At first order in the metric and state perturbations, and for pure states of the scalar field, we find that the ANEC integral vanishes, as it must for any positivity result to hold. For mixed states, the ANEC integral can be negative. However, we prove that if we average the ANEC integral transverse to the geodesic, using a suitable Planck scale smearing function, a strictly positive result is obtained in all cases except for the trivial flat spacetime/vacuum solution. Similar results hold for pure states at second order in perturbation theory, when we additionally specialize to the situation where incoming classical gravitational radiation does not dominate the first-order metric perturbation. These results suggest---in agreement with conclusions drawn by Ford and Roman from entirely independent arguments---that if traversable wormholes do exist as self-consistent solutions of the semiclassical equations, they cannot be macroscopic but must be "Planck scale." In the course of our analysis, we investigate a number of more general issues relevant to doing perturbative expansions of the semiclassical equations off of flat spacetime, including an analysis of the nature of the semiclassical Einstein equation and of prescriptions for extracting physically relevant solutions. A large portion of our paper is devoted to the treatment of these more general issues.
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TL;DR
The paper asks whether the semiclassical Einstein equation enforces the averaged null energy condition (ANEC) once backreaction is included. In perturbation theory about flat spacetime, the unsmeared ANEC integral can be violated, but a transversely smeared ANEC integral with Planck-scale smearing is strictly positive except for the trivial flat spacetime/vacuum solution.
Key findings
- At first order in perturbations, the ANEC integral vanishes for pure incoming states, as required for any positivity result; for mixed states it can be negative without transverse smearing, but is positive with transverse smearing when the smearing length exceeds a critical value of order the Planck length.
- At second order, for pure states and in the long-wavelength limit, the unsmeared ANEC integral can be negative, but the transversely smeared ANEC integral is always positive, assuming incoming classical gravitational radiation does not dominate the first-order metric perturbation.
- The authors conclude that if traversable wormholes exist as self-consistent semiclassical solutions, they cannot be macroscopic but must be “Planck scale,” in agreement with independent arguments by Ford and Roman.
- The paper also argues that the semiclassical Einstein equation has pathological higher-derivative solutions, but that in perturbation theory about flat spacetime the “reduction of order” procedure can eliminate spurious solutions while preserving long-wavelength accuracy.
Methods
- The authors study a free, linear, massless scalar field with arbitrary curvature coupling in perturbation theory about the flat spacetime/vacuum solution of the semiclassical Einstein equation \(G_{ab}=8\pi\langle T_{ab}\rangle\).
- They modify the perturbed semiclassical equations by the “reduction of order” procedure and restrict to lengthscales much larger than the Planck length.
- They analyze the ANEC integral and a transversely smeared version, using a smearing function \(S(x)\propto 1/(1+x^4/\Lambda_T^4)\), with critical smearing length \(\Lambda_{T,\rm crit}=8\pi\sqrt{a/\nu_0}\,L_p\) of order the Planck length.
Limitations
- The analysis applies only to non-self-interacting quantum fields; the paper notes that interacting fields could behave qualitatively differently, though it knows of no evidence for this.
- The results are perturbative about Minkowski spacetime/vacuum, and the second-order pure-state analysis additionally assumes that incoming classical gravitational radiation does not dominate the first-order metric perturbation.
- The positivity result requires a transverse smearing function that falls off like \(x^{-4}\) or more slowly; compact-support or Gaussian smearing does not always give positivity, and the paper states it has no obvious “smeared ANEC conjecture” outside the perturbative context.
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Claims the paper makes
0 of 66 cited sources checked · 0 supported · 0 flagged
- Findingcitation§ C. Gauge freedom and transformations
New 'run-away' solutions exist for the linearized semiclassical Einstein equation.
“and new “run-away” solutions exist.”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [48]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- Findingnone given§ Abstract
Similar results hold for pure states at second order in perturbation theory, when additionally specializing to the situation where incoming classical gravitational radiation does not dominate the first order metric perturbation.
“Similar results hold for pure states at second order in perturbation theory, when we additionally specialize to the situation where incoming classical gravitational radiation does not dominate the first order metric perturbation.”
Quote in the paperNot a substantial claim - Findingreasoning§ III. PERTURBATION THEORY ABOUT FLAT
If ρ̂(1) is a possible first order state perturbation, then −ρ̂(1) is an allowable first order state perturbation if and only if the state is pure to first order.
“In addition, it follows immediately from Eq. (3.19) that if ρ̂(1) is a possible first order state perturbation, then −ρ̂(1) will be an allowable first order state perturbation if and only if the state is pure to first order.”
Quote in the paperSubstantial claim - Findingown data§ Abstract
For mixed states, the ANEC integral can be negative.
“For mixed states, the ANEC integral can be negative.”
Quote in the paperSubstantial claim - Findingreasoning§ II. SEMICLASSICAL GRAVITY WITH
For all values of ξ, the classical ANEC condition holds for all solutions near the trivial solution of Minkowski spacetime with Φ = 0.
“it follows im- mediately from Eq. (2.5) that, for all values of ξ, the classical ANEC condition holds for all solutions near the trivial solution of Minkowski spacetime with Φ = 0.”
Quote in the paperSubstantial claim
- Findingown data§ Abstract
At first order in metric and state perturbations, for pure states of the scalar field, the ANEC integral vanishes.
“At first order in the metric and state perturbations, and for pure states of the scalar field, we find that the ANEC integral vanishes”
- Also stated in: § I. INTRODUCTION AND SUMMARY · plain
“When Eq. (1.1) holds, the ANEC integral always vanishes for pure states at first order in deviation from flatness.”
Quote in the paperSubstantial claim - Also stated in: § I. INTRODUCTION AND SUMMARY · plain
- Findingcitation§ C. Gauge freedom and transformations
The linearized semiclassical Einstein equation has more degrees of freedom than the corresponding classical equation.
“As found in Appendix A and in Ref. [48], the linearized semiclassical Einstein equation has, in effect, more de- grees of freedom than the corresponding classical equa- tion”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [48]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- Findingreasoning§ 1 + x4/Λ4
The smeared ANEC integral with transverse smearing of compact support is not always positive.
“In particular, the smeared ANEC integral with transverse smearing of compact support is not always positive.”
Quote in the paperSubstantial claim - Findingreasoning§ 1 + x4/Λ4
Mixed states at first order in perturbation theory behave very similarly to pure states at second order.
“Roughly speaking, we find that mixed states at first order in per- turbation theory behave very similarly to pure states at second order.”
Quote in the paperNot a substantial claim - Findingreasoning§ III. PERTURBATION THEORY ABOUT FLAT
The perturbed state is pure to first order if and only if P̂ = 0.
“Thus, the perturbed state is pure to first order if and only if P̂ = 0.”
Quote in the paperNot a substantial claim - Findingreasoning§ C. Gauge freedom and transformations
The coefficient a in Eq. (3.32) is positive for all values of ξ.
“Note that the coefficient a is positive for all values of ξ”
Quote in the paperSubstantial claim - Findingreasoning§ 1 − ǫ2ω2
Exact solutions to Eq. (4.20) fail to satisfy the unmodified linearized semiclassical equation (3.38) only by terms of order O(h̄^3).
“the exact solutions to this reduced order equation (4.20) will fail to satisfy the un- modified linearized semiclassical equation (3.38) only by terms of order O(h̄3).”
Quote in the paperSubstantial claim - Findingcitation§ 1 − ǫ2ω2
Eq. (4.19) differs from Eq. (4.4) at order O(τ^2) merely by the term τ^2 ä, which is of the same order of magnitude as the expected corrections to Eq. (4.4) due to finite size effects.
“Eq. (4.19) differs from Eq. (4.4) at order O(τ2) merely by the term τ2ä, which is of the same order of magnitude as the expected corrections to Eq. (4.4) dis- cussed in Sec. IVA above due to the finite size effects”
Quote in the paperSubstantial claim0 of 1 sources checked- cites [88]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- Findingreasoning§ 1 − ǫ2ω2
Different solutions obtained by choosing different Green's functions will all be tangent to the same approximate perturbative solution, in the sense of having the same derivatives with respect to ε at ε=0.
“approximate perturbative solution (in the sense of having”
Quote in the paperNot a substantial claim - Findingreasoning§ C. Gauge freedom and transformations
The free parameters α, β and λ are not independent.
“Therefore the free parameters α, β and λ are not inde- pendent.”
Quote in the paperNot a substantial claim - Findingreasoning§ 2 given by
When the electric field is bounded above, given any initial position and velocity, there exists a unique initial acceleration generating a non-runaway solution.
“generating a non-runaway solution.”
Quote in the paperNot a substantial claim - Findingreasoning§ 1 − ǫ2ω2
They will differ by a function which is smooth in ε, but non-perturbative in ε in the sense that all of its derivatives with respect to ε vanish at ε=0.
“derivatives with respect to ǫ vanish at ǫ = 0.”
Quote in the paperNot a substantial claim - Findingreasoning§ 1 − ǫ2ω2
This correspondence arises because all terms of order O(h̄) which involve h^(1) in the unmodified equation (3.38) are proportional to G^(1)_ab, and thus vanish in the classical limit.
“This very spe- cial situation arises because all terms of order O(h̄) which involve h(1) in the unmodified equation (3.38) are propor- tional to G (1) ab , and, thus, vanish in the classical limit.”
Quote in the paperSubstantial claim - Findingreasoning§ C. Extraction of a preferred subclass of "physical
Under circumstances where Eq. (4.5) is applicable, there are no solutions which are analytic in τ.
“lytic in τ .”
Quote in the paperNot a substantial claim - Findingnone given§ C. Gauge freedom and transformations
The ANEC integral vanishes identically for pure states to first order in deviation from flatness.
“As we have previously indicated, we will find that the ANEC integral vanishes identically for pure states to first order in deviation from flatness.”
Quote in the paperSubstantial claim - Findingnone given§ IV. DEALING WITH THE PATHOLOGICAL
For all ξ, β, and λ except for ξ = 1/6 and λ > λcrit, there exist solutions with spatial wavelength L ≫ Lp which oscillate in time at a frequency of order the Planck frequency.
“In addition, for all ξ, β, and λ except for ξ = 1/6 and λ > λcrit, there exist solutions with spatial wavelength L ≫ Lp which oscillate in time at a frequency of order the Planck frequency.”
Quote in the paperNot a substantial claim - Findingreasoning§ 2 to the solution will give rise
For the one-dimensional heat equation ∂T/∂t = σ ∂^2T/∂x^2, effects non-perturbative in σ are very significant for solutions.
“which are non-perturbative in the”
Quote in the paperNot a substantial claim - Findingown data§ 1 − ǫ2ω2
The series Eq. (4.16) fails to converge for some simple, analytic, very well-behaved choices of ρ, including Gaussian behavior in t.
“haved choices of ρ, including Gaussian behavior in t.”
Quote in the paperSubstantial claim - Findingreasoning§ C. Extraction of a preferred subclass of "physical
For the radiation reaction equation with analytic E independent of position, the series generated by solving order by order in τ is a(t)=Σ_{n=0}^∞ (q/m) τ^n d^n/dt^n E(t).
“order in τ is”
Quote in the paperNot a substantial claim - Findingreasoning§ 1 + |xT |4
The smeared first-order ANEC integral is always nonnegative to order 1/α2 beyond leading order.
“So far we have shown that the smeared, first order ANEC integral is always non-negative to order 1/α2 be- yond leading order.”
Quote in the paperSubstantial claim - Findingreasoning§ VIII. CONCLUSIONS
Apart from the restriction that incoming gravitational radiation does not dominate the first-order metric perturbation, the transversely smeared ANEC integral for nearly flat spacetimes is always strictly positive along every null geodesic in the long wavelength limit, except in the trivial vacuum state in Minkowski spacetime where it vanishes identically.
“Apart from this restriction, we have shown that the transversely smeared ANEC integral for nearly flat spacetimes is al- ways strictly positive along every null geodesic in the long wavelength limit, except in the trivial case of the vacuum state in Minkowski spacetime, where the ANEC integral vanishes identically.”
Quote in the paperSubstantial claim- The authors state this as an assumption: Incoming gravitational radiation does not dominate the first-order metric perturbation.
- Findingreasoning§ C. The first order ANEC integral: general formula
The test-field ANEC integral IF(xT) is smooth.
“We also remark that Eqs. (6.15), (6.16) and (6.30) imply that the function |kT |N F̃(kT ) is L1 for any N , which by Eq. (6.24) shows that the “test field ANEC integral” function IF (xT ) is smooth.”
Quote in the paperSubstantial claim - Findingreasoning§ VII. PURE INCOMING STATES AND THE
κĪ(2)s(ΛT) has the expansion Â/α3 + B̂ lnα/α5 + (Ĉ+∆C)/α5 + O((lnα)2/α7).
“κĪ(2) s (ΛT ) ≡ lim Λ→∞ lim ΛL→0 κI(2) s (Λ,ΛL,ΛT ) =  α3 + B̂ lnα α5 + Ĉ + ∆C α5 +O [ (lnα)2 α7 ] , (7.5)”
Quote in the paperSubstantial claim - Findingreasoning§ C. The first order ANEC integral: general formula
The existence of the integral (6.25) follows from the regularity properties of f^(1) and g^(1): they are continuous away from the light cone and have an integrable divergence ∝ 1/(ω_k ω_k') at the origin.
“The existence of the integral (6.25) follows from the reg- ularity properties of the functions f (1) and g(1) discussed in Appendix C: they are continuous away from the light cone, and have an integrable divergence ∝ 1/(ωkωk′) at the origin.”
Quote in the paperSubstantial claim - Findingreasoning§ C. The first order ANEC integral: general formula
For states whose first-order perturbed two-point function is pure (g(1)=0), the first-order ANEC integral vanishes in the limit Λ→∞ followed by ΛL,ΛT→0.
“We now show that in the limit Λ → ∞, the pure fre- quency contribution to the ANEC integral [the first term in Eq. (6.27)] vanishes.”
- Also stated in: § C. The first order ANEC integral: general formula · plain
“Therefore, when g(1) = 0 we have lim Λ→∞ lim ΛL,ΛT →0 I(1) s (Λ,ΛL,ΛT ) = 0, (6.28)”
Quote in the paperSubstantial claim - Also stated in: § C. The first order ANEC integral: general formula · plain
- Findingreasoning§ C. The first order ANEC integral: general formula
For arbitrary mixed incoming states, the first-order ANEC integral after taking Λ→∞ and ΛL→0 is given by Eq. (6.29).
“Using Eqs. (6.17), (6.19), (6.24) and (6.27) we find that Ī(1) s (ΛT ) ≡ lim Λ→∞ lim ΛL→0 I(1) s (Λ,ΛL,ΛT ) = ∫ d2∆kT (2π)2 F̃(∆kT ) K̃(∆kT ) S̃(ΛT∆kT ), (6.29)”
Quote in the paperSubstantial claim - Findingreasoning§ X. (4.21)
The second term in Eq. (4.22) will still be present unless N → ∞.
“However, the second term will still be present unless we let N → ∞.”
Quote in the paperSubstantial claim- Rests on an assumption: For finite N, the unknown corrections to the right hand side of Eq. (3.38) have the form h̄^2/N L_ab[h^(1)] + h̄^2/N K_ab[ω^(1)_in] + O(h̄^3,1/N^2), where L_ab and K_ab are linear but otherwise unknown functionals.
- Findingreasoning§ VII. PURE INCOMING STATES AND THE
For pure incoming states, the ANEC integral vanishes to O(ε).
“However, for pure in- coming states the ANEC integral vanishes to O(ε), and therefore we need to investigate the second order per- turbation equation (4.23).”
Quote in the paperSubstantial claim - Findingreasoning§ C. The first order ANEC integral: general formula
The second term involving S2 in Eq. (6.18) does not contribute to the ANEC integral (6.29).
“The second term involving S2 in Eq. (6.18) does not contribute to the ANEC integral (6.29), because it has a tensorial structure in momentum space proportional to kakb − ηabk 2. (6.32)”
Quote in the paperSubstantial claim - Findingreasoning§ VII. PURE INCOMING STATES AND THE
The coefficients Â, B̂, and Ĉ have the same functional dependence on ω̄(2)_in as A, B, and C have on ω̄(1)_in.
“Here the coefficients Â, B̂ and Ĉ are functions only of the state perturbation ω̄ (2) in , and have the exact same functional dependence on ω̄ (2) in as the coefficients A, B, and C in Eq. (6.42) have on ω̄ (1) in .”
Quote in the paperNot a substantial claim - Findingnone given§ 1 + |xT |4
There exist states for which ĪF(0) vanishes.
“However, as we now show, there do exist states for which ĪF (0) vanishes, and this opens up possibilities for violations of ANEC.”
Quote in the paperSubstantial claim - Findingreasoning§ 0. Since Q̂ is trace class there will exist an orthonormal
Φ̂′+(λ,0,0)|ψ>^(1)=0.
“It follows that Φ̂′ +(λ, 0, 0) |ψ〉(1) = 0, (7.13)”
Quote in the paperSubstantial claim - Findingreasoning§ 0. Since Q̂ is trace class there will exist an orthonormal
For sufficiently large α, for pure states the transversely smeared ANEC integral is positive.
“Since we showed above that ∆C = 0 whenever = B̂ = 0, we conclude from Eq. (7.5) that for sufficiently large α, for pure states the transversely smeared ANEC integral is positive.”
Quote in the paperSubstantial claim - Findingreasoning§ V. THE GENERALIZED ANEC INTEGRAL
In perturbation theory about flat spacetime, the transversely smeared ANEC integral (5.4) with Λ_T fixed at order Planck length can be chosen so that at each order in ε the quantities depend only on the length Λ_T, the smearing function S, and the choice of parallel propagated null vector ζ^a along γ with ζ^a λ_a = -1.
“In perturbation theory about flat space we can choose N to be the entire spacetime and χ to be unity, and obtain at each order in ε quantities which depend only on (i) the length ΛT , (ii) the smearing function S, and (iii) the choice of parallel propagated null vector ζa along γ with ζaλa = −1.”
Quote in the paperSubstantial claim - Findingreasoning§ 1 + |xT |4
When the transverse smearing length is larger than the critical length (6.45), B is always nonnegative.
“and (ii) From Eq. (6.44), when the transverse smearing length is larger than the critical length (6.45), B is always nonnegative.”
Quote in the paperSubstantial claim - Findingnone given§ 0. Since Q̂ is trace class there will exist an orthonormal
The overall density matrix will be positive to O(ε2) whenever the perpendicular projections of |ψ>^(1) and |ψ>^(2) into the kernel of Q̂ are orthogonal to each other.
“The overall density ma- trix will be positive to O(ε2) whenever the perpendicular projections of |ψ〉(1) and |ψ〉(2) into the kernel of Q̂ are orthogonal to each other.”
Quote in the paperNot a substantial claim - Findingreasoning§ 1. Nonnegativity of the ANEC integral in Minkowski
For all β0, ∫ d2kT ∫ d2k′T ĝ(β0,kT;β0,k′T) ≥ 0.
“∫ d2kT ∫ d2k′ T ĝ(β0,kT ;β0,k ′ T ) ≥ 0, (6.37) for all β0.”
Quote in the paperSubstantial claim - Findingnone given§ 1 + |xT |4
The leading coefficient A is always nonnegative.
“As we have just discussed, the leading coefficient (6.43) is always nonnegative.”
Quote in the paperSubstantial claim - Findingreasoning§ 1 + |xT |4
κĪ(1)s(ΛT) has the expansion A/α3 + B lnα/α5 + C/α5 + O((lnα)2/α7).
“Substituting Eqs. (6.31) and (6.41) into Eq. (6.39) and expanding in 1/α2 yields that κĪ(1) s (ΛT ) = A α3 +B lnα α5 + C α5 +O [ (lnα)2 α7 ] , (6.42)”
Quote in the paperSubstantial claim - Findingreasoning§ X. (4.21)
For finite N, there will be unknown corrections to Eq. (3.38) at the same order O(h̄^2) as terms that were retained.
“in the case of finite N , there will be unknown corrections to Eq. (3.38) at the same order [O(h̄2)] as terms that we have retained.”
Quote in the paperSubstantial claim- Rests on an assumption: For finite N, the unknown corrections to the right hand side of Eq. (3.38) have the form h̄^2/N L_ab[h^(1)] + h̄^2/N K_ab[ω^(1)_in] + O(h̄^3,1/N^2), where L_ab and K_ab are linear but otherwise unknown functionals.
- Findingreasoning§ 1 + |xT |4
There exist incoming states for which B=0.
“However, from Eq. (6.50) it is clear that there exist incoming states for which B = 0; for instance one can choose the function v(xT ) to vanish in a neighborhood of the origin.”
Quote in the paperSubstantial claim - Findingreasoning§ 1 + |xT |4
There exist states for which ĪF(0)=0 but ∇T2 ĪF(0) ≠ 0.
“It is clear that we can find states for which ĪF (0) = 0 but ∇2 T ĪF (0) 6= 0.”
Quote in the paperSubstantial claim - Findingreasoning§ C. The first order ANEC integral: general formula
In the limit of zero backreaction, the ANEC integral in Minkowski spacetime of a matrix element of the form <0|T^(0)_ab|ψ>^(1) must vanish.
“the ANEC integral in Minkowski spacetime of a matrix element of the form 〈0|T̂ (0) ab |ψ〉(1) must vanish;”
Quote in the paperSubstantial claim - Findingreasoning§ V. THE GENERALIZED ANEC INTEGRAL
The vector field v^c must satisfy Eq. (5.5) in order that γ(ε) be a geodesic to order ε.
“This vector field cannot be completely freely specified on γ but must satisfy the equation”
Quote in the paperSubstantial claim - Findingreasoning§ 1 + |xT |4
When A = ĪF(0) = 0, the quantity ∇T2 ĪF(0) is always positive or zero.
“Now when A = ĪF (0) = 0, then the quantity ∇2 T ĪF (0) is always positive or zero.”
Quote in the paperSubstantial claim - Findingown data§ 1 , e
For states in the above class, the stress tensor (3.43) which acts as a source in the semiclassical equations is an L^2 tensor field on Minkowski spacetime.
“In Appendix C we show that for states in the above class the stress tensor (3.43) which acts as a source in the semiclassical equations is an L2 tensor field on Minkowski spacetime.”
Quote in the paperSubstantial claim - Findingreasoning§ 1. Nonnegativity of the ANEC integral in Minkowski
The test-field ANEC integral IF(xT) is always nonnegative for a large class of states.
“We now give a rigorous proof of the positivity of IF (xT ); it follows directly from our general formula (6.34) for IF and the positivity condition on the two point function expressed in our coordinates (β,kT ).”
- Also stated in: § 1. Nonnegativity of the ANEC integral in Minkowski · boosted
“Therefore, from Eqs. (6.30) and (6.34) the quantity IF (0) is nonnegative. It is clear that the same is true for IF (xT ).”
Quote in the paperSubstantial claim0 of 2 sources checked- cites [16]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- cites [18]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- Also stated in: § 1. Nonnegativity of the ANEC integral in Minkowski · boosted
- Findingnone given§ 2. The long wavelength limit
If the incoming state has the form (3.41), the test-field ANEC integral varies as IF(xT;α)=α−3 ĪF(xT/α).
“If we assume an incoming state of the form (3.41), then the test field ANEC integral varies as IF (xT ;α) = α−3ĪF (xT /α), (6.38)”
Quote in the paperSubstantial claim - Findingreasoning§ 1 + |xT |4
ΛT,crit = 8π sqrt(a/ν0) Lp.
“ΛT,crit = 8π √ a ν0 Lp. (6.45)”
Quote in the paperSubstantial claim - Findingreasoning§ 0. Since Q̂ is trace class there will exist an orthonormal
The expression (7.7) should vanish.
“Therefore the expression (7.7) should vanish.”
Quote in the paperSubstantial claim - Findingreasoning§ VII. PURE INCOMING STATES AND THE
The last term in Eq. (7.3) vanishes.
“It is not difficult to see that the last term in Eq. (7.3) vanishes.”
Quote in the paperSubstantial claim - Findingreasoning§ VII. PURE INCOMING STATES AND THE
The O(ε2) contribution to the transversely smeared ANEC integral for solutions to Eq. (4.23) is positive in the long wavelength limit.
“In this section we calculate the O(ε2) contribution (5.19) to the transversely smeared ANEC integral for solutions to Eq. (4.23), and show that it is positive in the long wavelength limit.”
Quote in the paperSubstantial claim - Findingreasoning§ 1 =
Λmin(x0) is bounded above for all x0.
“we conclude that the function Λmin(x0) is bounded above for all x0.”
Quote in the paperSubstantial claim - Findingreasoning§ 1 =
There is some fixed length ΛT such that for the smearing function (6.40), the ANEC integral (B2) is always non-negative.
“We conclude that there is some fixed length ΛT such that for the smearing function (6.40), the ANEC inte- gral (B2) is always non-negative.”
Quote in the paperSubstantial claim - Findingreasoning§ 1 +
The smeared ANEC integral is proportional to ∫ d^2xT IF(xT)[K1 ◦ Sdil](xT), where Sdil(xT)=S(xT/ΛT) and K1◦Sdil is the convolution of K1 and Sdil.
“From Eq. (6.35), the smeared ANEC integral is pro- portional to ∫ d2xT IF (xT )[K1 ◦ Sdil](xT ), (B2) where Sdil(xT ) = S(xT /ΛT ) is a”
Quote in the paperSubstantial claim - Findingreasoning§ 0 and k2 = k2
Solutions in S have the property that their transversely smeared ANEC integral is always non-negative, even outside the long wavelength limit, whenever λ>λcrit.
“We shall show that the solutions in S have the property that their transversely smeared ANEC integral is always non-negative, even outside of the long wavelength limit, whenever λ > λcrit.”
Quote in the paperSubstantial claim - Findingnone given§ 1 =
Violations of ANEC do not occur when λ>λcrit, if the exponentially growing and decaying pieces of the solutions are discarded.
“[It can be shown that violations of ANEC do not occur when λ > λcrit, if we we discard the exponentially growing and de- caying pieces of the solutions.]”
Quote in the paperNot a substantial claim - Findingreasoning§ 1 + (µK)p+1
For a point mass m moving along a geodesic in Minkowski spacetime, the ANEC integral I along a null geodesic with impact parameter ∆T ≠ 0 in the self-consistent solution is I = −6ma/(2π)^4κ |u·λ| 1/∆T^4.
“Using Eqs. (6.17), (D13) and (E5) we obtain for ∆T 6= 0 I = − 6ma (2π)4κ |~u · ~λ| 1 ∆4 T , (E7)”
Quote in the paperNot a substantial claim - Findingreasoning§ 0 and k2 = k2
There are both tachyonlike and exponentially growing modes of this type for all values of λ.
“Thus, there are both tachyonlike and exponentially growing modes of this type for all values of λ.”
Quote in the paperNot a substantial claim - Findingreasoning§ 1 + (µK)p+1
The terms ∆I give a vanishing contribution in the limit K→∞ in Eq. (D3).
“Now it can be seen that these terms give a vanishing contribution in the limit K → ∞ in Eq. (D3).”
Quote in the paperSubstantial claim - Findingreasoning§ 2 log[K2
Lemma: Let h(x) be a non-negative, smooth, L1 function on R2 such that h(0)=h,i(0)=h,ij(0)=h,ijk(0)=0. Then ∫ d2k [∫ d2x e^{ik·x}h(x)] k^2 log(k^2) ≥ 0, with equality iff h≡0.
“Lemma Let h(x) be a non-negative, smooth, L1 function on R2 such that h(0) = h,i(0) = h,ij(0) = h,ijk(0) = 0, (D1) where the commas denote partial derivatives. Then ∫ d2k [∫ d2xeik·xh(x) ] k2 log(k2) ≥ 0, (D2) with equality iff h ≡ 0.”
Quote in the paperSubstantial claim - Findingcitation§ 1 + (µK)p+1
At leading order, in regions where Ψcl,(0) and Ψcl,(1) vanish, the Einstein tensor for this self-consistent solution will be just the test field quantum stress tensor on the classical background, as claimed by Visser.
“At leading order, in regions of the spacetime where Ψcl,(0) and Ψcl,(1) vanish, the Einstein tensor for this self consistent solution will be just the test field quantum stress tensor on the classical background, as claimed by Visser [43].”
Quote in the paperSubstantial claim0 of 1 sources checked- cites [43]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- Findingreasoning§ 1 =
When λ<λcrit, there exist exact solutions outside S which violate ANEC, even when transversely smeared.
“We now show that when λ < λcrit, there exist exact solutions outside of S which violate ANEC, even when transversely smeared.”
Quote in the paperSubstantial claim - Findingnone given§ 0 and k2 = k2
Some exact solutions outside the subclass S do violate ANEC.
“However, we also shall show that some exact solutions outside of this subclass do violate ANEC.”
Quote in the paperSubstantial claim - Findingreasoning§ 1 + (µK)p+1
The original integral (D2) can be written as ∫ dχ ∫ dx h(x,χ)[12π/x^3], which is manifestly positive.
“Thus, from Eq. (D7) the original integral (D2) can be written as ∫ 2π 0 dχ ∫ ∞ 0 dxh(x, χ) [ 12π x3 ] , (D13) which is manifestly positive.”
Quote in the paperSubstantial claim - Findingreasoning§ 1 + (µK)p+1
The ANEC integral is negative along all geodesics away from the point mass in the self-consistent solution.
“Thus, the ANEC integral is negative along all geodesics away from the point mass in the self consistent solution.”
Quote in the paperSubstantial claim - Findingreasoning§ 1 =
A negative I(1) cannot always be made positive by transverse smearing in this case.
“Moreover, it is easy to see that a negative I(1) cannot always be made positive by transverse smearing in this case.”
Quote in the paperNot a substantial claim - Findingreasoning§ 1 +
The expected stress tensor in state (C1) is automatically smooth, from relation (C5) and the smooth initial data for F.
“Now the expected stress tensor in the state (C1) will be automatically smooth, from the relation Tab(x) = Dab F (x, x′) (C5) and the fact that the initial data for F on Σ×Σ is smooth, so that F itself is smooth on M × M .”
Quote in the paperNot a substantial claim- The authors state this as an assumption: The paper assumes that the functions F, ∂F/∂t, ∂F/∂t′, and ∂2F/(∂t∂t′) lie in class V: they are smooth and all their spatial derivatives are L1 on Σ×Σ.
- Findingnone given§ 1 =
If h(1)ab(x;α) is a one-parameter family of exact solutions such that ANEC is violated, then ANEC will still be satisfied order by order in 1/α^2 and lnα/α^2.
“Note that if h (1) ab (x;α) is a one parameter family of exact solutions such that ANEC is violated, then it will still be true that ANEC will be satisfied order by order in 1/α2 and lnα/α2.”
Quote in the paperSubstantial claim - Findingreasoning§ 0 and k2 = k2
The ANEC integral for exact solutions to the unmodified semiclassical equation parallels that in Sec. VI B for the reduced order equation, with S1 and S2 replaced by 1/F1 and F2/F3.
“The analysis of the ANEC integral for the exact solutions to the unmodified semiclassical equation parallels that given in Sec. VI B for the solutions of the reduced order equation, with the only difference being that the functions S1 and S2 of Eqs. (6.19) and (6.20) are replaced by the expressions 1/F1 and F2/F3 respectively”
Quote in the paperSubstantial claim - Findingreasoning§ 1 +
For the choice (6.40) of smearing function, there exists some ΛT>0 such that S(xT/ΛT) satisfies the positive convolution condition.
“We now show that for the choice (6.40) of smearing func- tion, there exists some ΛT > 0 such that the function S(xT /ΛT ) will satisfy the positive convolution condition.”
Quote in the paperSubstantial claim - Premisecitation§ Abstract
The expectation value of the renormalized stress-energy tensor of quantum fields generically violates the classical local positive energy conditions of general relativity.
“The expectation value, 〈Tab〉, of the renormalized stress-energy tensor of quantum fields generically violates the classical, local positive energy conditions of general relativity.”
- Also stated in: § I. INTRODUCTION AND SUMMARY · boosted
“it is well known that quantum fields violate all the local, pointwise energy conditions [6,7].”
Quote in the paperSubstantial claim0 of 2 sources checked- cites [6]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- cites [7]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- Also stated in: § I. INTRODUCTION AND SUMMARY · boosted
- Interpretationnone given§ 0 (M). Then G(f, g)
The vacuum polarization term 〈Tab〉ω0 is a functional of the spacetime metric gab alone.
“The vacuum polarization term 〈Tab〉ω0 is functional of the spacetime metric gab alone.”
Quote in the paperNot a substantial claim - Premisecitation§ II. SEMICLASSICAL GRAVITY WITH
One piece of evidence that this is the case is that this seems to be the only way to escape the conclusion that flat spacetime is unstable [58].
“One piece of evidence that this is the case is that this seems to be the only way to escape the conclusion that flat spacetime is unstable [58].”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [58]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- Interpretationreasoning§ II. SEMICLASSICAL GRAVITY WITH
One formally obtains Eq. (2.6) exactly in the N → ∞ limit.
“Thus, one formally obtains Eq. (2.6) exactly in the N → ∞ limit.”
Quote in the paperNot a substantial claim - Premisecitation§ I. INTRODUCTION AND SUMMARY
ANEC can be violated in generic, curved four-dimensional spacetimes, even if the spacetime is nearly flat.
“However, it has been shown that it can be violated in generic, curved four dimensional spacetimes [18,42], even if the spacetime is nearly flat.”
Quote in the paperSubstantial claim0 of 2 sources checked- cites [18]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- cites [42]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- Interpretationcitation§ I. INTRODUCTION AND SUMMARY
In the second case, there can be macroscopic regions of spacetime in which ANEC is violated.
“In the second case, there can be macroscopic regions of spacetime which ANEC is violated.”
Quote in the paperSubstantial claim - Interpretationreasoning§ 1 + x4/Λ4
The transverse smearing is a crucial ingredient in the analysis.
“Thus, the transverse smearing is a crucial ingredient in our analysis.”
Quote in the paperSubstantial claim - Interpretationreasoning§ 1 + x4/Λ4
Results for pure states do not generalize to mixed states.
“Therefore, results for pure states do not generalize to mixed states.”
Quote in the paperSubstantial claim - Interpretationreasoning§ II. SEMICLASSICAL GRAVITY WITH
In the N → ∞ limit, the fluctuations in the expected total stress-energy tensor of the scalar fields become negligible.
“Furthermore, in the N → ∞ limit, the fluctuations in the expected total stress-energy tensor of the scalar fields becomes negligible.”
Quote in the paperSubstantial claim - Interpretationreasoning§ 1 + x4/Λ4
Even at first order in perturbation theory, positivity of I_s^(1) for all pure states does not imply positivity for mixed states.
“it is not true that pos- itivity of I (1) s for all pure states would imply positivity for mixed states.”
Quote in the paperSubstantial claim - Interpretationreasoning§ II. SEMICLASSICAL GRAVITY WITH
Under the scaling transformation gab → μ^2 gab, we must scale the 2-point function G of the quantum field as G(x, y) → μ^−2 G(x, y) in order to preserve Eq. (2.15) below.
“Under the scaling transforma- tion gab → μ2gab, we must scale the 2-point function, G, of the quantum field as G(x, y) → μ−2G(x, y) in order to preserve Eq. (2.15) below.”
Quote in the paperNot a substantial claim - Interpretationreasoning§ III. PERTURBATION THEORY ABOUT FLAT
For general algebraic states, if ω(1)in is a possible first order state perturbation off a pure state, then −ω(1)in is an allowable first order state perturbation if and only if the perturbed state is pure to first order.
“It should follow that for general algebraic states, if ω (1) in is a possible first order state perturbation off of a pure state, then −ω(1) in will be an allowable first order state perturbation if and only if the perturbed state is pure to first order.”
Quote in the paperSubstantial claim - Interpretationreasoning§ C. The semiclassical equations
States which differ only in their n point functions for n ≠ 2 are effectively identical as far as semiclassical gravity is concerned.
“From this point of view, states which differ only in their n point functions for n 6= 2 are effectively identical as far as semi- classical gravity is concerned.”
Quote in the paperSubstantial claim - Interpretationreasoning§ 0 (M). Then G(f, g)
Under our above assumptions about the asymptotic behavior of states, it follows from Eq. (2.20) that in the asymptotic past F(x, y) approaches the smooth function Fin(x, y) on Minkowski spacetime defined by Fin(x, y) = Gin(x, y) − Gin,0(x, y).
“Under our above assumptions about the asymptotic behavior of states, it follows from Eq. (2.20) that in the asymptotic past F (x, y) approaches the smooth function Fin(x, y) on Minkowski spacetime defined by”
Quote in the paperNot a substantial claim- The authors state this as an assumption: The state is sufficiently regular and the approach to flatness of the spacetime occurs at a sufficiently rapid rate that G(x, y) asymptotically approaches the two-point function Gin(x, y) of a state in Minkowski spacetime.
- Interpretationreasoning§ Abstract
These results suggest that if traversable wormholes do exist as self-consistent solutions of the semiclassical equations, they cannot be macroscopic but must be Planck scale.
“These results suggest — in agreement with conclusions drawn by Ford and Roman from entirely independent arguments — that if traversable wormholes do exist as self-consistent solutions of the semiclassical equations, they cannot be macroscopic but must be”
Quote in the paperSubstantial claim - Premisereasoning§ II. SEMICLASSICAL GRAVITY WITH
In four dimensions, most backreaction calculations have been restricted to linear order perturbation theory off some fixed background (except for analyses of various conformally flat spacetimes [36,47]).
“However, in four dimensions, most backreaction calculations have been re- stricted to linear order perturbation theory off some fixed background (except for analyses of various conformally flat spacetimes [36,47]).”
Quote in the paperSubstantial claim0 of 2 sources checked- cites [36]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- cites [47]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- Interpretationreasoning§ I. INTRODUCTION AND SUMMARY
If the semiclassical equations were to enforce the positivity of a transversely smeared ANEC integral in general spacetimes, with a smearing width of order of the Planck length, this would provide almost as strong a constraint on physical possibilities as the positivity of the ANEC integral itself.
“Consequently, if the semiclassical equations were to enforce the positivity of a transversely smeared ANEC integral in general spacetimes, with a smearing width of order of the Planck length, this would provide almost as strong a constraint on physical possibilities as the positivity of the ANEC integral itself.”
Quote in the paperSubstantial claim - Premisecitation§ II. SEMICLASSICAL GRAVITY WITH
There exist pathological runaway-type solutions to the semiclassical equations, as analyzed in detail by Horowitz [48] for the linearized equations.
“In addition there exist pathological runaway- type solutions to these equations, as analyzed in detail by Horowitz [48] for the linearized equations.”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [48]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- Interpretationreasoning§ 1 + x4/Λ4
Pure states and mixed states behave qualitatively very differently in this analysis.
“Here, however, it turns out that pure states and mixed states behave qualitatively very differently.”
Quote in the paperSubstantial claim - Interpretationreasoning§ II. SEMICLASSICAL GRAVITY WITH
An important feature of 〈T̂ab〉 is that it has an anomalous behavior under a scaling of the spacetime metric and the corresponding scaling transformation of the state.
“An important feature of 〈T̂ab〉 is that it has an anoma- lous behavior under a scaling of the spacetime metric and the corresponding scaling transformation of the state.”
Quote in the paperNot a substantial claim - Interpretationreasoning§ 0 (M). Then G(f, g)
The positivity condition will hold for G(x, y) if and only if it holds for Gin(x, y).
“Note that the positivity con- dition will hold for G(x, y) if and only if it holds for Gin(x, y).”
Quote in the paperNot a substantial claim - Interpretationnone given§ 1 + x4/Λ4
The space of allowed state perturbations ω_in^(1) is the tangent space T_vac(D) to D at ω0 = |0><0|, not D.
“the space of allowed state perturbations ω (1) in is not D but is the tangent space Tvac(D) to D at ω0 = |0〉 〈0|.”
Quote in the paperSubstantial claim - Premisecitation§ 0 (M). Then G(f, g)
For massless fields, 〈Tab〉ω0 has been evaluated by Horowitz [48] to first order in the perturbed metric about flat spacetime.
“For massless fields, it has been evaluated by Horowitz [48] to first order in the perturbed metric about flat spacetime”
Quote in the paperSubstantial claim0 of 1 sources checked- cites [48]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- Interpretationreasoning§ II. SEMICLASSICAL GRAVITY WITH
Corrections to this equation should be of order 1/N or higher.
“Correc- tions to this equation should be of order 1/N or higher.”
Quote in the paperNot a substantial claim - Interpretationreasoning§ II. SEMICLASSICAL GRAVITY WITH
In the semiclassical theory, one is forced to introduce a lengthscale, λ0, in the prescription for defining 〈T̂ab〉.
“However, the situation is quite different in the semiclassical the- ory because one is forced to introduce a lengthscale, λ0, in the prescription for defining 〈T̂ab〉.”
Quote in the paperNot a substantial claim - Interpretationnone given§ I. INTRODUCTION AND SUMMARY
The positivity of smeared ANEC would restrict the amount of violation to be incredibly small compared to the distant, positive mass.
“In this second case, however, the positivity of smeared ANEC would restrict the amount of violation to be incredibly small compared to the distant, positive mass.”
Quote in the paperSubstantial claim - Premisecitation§ C. Gauge freedom and transformations
The corresponding coefficient for other fields such as Maxwell and neutrino fields is also positive.
“and moreover the corresponding coefficient for other fields such as Maxwell and neutrino fields is also positive [48].”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [48]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- Premisecitation§ 1 + x4/Λ4
The analog of the first-order pure-state vanishing result fails to hold when the semiclassical Einstein equation is not imposed.
“As was already mentioned in the previous subsection, the analog of result (i) fails to hold when the semiclassical Einstein equation is not imposed.”
Quote in the paperSubstantial claim0 of 1 sources checked- cites [18]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- Premisenone given§ II. SEMICLASSICAL GRAVITY WITH
Our backreaction analysis is apparently the first to go beyond linear order perturbation theory for a generic class of four dimensional spacetimes.
“Our backreaction analysis is ap- parently the first to go beyond linear order perturbation theory for a generic class of four dimensional spacetimes.”
Quote in the paperNot a substantial claim - Premisenone given§ C. The semiclassical equations
In free field theory, the evolution of the two-point function is decoupled from that of the higher n-point functions.
“Moreover, in free field theory (which we are considering here) the evolution of the two-point function is decou- pled from that of the higher n-point functions.”
Quote in the paperSubstantial claim - Interpretationreasoning§ III. PERTURBATION THEORY ABOUT FLAT
The positivity condition, Eq. (2.16), applied to both ωin,0 + εω(1)in and ωin,0 − εω(1)in implies the vanishing of the mixed-frequency part of the two-point function for general first-order pure states.
“In addition, the positivity condition, Eq. (2.16), applied to both ωin,0 + εω (1) in and ωin,0 − εω (1) in should then imply the vanishing of the mixed-frequency part of the two-point function for general first-order pure states.”
Quote in the paperSubstantial claim - Interpretationreasoning§ IV. DEALING WITH THE PATHOLOGICAL
The limit L→0 for fixed mass m and charge q is unphysical.
“for fixed mass m and charge q is unphysical.”
Quote in the paperSubstantial claim - Interpretationreasoning§ 2 to the solution will give rise
Approximate perturbative solutions similar to Eq. (4.7) to any finite order in hbar will not be adequate to describe phenomena such as evaporation of a black hole over timescales long enough for the black hole to lose a significant fraction of its initial mass.
“not be adequate to describe such phenomena as the evap-”
Quote in the paperSubstantial claim - Interpretationcitation§ IV. DEALING WITH THE PATHOLOGICAL
In the special case of perturbation theory about Minkowski spacetime, Simon's 'reduction of order' proposal yields a satisfactory prescription for extracting physical predictions from the semiclassical equations.
“However, we also will argue that in the special case of perturbation theory about Minkowski spacetime, Simon's “reduction of order” proposal [36] yields a sat- isfactory prescription for extracting physical predictions from the semiclassical equations.”
Quote in the paperSubstantial claim0 of 1 sources checked- cites [36]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- Interpretationreasoning§ 1 − ǫ2ω2
To see the dominant curvature-related contributions to ANEC at small curvatures and long wavelengths, one must go to second order in h̄.
“In order to see these effects – and, thus, the dominant curvature-related contributions to ANEC at small curva- tures and long wavelengths – we must go to second order in h̄.”
Quote in the paperSubstantial claim - Interpretationreasoning§ 1 − ǫ2ω2
The criterion of perturbative expandability is of very limited applicability.
“pandability is of very limited applicability.”
Quote in the paperNot a substantial claim - Interpretationreasoning§ C. Extraction of a preferred subclass of "physical
The criterion of perturbative expandability fails in the case of smooth but non-analytic E.
“fails in the case of smooth but non-analytic E.”
Quote in the paperNot a substantial claim - Interpretationreasoning§ IV. DEALING WITH THE PATHOLOGICAL
All physical finite distributions of charge satisfy L >~ cτ, assuming only that the electromagnetic self energy ~ q^2/L cannot exceed the externally measured mass-energy mc^2.
“all physical, finite distributions of charge satisfy”
Quote in the paperNot a substantial claim- The authors state this as an assumption: The electromagnetic self energy ~ q^2/L cannot exceed the externally measured mass-energy mc^2, i.e., the bare mass for a finite distribution of charge is always positive.
- Interpretationnone given§ C. Gauge freedom and transformations
The long-wavelength limit is equivalent to a h̄→0 limit, as long as the lengthscale λ is taken to scale proportionally to Lp.
“However, we remark that this limit is equiv- alent to a limit in which h̄ = L2 p → 0 with L and λ/Lp fixed, i.e., the long-wavelength limit is equivalent to a h̄→ 0 limit, as long as the lengthscale λ is taken to scale proportionally to Lp.”
Quote in the paperNot a substantial claim - Interpretationnone given§ 2 given by
There are situations where Eq. (2.6) may predict large deviations from classical behavior even though L ≫ Lp everywhere.
“from classical behavior even though L ≫ Lp everywhere.”
Quote in the paperSubstantial claim - Interpretationreasoning§ C. Extraction of a preferred subclass of "physical
Consequently, the series which attempts to define the perturbatively expandable solutions cannot converge.
“pandable”
Quote in the paperSubstantial claim - Interpretationreasoning§ 1 − ǫ2ω2
When ρ̃ fails to be of compact support in ω, it appears that there do not exist any perturbatively expandable solutions to Eq. (4.13).
“that there do not exist any perturbatively expandable so-”
Quote in the paperNot a substantial claim - Interpretationreasoning§ 2 given by
Eq. (4.8) should be a poor approximation whenever radiation reaction has any significant effect upon the motion of the particle.
“any significant effect upon the motion of the particle.”
Quote in the paperNot a substantial claim - Interpretationreasoning§ 1 − ǫ2ω2
Since the unmodified equation (4.4) has unknown corrections at order O(τ^2), the modified radiation reaction equation (4.19) gives a description of the motion whose expected accuracy in the regime τ* ≫ τ is just as high as that of the original equation (4.4).
“the modified radiation reaction equation (4.19) gives a description of the mo- tion whose expected accuracy in the regime τ∗ ≫ τ is just as high as that of the original equation (4.4).”
Quote in the paperSubstantial claim - Interpretationreasoning§ 2 to the solution will give rise
Approximate perturbative solutions (4.7) to any finite order are completely inadequate for describing such phenomena.
“tions (4.7) to any finite order are completely inadequate”
Quote in the paperSubstantial claim - Interpretationown data§ C. Extraction of a preferred subclass of "physical
The criterion of perturbative expandability appears to fail much more dramatically when at least some additional degrees of freedom are oscillatory, as is the case for the semiclassical equations.
“to fail much more dramatically when (at least some of)”
Quote in the paperNot a substantial claim - Interpretationreasoning§ 2 given by
In semiclassical QED, a one-particle nonrelativistic electron state is effectively a finite distribution of charge with width L ~ cτ/α, where α is the fine structure constant.
“width L ∼ cτ/α, where α is the fine structure constant,”
Quote in the paperNot a substantial claim- Rests on an assumption: In semiclassical QED, the expected value of the current operator will not be concentrated at a point but will typically have a width of order L.
- Interpretationreasoning§ IV. DEALING WITH THE PATHOLOGICAL
The additional degrees of freedom admitted by the semiclassical equations are merely artifacts of the semiclassical approximation.
“From this point of view, the additional degrees of free- dom admitted by the semiclassical equations are merely artifacts of the semiclassical approximation.”
Quote in the paperSubstantial claim- The authors state this as an assumption: The semiclassical equations are approximate equations with domain of validity L ≫ Lp.
- Interpretationnone given§ IV. DEALING WITH THE PATHOLOGICAL
Semiclassical theory should be able to accurately describe phenomena where the deviations from classical behavior are locally small, but where long term cumulative effects result in very large global deviations from classical solutions.
“Semiclassical theory should be able to accurately describe phenomena where the deviations from classical behavior are locally small, but where, nevertheless, long term cumulative effects re- sult in very large global deviations from classical solu- tions.”
Quote in the paperNot a substantial claim - Interpretationnone given§ 1 − ǫ2ω2
In more general situations, even for linear equations, solutions to reduced order equations will differ significantly from approximate perturbative solutions.
“In more general situations, even for linear equations, solu- tions to reduced order equations will differ significantly from approximate perturbative solutions.”
Quote in the paperNot a substantial claim - Interpretationreasoning§ 1 − ǫ2ω2
The problem of pathological solutions can be overcome by adopting Eq. (4.19) as the equation of motion.
“We conclude that, in this case, the problem of pathological solutions can therefore be over- come by adopting Eq. (4.19) as the equation of motion.”
Quote in the paperSubstantial claim - Interpretationreasoning§ 2 to the solution will give rise
Even if the equation being considered is itself valid only to first order in some small parameter, it can occur that solutions which are non-perturbative in this parameter are physically meaningful.
“non-perturbative in this parameter are physically mean-”
Quote in the paperSubstantial claim - Interpretationreasoning§ 2 given by
The equations for x^(j)(t) for all j>1 are completely ambiguous because of the unknown correction terms appearing in Eq. (4.4).
“are completely ambiguous because”
Quote in the paperNot a substantial claim - Interpretationreasoning§ 2 given by
In generic situations, the higher order corrections x^(j)(t) for j≥2 will be sensitive to the unknown higher order corrections to the equation of motion, and therefore only the approximate solution (4.8) will be physically meaningful.
“fore only the approximate solution (4.8) will be physically”
Quote in the paperSubstantial claim - Interpretationnone given§ 2 to the solution will give rise
Given an equation of motion whose range of validity restricts a correction term to be locally very small, there can nevertheless be a wide range of circumstances where this equation can reliably predict phenomena where this correction term is responsible for producing large deviations from the uncorrected motion.
“reliably predict phenomena where this correction term is”
Quote in the paperNot a substantial claim - Interpretationreasoning§ 1 − ǫ2ω2
In situations where solutions do differ and where the reduction of order procedure can be justified, solutions of the reduced order equations should give a much better description of physical phenomena than approximate perturbative solutions.
“solutions of the reduced order equations should give a much better description of physical phenomenon than approximate perturbative solutions.”
Quote in the paperNot a substantial claim - Interpretationnone given§ C. Extraction of a preferred subclass of "physical
When ρ̃ is of compact support, Eq. (4.15) yields the unique perturbatively expandable solution to Eq. (4.13).
“batively expandable”
Quote in the paperNot a substantial claim - Interpretationreasoning§ 1 + |xT |4
The sign of the coefficient a determines the sign of the coefficient B without smearing.
“Note that the sign of the coefficient a in the formula (2.10) for the anomalous scaling of the stress energy de- termines the sign of the coefficient B without smearing.”
Quote in the paperSubstantial claim - Interpretationreasoning§ C. The first order ANEC integral: general formula
Any nonzero first-order contribution for pure states could be arranged to be negative by choosing the sign of the first-order state perturbation appropriately.
“any nonzero first order contribution for pure states could be arranged to be negative by choosing the sign of the first order state perturbation appropriately.”
Quote in the paperSubstantial claim - Interpretationreasoning§ C. Second order vacuum polarization
If the condition on the second-order vacuum polarization term is satisfied, then without assumptions restricting incoming classical gravitational radiation, the transversely smeared ANEC integral is always nonnegative for solutions of the reduced-order equations, for general non-vacuum incoming states, in the long wavelength limit.
“Moreover, if the condition is satisfied, then it can be shown that without any assumptions restricting the incoming classical gravitational radiation, that the trans- versely smeared ANEC integral is always nonnegative for solutions of the reduced order equations, for general, non- vacuum incoming states, in the long wavelength limit.”
Quote in the paperSubstantial claim - Interpretationreasoning§ X. (4.21)
One can only justify going to order h̄^2 (or higher) in the reduction of order procedure in the context of the 1/N limit.
“we can only justify going to order h̄2 (or higher) in the reduction of order procedure in the context of the 1/N limit.”
Quote in the paperSubstantial claim - Premisecitation§ 1. Nonnegativity of the ANEC integral in Minkowski
The ANEC integral of the expected value of T^(0)_ab in Minkowski spacetime is nonnegative for a large class of states.
“From previous analyses by Klinkhammar [16] and by Wald and Yurtsever [18], it is known that the test field ANEC integral IF (xT ) is always nonnegative for a large class of states.”
Quote in the paperSubstantial claim0 of 2 sources checked- cites [16]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- cites [18]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- Interpretationreasoning§ C. The first order ANEC integral: general formula
The result that the ANEC integral vanishes to first order for pure incoming states eliminates the counterexample to ANEC given in Ref. [18].
“It eliminates the counterexample to ANEC given in Ref. [18].”
Quote in the paperSubstantial claim0 of 1 sources checked- cites [18]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- Interpretationown data§ VIII. CONCLUSIONS
The results are evidence in favor of the conjecture that ANEC comes sufficiently close to holding in general solutions of the semiclassical equations to rule out macroscopic traversable wormholes.
“Therefore, we consider our results to be evidence in favor of the conjecture that ANEC comes sufficiently close to holding in general solutions of the semiclassical equations to rule out macroscopic traversable wormholes.”
Quote in the paperSubstantial claim - Interpretationreasoning§ X. (4.21)
The 1/N limit is still necessary even if the incoming gravitational radiation does not dominate the first order metric perturbation.
“The 1/N limit is still necessary even if we specialize to the situ- ation, discussed in Sec. III E above, that the incoming gravitational radiation does not dominate the first order metric perturbation.”
Quote in the paperSubstantial claim- Rests on an assumption: For finite N, the unknown corrections to the right hand side of Eq. (3.38) have the form h̄^2/N L_ab[h^(1)] + h̄^2/N K_ab[ω^(1)_in] + O(h̄^3,1/N^2), where L_ab and K_ab are linear but otherwise unknown functionals.
- Interpretationreasoning§ X. (4.21)
Only when the reduction of order procedure simultaneously eliminates all higher order time and space derivatives is it likely to yield an equation with satisfactory mathematical properties.
“it is only in the happy circumstance — such as in the case of Eq. (3.38) — where the reduction of order procedure simultaneously eliminates all of the higher order time and space derivatives that this procedure is likely to yield an equation with satisfactory mathematical properties.”
Quote in the paperNot a substantial claim - Interpretationreasoning§ 1 , e
Consequently its spacetime Fourier transform exists as an L^2 function.
“Consequently its spacetime Fourier transform exists as an L2 function.”
Quote in the paperSubstantial claim - Interpretationreasoning§ C. The first order ANEC integral: general formula
The vanishing of the ANEC integral to first order is a necessary condition for the ANEC integral to be positive generally.
“Moreover, the vanishing of the ANEC integral to first order is a necessary condition for the ANEC integral to be positive generally;”
Quote in the paperSubstantial claim - Interpretationreasoning§ C. The first order ANEC integral: general formula
The result for pure states extends to all orders in hbar, i.e., to solutions of reduced-order equations accurate to higher order in hbar.
“However, it is straightforward to extend this result to all orders in h̄, that is, to solutions of reduced order equations which are accurate to higher order in h̄.”
Quote in the paperNot a substantial claim - Interpretationreasoning§ 1 + (µK)p+1
Therefore, the approximate self-consistent solution obtained from the above scheme starting from a compact star and a test field in the static vacuum state should violate ANEC over macroscopically large regions far from the star.
“Therefore, the approximate self consistent solution obtained from the above scheme starting from a compact star and a test field in the static vacuum state should violate ANEC over macroscopically large regions far from the star.”
Quote in the paperSubstantial claim - Interpretationreasoning§ 1 +
The fact that K1 is negative for some values of its argument implies that there are incoming states for which the ANEC integral including backreaction is negative.
“The fact that this function is negative for some values of its argument implies that there are incoming states for which the ANEC integral including backreaction is negative.”
Quote in the paperSubstantial claim - Interpretationreasoning§ 1 + (µK)p+1
Since ∆ >∼ L, M+ >∼ 10^130 M⊙ (L/1 cm)^5.
“Since the distance ∆ to the positive mass region should be >∼ L, we obtain M+ >∼ 10130M⊙(L/1 cm)5, which is a ridiculuously large mass.”
Quote in the paperSubstantial claim- Rests on an assumption: The distance ∆ to the positive mass region is at least of order L.
- Interpretationreasoning§ 1 + (µK)p+1
In order of magnitude, the paper's result implies M− + (Lp/∆)^4 M+ ≥ 0.
“Then, in order of magnitude, our result implies that M− + ( Lp ∆ )4 M+ ≥ 0. (E9)”
Quote in the paperSubstantial claim - Interpretationreasoning§ 1 + (µK)p+1
The paper's results are consistent with having negative ANEC integrals over a macroscopic region.
“This example illustrates that our results are consistent with having negative ANEC integrals over a macroscopic region.”
Quote in the paperSubstantial claim - Interpretationreasoning§ 1 + (µK)p+1
Therefore M+ >∼ (∆/Lp)^4 L.
“and therefore M+ >∼ ( ∆ Lp )4 L.”
Quote in the paperSubstantial claim - Interpretationreasoning§ 1 +
Since IF(xT) is positive, to make the integral (B2) positive it suffices to find smearing functions whose convolutions with K1 are pointwise positive everywhere.
“Since we know IF (xT ) is positive, to make the integral (B2) positive it suffices to find smearing functions whose convolutions with K1 are pointwise positive everywhere.”
Quote in the paperSubstantial claim - Premisenone given§ 1 + (µK)p+1
The Boulware vacuum outside a Schwarzschild black hole is unphysical because the expected stress tensor diverges on the horizon.
“This state is unphysical because the expected stress ten- sor diverges on the horizon.”
Quote in the paperSubstantial claim - Interpretationreasoning§ 0 and k2 = k2
The perturbative series up to any finite order should coincide with what would be obtained by carrying the reduction of order procedure to the appropriate order and solving exactly the new reduced order equation.
“This perturbative series up to any finite order also should coincide with what would be obtained by carrying the reduction of order procedure of the semiclassical equation to the appropriate order in 1/α2 and solving exactly the new, reduced order equa- tion.”
Quote in the paperSubstantial claim - Interpretationreasoning§ 1 + (µK)p+1
The amount of ANEC violation is restricted to be very small compared to distant mass scales.
“The price one must pay is that the amount of ANEC violation is restricted to be very small compared to distant mass scales.”
Quote in the paperSubstantial claim - Interpretationreasoning§ 1 + (µK)p+1
These examples satisfy the paper's smeared version of ANEC provided only that the stress-energy of the classical matter itself satisfies ANEC.
“these examples satisfy our smeared version of ANEC provided only that stress-energy of the classical matter itself satisfies ANEC.”
Quote in the paperSubstantial claim - Interpretationreasoning§ 0 and k2 = k2
An expansion in 1/α^2 and lnα/α^2 of the positivity result of Appendix B provides an alternative proof of the results established in Sec. VI for solutions of the reduced order equation (4.20), at least for λ>λcrit.
“Thus, an expansion in 1/α2 and lnα/α2 of the positivity result of this appendix provides an alternative proof of the results we established in Sec. VI above for the solutions of the reduced order equation (4.20), at least for λ > λcrit.”
Quote in the paperNot a substantial claim
- Classified as probably not a substantial claim. 193
- May combine two claims. 97
- The quote only partly states this claim. 18
Classified as probably not a substantial claim. May combine two claims.
Findingreasoning§ II. SEMICLASSICAL GRAVITY WITHPathological solutions of the linearized version of Eq. (2.6) exist on scales L ∼ L_p,eff, and we will not regard these solutions as being physical.
“As we shall see in de- tail in Appendix A below, pathological solutions of the linearized version of Eq. (2.6) exist on scales L ∼ Lp,eff , and we will not regard these solutions as being physical.”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Findingnone given§ III. PERTURBATION THEORY ABOUT FLATFor a fixed metric gab, the state ω is a linear function of ωin.
“Note that for a fixed metric gab, the state ω is a linear function of ωin.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S4 (based).
Findingnone given§ III. PERTURBATION THEORY ABOUT FLATFor states in the usual Fock space, a perturbed state will be pure to first order if and only if its perturbed two-point function is pure (i.e., its mixed-frequency part vanishes).
“For states in the usual Fock space – and, presumably, also for general algebraic states – a perturbed state will be pure to first order if and only if its perturbed two-point function is pure.”
Quote in the paperNot a substantial claimMay combine two claims.
Findingreasoning§ II. SEMICLASSICAL GRAVITY WITHIn the classical theory, the stress tensor violates the pointwise null energy condition for ξ ≠ 0, but satisfies the averaged null energy condition for all negative values of ξ, provided that suitable asymptotic fall-off conditions hold for Φ.
“In the classical theory, this stress tensor violates the pointwise null energy condition for ξ 6= 0, but satisfies the averaged null energy condition for all negative val- ues of ξ, provided that suitable asymptotic fall-off con- ditions hold for Φ.”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Findingcitation§ 1 − ǫ2ω2If one introduces a new variable y=y(x;τ), rewrites Eq. (4.18) as an equation for y, and neglects terms of order τ^2 and higher, the resulting reduced order equation for y need not be precisely equivalent to the reduced order equation for x.
“not be precisely equivalent to the reduced order equation”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [87]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
May combine two claims.
Findingreasoning§ 1 − ǫ2ω2The modified equation of motion (4.19) is formally equivalent to Eq. (4.4) up to order O(τ), and differs from it at order O(τ^2).
“This modified equation of motion is formally equivalent”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S3 (load-bearing). The quote only partly states this claim.
Findingnone given§ 1 − ǫ2ω2The final reduced order equation is uniquely determined by the requirements (i) it contains only terms zeroth or first order in τ, (ii) it is formally equivalent to Eq. (4.18) to O(τ^2), and (iii) it is of form (4.18) where the right hand side contains no time derivatives of order higher than n−1.
“should contain only terms that are zeroth order or first”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Findingreasoning§ 1 − ǫ2ω2Although h̄ was formally treated as the small parameter, one could equivalently have started from Eq. (3.45) and used 1/α^2 instead.
“although we have formally treated h̄ as the small parameter, we could equivalently have started from Eq. (3.45) and used 1/α2 instead”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Findingreasoning§ C. Extraction of a preferred subclass of "physicalThis series is precisely the expansion in τ of the non-runaway solution, the second term in Eq. (4.5).
“solution [the second term in Eq. (4.5)].”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Findingreasoning§ 1 − ǫ2ω2Eq. (4.19) suffers from none of the problems of the original equation.
“However, Eq. (4.19) suffers from none of the prob- lems of the original equation.”
Quote in the paperNot a substantial claimMay combine two claims.
Findingreasoning§ 1 − ǫ2ω2Eq. (4.20) is second order in time and has the form of the classical linearized Einstein equation with a given source.
“This modified equation is second order in time and simply has the form of the classical linearized Einstein equation with a given source.”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Findingreasoning§ 1 − ǫ2ω2Iterating the reduction of order procedure until the maximum number of time derivatives in Q is reduced to n−1 yields an equation of the same differential order in time as the original equation with τ=0.
“tion Eq. (4.18) with τ = 0.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing). The quote only partly states this claim.
Findingcitation§ 1 − ǫ2ω2By following the reduction of order steps for the radiation reaction equation, one obtains Eq. (4.19).
“obtains the equation [82,83]”
Quote in the paperNot a substantial claim0 of 2 sources checked- cites [82]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- cites [83]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
Classified as probably not a substantial claim.
Findingnone given§ 1 − ǫ2ω2The quantity λ/L_p in Eq. (4.20) is a h̄-independent constant.
“the quantity λ/Lp in Eq. (4.20) is a h̄-independent constant.”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Findingreasoning§ 1 − ǫ2ω2For the linearized semiclassical Einstein equation (3.38), the reduction of order procedure could be ambiguous because integration by parts may alter the apparent differential order of terms in an integrand.
“In general, the reduction of order procedure could be ambiguous for such equations, since it may be possible to alter the apparent differential order of terms in an inte- grand via integration by parts.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing). The quote only partly states this claim.
Findingreasoning§ 1 − ǫ2ω2The reduced order equation obtained from Eq. (3.38) to order h̄^2 is Eq. (4.20).
“the resulting reduced order equation is”
Quote in the paperNot a substantial claimClassified as probably not a substantial claim.
Findingreasoning§ 1 − ǫ2ω2Applying the refined reduction of order algorithm to Eq. (3.38) to order h̄^2 corresponds to substituting h̄ s_ab/κ for G^(1)_ab everywhere on the right hand side of Eq. (3.38), where s_ab ≡ D^(0)_ab F^(1)_in.
“This corresponds to substituting h̄sab/κ for G (1) ab everywhere on the right hand side of Eq. (3.38), where sab ≡ D(0) ab F (1) in .”
Quote in the paperSubstantial claimMay combine two claims.
Findingcitation§ 2 given byThere is no problem with runaway effects in constructing approximate solutions x_J, and for any given order J, an initial position and velocity determine a unique approximate solution x_J, unlike the exact solutions.
“velocity will determine a unique approximate solution xJ”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [75]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
The quote only partly states this claim.
Findingcitation§ 2 to the solution will give riseContributions of order τ2^2 to the solution give small corrections to the inspiral of relative magnitude <~ τ/τp, where τp ≫ τ is the initial orbital period.
“to small corrections to the inspiral of relative magnitude”
Quote in the paperNot a substantial claim- The authors state this as an assumption: The exact equation of motion including all higher order corrections is of the form a = a_ext + τ1 ȧ + α1 τ2^2 ä.
May combine two claims.
Findingreasoning§ 1 − ǫ2ω2All solutions of Eq. (4.19) are well behaved, i.e., there are no runaway solutions nor any preacceleration effects.
“All of its solutions are well behaved, i.e, there are no runaway solutions nor any pre- acceleration effects.”
Quote in the paperSubstantial claimClassified as probably not a substantial claim.
Findingreasoning§ 1 − ǫ2ω2The equation obtained by substituting G^(1)_ab = 0 on the right hand side of Eq. (3.38) is too trivial in that it does not incorporate any effects of the curved spacetime.
“However, the resulting equation is too trivial in that it does not incorporate any of the effects of the curved spacetime.”
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Findingreasoning§ 2 given byIf the electric field E is of compact support in time, the runaway solutions of Eq. (4.4) have ẍ ∝ exp(t/τ) for large t.
“the property that ẍ ∝ exp(t/τ) for large t.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Findingown data§ C. Gauge freedom and transformationsIn Appendix A we obtain all solutions to Eq. (3.38) whose spatial Fourier transforms exist, thereby generalizing the analysis of Horowitz to allow for a non-vacuum incoming quantum state.
“In Appendix A we obtain all solutions to Eq. (3.38) whose spatial Fourier transforms exist, thereby generalizing the analy- sis of Horowitz to allow for a non-vacuum incoming quan- tum state.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Findingreasoning§ 1 − ǫ2ω2The refined reduction of order procedure can be generalized to any finite order in τ.
“Clearly, this procedure can be generalized to any finite order in τ .”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing). May combine two claims.
Findingreasoning§ 1 − ǫ2ω2The reduction of order algorithm produces a new equation formally equivalent to Eq. (4.18) to order τ and with the same general form, but where Q contains at most m−1 time derivatives of x.
“the role of Q now contains at most (m− 1) time deriva-”
Quote in the paperNot a substantial claimClassified as probably not a substantial claim.
Findingreasoning§ 1 − ǫ2ω2Since the right hand side of Eq. (3.38) involves only derivatives of the linearized Einstein tensor, there is an obvious procedure for obtaining a reduced order equation valid to order h̄: substitute G^(1)_ab = 0 on the right hand side of Eq. (3.38).
“since the right hand side of Eq. (3.38) involves only derivatives of the linearized Einstein tensor, there is an obvious procedure in this case for obtaining a reduced order equation valid to order h̄”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Findingreasoning§ 2 given byThe choice of initial acceleration a0 that makes the first term in Eq. (4.5) vanish is the unique choice generating a non-runaway solution.
“unique choice which generates a non-runaway solution.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Findingreasoning§ 2 given byNon-runaway solutions of Eq. (4.4) form a 6-dimensional submanifold of the 9-dimensional manifold of solutions, since they have vanishing acceleration at late times for E of compact support in time.
“dimensional submanifold of the 9-dimensional manifold”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Findingreasoning§ 1 − ǫ2ω2For a one-parameter family of electric fields E(x,t;α)=α^{-2}E_0(x,t/α) and X(t;α)=x(αt;α), X satisfies Eq. (4.21).
“If we consider a one parameter family of electric fields given by E(x, t;α) = α−2E0(x, t/α) and define X(t;α) = x(αt;α), then X satisfies the differential equation”
Quote in the paperNot a substantial claimThe quote only partly states this claim.
Findingreasoning§ 1 − ǫ2ω2If ρ̃(ω) is of compact support in ω, then ginhom(t;ε) is analytic in ε.
“ginhom(t; ǫ) is analytic in ǫ.”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Findingreasoning§ ACKNOWLEDGMENTSF1(k) can be written as the limit of a function G1(k,ω) analytic on the upper half ω plane.
“From Eqs. (6.17) and (A6) we can write F1 as the limit of a function analytic on the upper half ω plane: F1(k) = limǫ→0+ G1(k, ω + iǫ)”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Findingreasoning§ 1 , eThe reduced order semiclassical equation (4.20) expresses the linearized Einstein tensor G^(1)_ab[h^(1)] in terms of the source tensor (3.43).
“The reduced order semiclassical equation (4.20) ex- presses the linearized Einstein tensor G (1) ab [h(1)] in terms of the source tensor (3.43).”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Findingreasoning§ C. Expansion of the generalized ANEC integralIn the limit Λ→∞, Λ_L,Λ_T→0 of no transverse smearing, expression (5.19) reduces to expression (5.11), since h^(1)e_e vanishes on γ in the chosen gauge.
“in the limit Λ → ∞, ΛL,ΛT → 0 of no transverse smearing, the expression (5.19) reduces to the previously obtained expression (5.11), since h (1) e e vanishes on γ in our chosen gauge.”
Quote in the paperNot a substantial claimClassified as probably not a substantial claim. May combine two claims.
Findingreasoning§ X. (4.21)The approximate equation (3.59) has higher derivative terms multiplied by a small parameter 1/α^2 and has unknown correction terms of order O(lnα/α^6).
“The approximate equation (3.59) also has the char- acter of possessing higher derivative terms multiplied by a small parameter (namely, 1/α2), and has unknown cor- rection terms of order O(lnα/α6).”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Findingreasoning§ ACKNOWLEDGMENTSThe general Fourier-transformable solution of the semiclassical equation (3.38) has the formal expression (A5).
“Using Eqs. (3.38), (3.33) and (6.17) we find the following formal expression for the general Fourier transformable solution”
Quote in the paperNot a substantial claimMay combine two claims.
Findingreasoning§ ACKNOWLEDGMENTSThe locations of the zeros of G1 depend on λ and ωk: when λ≥λcrit there are four complex zeros ±ω,±ω* with ω=α0+iβ0 in the first quadrant; when λ≤λcrit there are three separate cases.
“When λ ≥ λcrit, there are four complex zeros ±ω,±ω∗, where ω = α0 + iβ0 lies in the first quadrant. When λ ≤ λcrit there are three separate cases.”
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Findingreasoning§ VI. THE ANEC INTEGRAL IN FIRST ORDERFor general algebraic states, the positivity condition is equivalent to the positivity of the operator M_ij = [[g, f],[f*, g*+J]] in the sense of Eq. (6.6).
“For general, alge- braic states ωin the positivity condition is equivalent to the positivity of the operator Mij = [ g f f∗ g∗ + J ] , (6.5)”
Quote in the paperNot a substantial claimMay combine two claims.
Findingreasoning§ VI. THE ANEC INTEGRAL IN FIRST ORDERM is a positive operator on L^2(R^3) ⊕ L^2(R^3), which implies that g is a positive operator on L^2(R^3): ∫∫ g(k,k') u(k)u(k')* ≥ 0.
“Thus, M is a positive operator on L2(R3) ⊕ L2(R3), which implies, in particular, that g is a positive operator on L2(R3):”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Findingreasoning§ C. Expansion of the generalized ANEC integralSince the smearing function S depends only on the magnitude σ_T≡x_T^2 of x_T, the function Θ^(1)_γ is given by Eq. (5.17).
“Since the smearing function S in Eq. (5.2) depends only on the magnitude σT ≡ x2 T of xT , the function Θ (1) γ that appears in Eq. (5.16) is given by”
Quote in the paperNot a substantial claimClassified as probably not a substantial claim.
Findingreasoning§ C. Expansion of the generalized ANEC integralInserting these expansions into Eq. (5.2) yields I_s(ε)=εI_s^(1)+ε^2I_s^(2)+O(ε^3).
“Inserting these expansions into Eq. (5.2) yields Is(ε) = εI(1) s + ε2I(2) s +O(ε3), (5.14)”
Quote in the paperSubstantial claimMay combine two claims.
Findingreasoning§ 0. Since Q̂ is trace class there will exist an orthonormalThe case Â=B̂=Ĉ=0 can be excluded; if all these coefficients vanish, Q̂ must vanish and |ψ>= ̄ρ^(1)=0.
“Moreover, the case = B̂ = Ĉ = 0 can be excluded in the following way. If all these coefficients vanish, an argument similar to that given in Sec. VI E 2 shows that the operator Q̂ in Eq. (7.10) must vanish, and that con- sequently |ψ〉 = ¯̂ρ (1) = 0.”
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Findingreasoning§ C. Expansion of the generalized ANEC integralIn this gauge the vector field v^a described in Sec. V B vanishes.
“In this gauge the vector field va described in Sec. VB vanishes.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Findingreasoning§ C. The first order ANEC integral: general formulaCombining the alternative representation (6.14) of the two point function with Eqs. (6.25) and (6.26) yields Eq. (6.27).
“Now by combining the alternative representation (6.14) of the two point function with Eqs. (6.25) and (6.26), we obtain”
Quote in the paperNot a substantial claimClassified as probably not a substantial claim.
Findingreasoning§ V. THE GENERALIZED ANEC INTEGRALThe generalized ANEC integral depends on arbitrary choices of P, χ, ζ^a, S, etc.
“Clearly this quantity depends on our arbitrary choices of P , χ, ζa, S etc.”
Quote in the paperSubstantial claimClassified as probably not a substantial claim.
Findingreasoning§ 1 , eUsing Eqs. (1.13), (2.4) and (6.1), the source tensor s̃_ab can be rewritten in terms of the regularized two-point function of the incoming state as Eq. (6.21), where σ_ab is given by Eq. (6.22).
“Next we rewrite the source tensor s̃ab in terms of the regularized two-point function of the incoming state. Us- ing Eqs. (1.13), (2.4) and (6.1), we find that”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S3 (load-bearing). May combine two claims.
Findingnone given§ X. (4.21)In the large N limit, the original equation (3.38) is formally known to all orders in h̄, whereas the reduced order equation is valid only to order h̄^2.
“in the large N limit, the orig- inal equation (3.38) is formally known to all orders in h̄, whereas the reduced order equation is valid only to or- der h̄2.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing). May combine two claims.
Findingnone given§ X. (4.21)The full nonlinear semiclassical Einstein equation is highly nonlocal and is not known to be even of an integro-differential type.
“the full, nonlin- ear semiclassical Einstein equation is a highly nonlocal equation, which is not known to be even of an integro- differential type.”
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Findingreasoning§ VII. PURE INCOMING STATES AND THEThe second-to-last term in Eq. (7.3) is proportional to Eq. (7.7).
“The more interesting term in Eq. (7.3) is the second to last term, which can be shown to be proportional (at the relevant order in 1/α2) to”
Quote in the paperNot a substantial claimClassified as probably not a substantial claim. The quote only partly states this claim.
Findingreasoning§ 1 , eInserting Eq. (6.21) into Eq. (6.18) yields the null-null component of the linearized Einstein tensor, Eq. (6.23), with J given by Eq. (6.24).
“Inserting Eq. (6.21) into Eq. (6.18) yields the null-null component of the linearized Einstein tensor”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Findingnone given§ X. (4.21)The explicit form of the second order semiclassical Einstein equation (3.5) is not known, since the term <T^(2)_ab[h^(1),h^(1)],ω_in,0> has not been evaluated.
“the explicit form of this equation is not known, since the term 〈T (2) ab [h(1), h(1)], ωin,0〉 has not been evaluated.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Findingreasoning§ ACKNOWLEDGMENTSSolving Eq. (A1) using Fourier transform methods reproduces the last term in Eq. (A3).
“Hence, solving Eq. (A1) using Fourier transform methods will re- produce the last term in Eq. (A3).”
Quote in the paperNot a substantial claimClassified as probably not a substantial claim.
Findingreasoning§ VII. PURE INCOMING STATES AND THE∆C depends on ω̄(1)_in, ω̄(2)_in, and the freely specifiable incoming piece of the metric perturbation χ(1,0)_ab.
“The coefficient ∆C in Eq. (7.5) is defined to the contribution from the last two terms in Eq. (7.3), and depends both on ω̄ (1) in and ω̄ (2) in as well as the freely specifiable incoming piece of the metric perturbation χ (1,0) ab .”
Quote in the paperSubstantial claimClassified as probably not a substantial claim. The quote only partly states this claim.
Findingreasoning§ V. THE GENERALIZED ANEC INTEGRALI(ε)=εI^(1)+ε^2I^(2)+O(ε^3), where I^(1) and I^(2) are given by Eqs. (5.10) and (5.11).
“I(ε) = εI(1) + ε2I(2) +O(ε3), (5.9)”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Findingreasoning§ C. Expansion of the generalized ANEC integralIn this gauge, the expression for I_s^(2) reduces to Eq. (5.19).
“The expression for I (2) s in this gauge reduces to”
Quote in the paperNot a substantial claimClassified as probably not a substantial claim.
Findingreasoning§ X. (4.21)In subsection III E, an explicit approximate form (3.59) of the second order semiclassical Einstein equation was derived, valid for long wavelengths and when the incoming gravitational radiation does not dominate the first order metric perturbation.
“in subsection III E above, we derived the explicit approx- imate form (3.59) of this equation, which is valid for long wavelengths and when the incoming gravitational radia- tion does not dominate the first order metric perturba- tion.”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Findingnone given§ ACKNOWLEDGMENTSThe general solution to Eq. (3.38) can be written as G(1)ab = G(1),inhom_ab + G(1),free_ab + G(1),free,T_ab.
“The general solution to Eq. (3.38) can be written as G (1) ab = G (1), inhom ab +G (1), free ab +G (1), free,T ab . (A12)”
Quote in the paperNot a substantial claimMay combine two claims.
Findingreasoning§ 1 + |xT |4IF(xT) vanishes identically if and only if g(1)=0, i.e., if and only if the perturbed two-point function is pure to first order.
“We now show that ĪF (xT ) cannot vanish identically unless g(1) = 0, i.e., unless the perturbed two-point function is pure to first order.”
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Findingnone given§ C. Expansion of the generalized ANEC integralThe volume 4-form can be expanded as ǫ_abcd(ε)=ǫ^(0)_abcd+εǫ^(1)_abcd+O(ε^2), where ǫ^(1)=h^(1)e_e ǫ^(0)/2.
“Similarly the volume 4-form can be expanded as ǫabcd(ε) = ǫ (0) abcd + εǫ (1) abcd + O(ε2), where ǫ(1) = h (1) e e ǫ(0)/2.”
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Findingreasoning§ ACKNOWLEDGMENTSThe poles in the Green's function 1/F1 are the zeros of G1.
“The poles in the Greens function are just the zeros of G1.”
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Findingreasoning§ ACKNOWLEDGMENTSEq. (A5) is not the general solution; the general solution is obtained by adding extra terms corresponding to poles of 1/F1 and 1/(F1F3).
“While Eq. (A5) is not the general solution we are looking for, it is straightforward to write down the gen- eral solution by inspection, essentially by adding extra terms to Eq. (A5) that correspond to poles of the func- tions 1/F1 and 1/(F1F3).”
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Findingnone given§ V. THE GENERALIZED ANEC INTEGRALFor a one-parameter family of null geodesics γ(ε), to order ε the family is characterized by the zeroth order geodesic γ and by the vector field v^c=(∂/∂ε)^c on γ.
“To order ε, this one parameter family of geodesics is characterized by the zeroth order geodesic γ = γ(0) (a null geodesic in Minkowski space- time), and by the vector field vc = (∂/∂ε)c on γ.”
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Findingreasoning§ 1 + |xT |4A = ∫γ <T^(0)_ab, ω̄^(1)_in> λaλb = ĪF(0).
“A = ∫ γ 〈T (0) ab , ω̄ (1) in 〉λaλb = ĪF (0), (6.43)”
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Findingreasoning§ 1 , eIn the coordinates γ, β, k_T on momentum space, the positive light cone volume element can be written as Eq. (6.13).
“In these coordinates the positive light cone volume ele- ment can be written as”
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Findingreasoning§ 1 , eThe linearized Einstein tensor (6.23) has the same regularity properties as were proved in Appendix C for the source tensor (3.43).
“By using the techniques of Appendix C, it is possible to show that the linearized Einstein tensor (6.23) has the same regularity properties as were proved in Appendix C for the source tensor (3.43).”
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Findingnone given§ X. (4.21)For partial differential equations, the reduction of order procedure is guaranteed only to reduce the differential order of the time derivatives, not of the spatial derivatives.
“in the case of partial differential equa- tions, the procedure is guaranteed only to reduce the dif- ferential order of the time derivatives, not of the spa- tial derivatives.”
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Findingnone given§ ACKNOWLEDGMENTSThere exists a unique k0>0 depending on λ such that the locus of the zeros of F3(k) is k^2=ωk^2−w^2=k0^2.
“There exists a unique k0 > 0 depend- ing on λ such that the locus of the zeros of F3(k) is k2 = ω2 k − w2 = k2 0 .”
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Findingreasoning§ VII. PURE INCOMING STATES AND THEThe choice of gauge guarantees that χ(1)_ab=0 along γ, and χ(1,0)_ab also vanishes on γ.
“However, our choice of gauge guarantees that χ (1) ab = 0 along γ. In particular this will be true to each order in the 1/α2 expansion of Eq. (3.52), so that χ (1,0) ab also vanishes on γ, and therefore this term vanishes.”
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Findingreasoning§ C. Expansion of the generalized ANEC integralThe scalar fields λ(ε), ζ(ε), σ_T(ε), and vector field λ^a(ε) are coordinate-independent scalar and tensor fields, though their domain is restricted to a neighborhood of γ.
“although these objects are defined in terms of an algo- rithm to obtain a coordinate system, they are themselves coordinate-independent scalar and tensor fields. Their domain of definition is however restricted to some neigh- borhood of the geodesic γ.”
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Findingnone given§ C. Second order vacuum polarizationThe stress tensor (7.21) does not depend on which solution h(2) of G(1)_ab[h(2)] + G(2)_ab[h(1),h(1)]=0 is chosen, and thus is a function only of h(1).
“Moreover, the stress tensor (7.21) does not depend on which solution h(2) of G (1) ab [h(2)] + G (2) ab [h(1), h(1)] = 0 is chosen, and thus is a function only of h(1).”
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Findingreasoning§ 0. Since Q̂ is trace class there will exist an orthonormalThe coefficients Â, B̂, and Ĉ obey the same positivity conditions as A, B, and C: Â≥0, B̂≥0 whenever Â=0, and Ĉ≥0 whenever Â=B̂=0.
“Hence the coefficients Â, B̂ and Ĉ obey the same pos- itivity conditions as the coefficients A, B and C: Â ≥ 0, B̂ ≥ 0 whenever = 0, and Ĉ ≥ 0 whenever = B̂ = 0.”
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Findingreasoning§ VII. PURE INCOMING STATES AND THEEq. (7.7) contains both a contribution quadratic in ω̄(1)_in and a cross term between ω̄(1)_in and incoming classical gravitational radiation.
“Thus, Eq. (7.7) contains both a contribution quadratic in the incoming state perturbation ω̄ (1) in and a cross term between ω̄ (1) in and the incoming classical gravitational ra- diation.”
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Findingnone given§ X. (4.21)Reducing order treating 1/α as the small parameter is equivalent to treating τ as the small parameter.
“It is clear that reducing order treating 1/α as the small parameter is equivalent to treating τ as the small param- eter.”
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Findingown data§ C. The first order ANEC integral: general formulaThe distribution K(xT) is given by a smooth function away from the origin xT=0, but not at the origin.
“Note that it follows from the analysis in Appendix D that the distribution K(xT ) is given by a smooth func- tion away from the origin xT = 0, but not at the origin.”
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Findingreasoning§ VII. PURE INCOMING STATES AND THEWhenever Â=B̂=0, the last two terms in Eq. (7.3) vanish, and consequently ∆C=0.
“We now show that whenever = B̂ = 0, the last two terms in Eq. (7.3) vanish, and that consequently ∆C = 0.”
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Findingreasoning§ 0. Since Q̂ is trace class there will exist an orthonormalFrom Eq. (7.12), all terms on the left-hand side are individually nonnegative, and hence they all vanish.
“From the arguments given in Sec. VI E 1, it is clear that all the terms on the left hand side are individually non- negative, and hence they all vanish.”
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Findingreasoning§ 1 , eEqs. (6.18)-(6.20) could also be obtained by expanding the exact solutions (A5)-(A8) in powers of h̄ and h̄ ln h̄, assuming λ ∝ √h̄.
“Note that Eqs. (6.18) – (6.20) could also be obtained by ex- panding the exact solutions (A5) – (A8) given in Ap- pendix A in powers of h̄ and h̄ ln(h̄) (assuming λ ∝ √ h̄ as discussed in Sec. III E above).”
Quote in the paperNot a substantial claim- The authors state this as an assumption: λ ∝ √h̄.
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Findingreasoning§ VI. THE ANEC INTEGRAL IN FIRST ORDERFor Fock space states, the positivity condition is the statement <Φ̂(u)Φ̂(u)†> ≥ 0 for all complex smearing functions u.
“which for Fock space states is just the statement that 〈Φ̂(u)Φ̂(u)†〉 ≥ 0 (6.4) for all complex smearing functions u.”
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Findingreasoning§ X. (4.21)In the example Eq. (4.25), the reduction of order procedure can eliminate the third order time derivative of Φ but does not eliminate the third order spatial derivatives or all third order mixed spatial and time derivatives.
“The reduction of order procedure can be used to eliminate the third order time derivative of Φ from the equation, but it does not eliminate the third or- der spatial derivatives or all of the third order mixed spa- tial and time derivatives.”
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Findingnone given§ X. (4.21)The method of reduction of order is directly applicable only to local ordinary or partial differential equations, although it was extended to the integro-differential equation (3.38).
“the method is directly applicable only to local, ordinary or partial, differential equations, although we were able to extend it in a natural manner to the integro- differential equation (3.38).”
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Findingreasoning§ VI. THE ANEC INTEGRAL IN FIRST ORDERAt second order, the restriction on g^(2) is Eq. (6.10); in particular, when g^(1)=0 this reduces to Eq. (6.11).
“At second order we obtain the restriction on g(2) that [ P 0 0 1 ] [ g(2) f (1) f (1) ∗ J ] [ P 0 0 1 ] ≥ 0, (6.10) where P is the projection operator onto the kernel of g(1). In particular, when g(1) = 0 this reduces to”
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Findingnone given§ V. THE GENERALIZED ANEC INTEGRALA generalized ANEC integral is defined as an integral over all of spacetime, and it reduces to the transversely smeared ANEC integral in a certain limit.
“we define a third in- tegral which we call a generalized ANEC integral, which is an integral over all of spacetime, and which reduces to the transversely smeared ANEC integral in a certain limit”
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Findingreasoning§ 1 + |xT |4When A=B=0, for ΛT>ΛT,crit, C ≥ 0, with equality holding if and only if g(1)=0.
“We now shall show that when A = B = 0, for ΛT > ΛT,crit we have C ≥ 0, with equality holding if and only if g(1) = 0.”
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Findingreasoning§ VI. THE ANEC INTEGRAL IN FIRST ORDERFor Fock space states, Eq. (6.7) is the statement that <Φ̂_+(u)†Φ̂_+(u)> ≥ 0 for any test function u.
“For Fock space states, Eq. (6.7) is just the statement that 〈Φ̂+(u)†Φ̂+(u)〉 ≥ 0 for any test function u.”
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Findingreasoning§ 1 + |xT |4B = ν0(ΛT2 − ΛT,crit2)(∇T2 ĪF)(0).
“B = ν0(Λ 2 T − Λ2 T,crit)(∇2 T ĪF )(0), (6.44)”
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Findingnone given§ X. (4.21)Solutions to Eq. (4.23) coincide with second order approximate perturbative solutions.
“Note that solutions to Eq. (4.23) also coincide with second order approximate perturbative solutions.”
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Findingreasoning§ 1 , eUsing Horowitz's formula for the Fourier transform of H_λ, H̃_λ(k)=−2π[lnλ^2|k^2|+2γ−1−iπ sgn(k0)Θ(−k2)], and Eqs. (3.33) and (3.36), one obtains Eqs. (6.18)-(6.20).
“We use the following formula given by Horowitz [48] for the Fourier transform of the distri- bution Hλ”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [48]
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Findingreasoning§ VI. THE ANEC INTEGRAL IN FIRST ORDERThe corresponding classical positivity condition is the stronger condition that the matrix [[g,f],[f*,g*]] ≥ 0.
“the corresponding classical positivity condi- tion, which requires that the two point function be the expected value of Φ(x)Φ(y) with respect to some posi- tive measure on the space of field configurations, is the stronger condition that [ g f f∗ g∗ ] ≥ 0. (6.8)”
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Findingreasoning§ C. The first order ANEC integral: general formulaCombining Eqs. (5.15) and (6.23) yields the first order perturbation to the generalized ANEC integral expressed in terms of f^(1) and g^(1), Eq. (6.25).
“Combining Eqs. (5.15) and (6.23) yields that”
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Findingreasoning§ X. (4.21)The resulting equation from applying reduction of order to Eq. (3.59) is Eq. (4.23).
“We obtain”
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Findingreasoning§ 1 , eThe assumed regularity properties on the incoming state imply that f̂ and ĝ are continuous as functions of (β,k_T,β',k'_T) and satisfy the bound (6.16) for any integer N.
“our assumed regularity properties on the incoming state imply that f̂ and ĝ are continuous as functions of (β,kT , β ′,k′ T ) and satisfy, for any integer N ,”
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Findingown data§ 1 , eThe Fourier transform s̃_ab is continuous everywhere away from the light cone, and is bounded everywhere except for an integrable divergence at the origin in momentum space.
“In Appendix C we show that the Fourier transform s̃ab is actually continuous every- where away from the light cone, and is bounded every- where except for an (integrable) divergence at the origin in momentum space.”
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Findingnone given§ V. THE GENERALIZED ANEC INTEGRALThe gauge transformation properties (3.31) and (5.7) are consistent with differential equation (5.5).
“The gauge transformation properties (3.31) and (5.7) are consistent with differential equation (5.5).”
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Findingreasoning§ C. Expansion of the generalized ANEC integralIn the gauge associated with the coordinate system described in Sec. V A, λ^(1)a=λ^(1)=ζ^(1)=σ_T^(1)=0.
“This yields a choice of gauge in which we have λ(1) a = λ(1) = ζ(1) = σ (1) T = 0. (5.18)”
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Findingnone given§ ACKNOWLEDGMENTSThe inhomogeneous part of the solution is given by Eq. (A13).
“The inhomoge- neous part of the solution is given by”
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Findingnone given§ C. Expansion of the generalized ANEC integralThe quantities I_s^(1) and I_s^(2) are gauge invariant.
“As in the previous subsection, the quantities I (1) s and I (2) s are gauge invariant.”
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Findingnone given§ 1 +If λ>λcrit then K̃1(kT) is continuous; its Fourier transform K1(xT) is L2 and continuous everywhere away from the origin.
“Note that if λ > λcrit then K̃1(kT ) is a continuous function; its Fourier transform K1(xT ) is L2 and is con- tinuous everywhere away from the origin.”
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Findingreasoning§ 1 +From properties of f and g and the form of Eq. (C12), Fab and hence S̃ab(l,ω) is continuous everywhere away from the lightcone, and |l|Fab(l,ω) is bounded in a neighborhood of l=0.
“From the properties of the functions f and g and the form of Eq. (C12), it is clear that Fab and hence also S̃ab(l, ω) is continuous everywhere away from the lightcone, and that |l|Fab(l, ω) is bounded in a neighborhood of l = 0.”
Quote in the paperNot a substantial claim- The authors state this as an assumption: The paper assumes that the functions F, ∂F/∂t, ∂F/∂t′, and ∂2F/(∂t∂t′) lie in class V: they are smooth and all their spatial derivatives are L1 on Σ×Σ.
Probably not a substantial claim: may not pass S3 (load-bearing). May combine two claims. The quote only partly states this claim.
Findingreasoning§ ACKNOWLEDGMENTSFor λ<λcrit, the homogeneous term G(1),free_ab has freely specifiable terms for each pole of 1/F1; poles off the real axis give exponentially growing/decaying terms, and poles on the real axis give tachyonlike contributions analogous to Eq. (A2).
“The poles off the real axis will give exponentially grow- ing/decaying terms, and the poles on the real axis will give”
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Findingreasoning§ 1 +The assumptions imply that f̂≡ωkωk′f and ĝ≡ωkωk′g are at least C0.
“Moreover our assumptions imply the functions f̂ ≡ ωkωk′f and ĝ ≡ ωkωk′g defined before Eq. (6.15) are at least C0, a fact which is used in the body of the paper.”
Quote in the paperSubstantial claim- The authors state this as an assumption: The paper assumes that the functions F, ∂F/∂t, ∂F/∂t′, and ∂2F/(∂t∂t′) lie in class V: they are smooth and all their spatial derivatives are L1 on Σ×Σ.
May combine two claims.
Findingnone given§ 1 =The positivity result would not hold for any smearing function which falls off more rapidly than |K1|; there is no positivity result for Gaussian transverse smearing.
“We remark that this positivity re- sult would not hold for any smearing function which falls off more rapidly than |K1|. Thus, for example, there is no positivity result for Gaussian transverse smearing.”
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Findingnone given§ ACKNOWLEDGMENTSThe freely specifiable piece associated with the second term in Eq. (A13) does not vanish even for conformal coupling.
“However, as we discuss below, the freely specifiable piece of the solution associated with the second term in Eq. (A13) [Eq. (A16) below] does not van- ish even for conformal coupling.”
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Findingnone given§ ACKNOWLEDGMENTSPoles on the real ω axis occur only for λ<λcrit for 1/F1, but occur for all values of λ for 1/F3.
“As discussed above, poles on the real ω axis will occur only for λ < λcrit for the function 1/F1, but will occur for all values of λ for the function 1/F3.”
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Findingreasoning§ 1 +Fab(l,ω) is given by Eq. (C8).
“where la = (l, ω) and Fab(l, ω) = ∫ d3kωkωk−l (1,n)a × [ δ(ω − ωk + ωk−l)g(k,k − l)(1,−n′)b −δ(ω − ωk − ωk−l)f(k, l − k)(1,n′)b ] . (C8)”
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Findingnone given§ 0 and k2 = k2The freely specifiable transverse piece of the solution does not vanish in the conformally coupled case ξ=1/6, despite the analogous transverse contribution to the inhomogeneous piece vanishing for conformal coupling.
“Also, as remarked above, this freely specifiable transverse piece of the solution does not vanish in the conformally cou- pled case ξ = 1/6, despite the fact that the the analo- gous transverse contribution to the inhomogeneous piece of the general solution [the second term in Eq. (A13) above] does vanish for conformal coupling.”
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Findingcitation§ ACKNOWLEDGMENTSThe second term G(1),free_ab in Eq. (A12) is the freely specifiable homogeneous piece associated with 1/F1; for λ>λcrit it can be written as Eq. (A14).
“The second term G (1), free ab in Eq. (A12) is the freely specifiable, homogeneous piece of the general solution as- sociated with the Greens function 1/F1(k). In the case λ > λcrit, it can be written as [92]”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [92]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
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Findingreasoning§ ACKNOWLEDGMENTSIn the conformally coupled case ξ=1/6, the trace of the source tensor sab vanishes, and hence the second term in Eq. (A13) vanishes.
“Note also that in the conformally coupled case ξ = 1/6, the trace of the source tensor sab vanishes, and hence the second term in Eq. (A13) vanishes.”
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Findingnone given§ ACKNOWLEDGMENTSThe solution (A14) is purely exponentially growing/decaying and has no oscillatory parts.
“This is purely an exponentially growing/decaying type solution and has no oscillatory parts.”
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Findingreasoning§ 1 +The proof can be extended to any positive smearing function which does not fall off at large xT more rapidly than K1 (∝|xT|^-4); any function falling off slowly enough will be suitable when sufficiently dilated.
“In fact, our proof below can be easily extended to apply to any positive smearing function which does not fall off at large xT more rapidly than K1 does (∝ |xT |−4); in other words, any function which falls off slowly enough will be a suitable smearing function when sufficiently”
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Findingreasoning§ 0 and k2 = k2Exact solutions to the alternative rescaled version (3.45) of the first-order perturbation equation can be obtained from the above analysis using substitutions h(1)ab→α^2ĥ(1)ab, Lp→Lp/α, λ→λ/α, and sab→s̄ab.
“Finally, we remark that exact solutions to the alterna- tive, rescaled version (3.45) of the first order perturbation equation can be obtained from the above analysis using the substitutions”
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Findingcitation§ 0 and k2 = k2The third term G(1),free,T_ab in Eq. (A12) is a purely transverse, freely specifiable piece associated with 1/F3; it can be written as Eq. (A16).
“The third term G (1), free,T ab in Eq. (A12) is a purely transverse, freely specifiable piece of the solution which is associated with the Greens function 1/F3. It can be written as [92]”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [92]
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Probably not a substantial claim: may not pass S3 (load-bearing).
Findingnone given§ 1 =For the tachyon type solution (A15), the linearized Einstein tensor can be written as Eq. (B13).
“For the tachyon type solution (A15), the linearized Ein- stein tensor can be written as G̃ab(β, γ,kT ) = δ(−2γβ + k2 T − k2 0)Fab(β, γ, k̂T ), (B13)”
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Findingnone given§ 1 =The proof could be modified to apply to smearing functions that fall off more slowly than |K1|.
“However, as mentioned above, our proof could easily be modified to apply to smearing functions that fall off more slowly than |K1|.”
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Findingreasoning§ 2 log[K2I(K,x)=12π/x^3+∫ dφ ∆I(K,x,μ).
“it can be shown that I(K,x) = 12π/x3 + ∫ 2π 0 dϕ∆I(K,x, µ). (D7)”
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Findingreasoning§ 1 =Since Fab is freely specifiable away from 2βγ+k0^2=0, I(1) is generally nonvanishing and can be of either sign.
“Since Fab(β, γ, k̂T ) is freely specifiable away from 2βγ + k2 0 = 0, it is clear that in general I(1) is non vanishing and can be of either sign.”
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Findingnone given§ 1 =F is determined by the restrictions of F, ∂F/∂t, ∂F/∂t′, and ∂2F/(∂t∂t′) to Σ×Σ, where Σ is the hypersurface t=0.
“The function F is determined by the restrictions of the four functions F , ∂F/∂t, and ∂F/∂t′ and ∂2F/(∂t∂t′) to Σ×Σ, where Σ is the hypersurface t = 0.”
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Findingnone given§ 1 =It would be sufficient for all results to assume only that all spatial derivatives up to seventeenth order are L1; the sharp falloff requirements have not been investigated.
“It would be sufficient for all of our results to assume only that the all spatial derivatives up to seventeenth order are L1; we have not investigated what the sharp falloff requirements are.”
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Findingreasoning§ 1 =The conditions on F apply to both F_in^(1) and F_in^(2); conclusions about the expected stress tensor in state (C1) apply to source term (3.43) and to the first term in Eq. (3.54).
“Also the conditions on F that we discuss below apply to both the functions F (1) in and F (2) in that appear in the body of the paper, and our conclusions about the expected stress tensor in the state (C1) clearly then will apply to the source term (3.43) and to the first term in Eq. (3.54).”
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Findingreasoning§ 1 +Similar conclusions apply to the entire stress tensor T̃ab(k).
“Similar conclusions apply to the entire stress tensor T̃ab(k).”
Quote in the paperNot a substantial claimMay combine two claims.
Findingreasoning§ 1 +For λ<λcrit, expression (B1) blows up at some finite |kT| so that K̃1 is not even L2.
“For λ < λcrit, the expression (B1) blows up at some finite value of |kT | so that K̃1 is not even L2.”
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Findingnone given§ 1 =Imposing the condition on any other surface of constant time yields the same class of states.
“Note that imposing this condition on any other surface of constant time would yield the same class of states.”
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Findingreasoning§ 1 +The Fourier transform T̃ab(k) exists as a distribution.
“Therefore its Fourier transform T̃ab(k) exists as a distribution.”
Quote in the paperNot a substantial claim- The authors state this as an assumption: The paper assumes that the functions F, ∂F/∂t, ∂F/∂t′, and ∂2F/(∂t∂t′) lie in class V: they are smooth and all their spatial derivatives are L1 on Σ×Σ.
May combine two claims.
Findingreasoning§ 2 log[K2The Fourier transform of k^2 log(k^2) consists of a smooth positive function away from the origin, plus distributional contributions at the origin whose effects are unimportant because of condition (D1).
“The essential idea is that the Fourier trans- form of k2 log(k2) consists of a smooth positive function away from the origin, plus distributional contributions at the origin whose effects are unimportant because of the condition (D1).”
Quote in the paperSubstantial claimMay combine two claims.
Findingnone given§ 1 + (µK)p+1If the state of the quantum field is the incoming vacuum, the second term on the right-hand side of Eq. (E2) is of order Lp^2/L^4, whereas the first term is of order 1/L^2, where L is the length scale determined by the classical background solution.
“Now if the state of the quantum field is the incoming vac- uum state, then the second term on the right hand side above will be in order of magnitude ∼ L2 p/L4, whereas the first term should be ∼ 1/L2, where L is the length- scale determined by the classical background solution g (0) ab .”
Quote in the paperSubstantial claimThe quote only partly states this claim.
Findingreasoning§ 1 + (µK)p+1Examples of the type that appear to violate ANEC qualitatively differently from the cases in the body also exist in perturbation theory off Minkowski spacetime.
“examples of this type also exist in the context of perturbation theory off of Minkowski spacetime”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Findingreasoning§ 1 +S̃ab(la)=Fab(la)+Fab(−la)*.
“S̃ab(la) = Fab(la) + Fab(−la)∗, (C7)”
Quote in the paperNot a substantial claimMay combine two claims.
Findingreasoning§ 1 +The stress tensor T̃ab(k) is L2, from which it follows that Tab(x) is L2 on Minkowski spacetime.
“Finally, we note that the stress tensor T̃ab(k) is L2, from which it follows that Tab(x) is L2 on Minkowski spacetime.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing). May combine two claims.
Findingreasoning§ 1 +In the λ<λcrit case, an appropriate iε regularization prescription yields a well-defined distribution K̃1 with well-defined distributional Fourier transform K1(xT).
“The regularization prescription yields a well defined distribution K̃1, with well defined distributional Fourier transformK1(xT ).”
Quote in the paperNot a substantial claimMay combine two claims.
Findingreasoning§ 0 and k2 = k2In the subclass S of exact first-order semiclassical solutions, using half advanced plus half retarded Green's function to obtain the linearized Einstein tensor is equivalent to throwing away runaway solutions by hand for exponential type modes, and yields a particular subclass for oscillatory modes.
“In the case of exponen- tial type modes discussed in Sec. IVC above, the use of this Greens function to pick out a class of solutions is equivalent to throwing away the runaway solutions by hand. For the oscillatory type modes, this choice of Greens function yields a particular subclass of solutions.”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S3 (load-bearing). The quote only partly states this claim.
Findingreasoning§ 1 +The inequality (C13) is finite for N≥5.
“where C0 is a constant, which is finite for N ≥ 5.”
Quote in the paperNot a substantial claimMay combine two claims.
Findingcitation§ ACKNOWLEDGMENTSThere is a portion of the general solution with the form of an integral over k for which both poles are real; it has the same form as Φ> of Eq. (A2) except A and B are replaced by transverse traceless tensors and m^2 is replaced by either of two independent constants depending only on λ.
“In particular, there will be a portion of the general so- lution which has the form of an integral over the values of k for which both poles are real. This expression will have the same form as Φ> of Eq. (A2), except that A and B are replaced by transverse traceless tensors, and the quantity m2 is replaced by either of two independent constants depending only on λ”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing). May combine two claims.
Premisecitation§ II. SEMICLASSICAL GRAVITY WITHWe shall build upon and extend the work of Horowitz [48], who considered semiclassical gravity in perturbation theory about flat spacetime to linear order, without allowing perturbations to the incoming quantum state.
“We shall build upon and extend the work of Horowitz [48], who considered semiclassical gravity in perturba- tion theory about flat spacetime to linear order, without allowing perturbations to the incoming quantum state.”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [48]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
Probably not a substantial claim: may not pass S3 (load-bearing). May combine two claims.
Interpretationreasoning§ II. SEMICLASSICAL GRAVITY WITHFrom the viewpoint of the first scheme, we would expect there to be modifications to Eq. (2.6) which are of order ∼ L_p^2/L^2, and consequently the domain of validity of the equation is restricted to L ≫ L_p.
“Thus, from the viewpoint of this first scheme we would expect there to be modifications to Eq. (2.6) which are of order ∼ L2 p/L2, and consequently the domain of validity of the equation is restricted to L ≫ Lp, where Lp is the Planck length.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S2 (checkable).
Interpretationreasoning§ II. SEMICLASSICAL GRAVITY WITHThis class of models should provide a good testing ground as to whether, in the context of perturbation theory, quantum fields can attain violations of ANEC which are classically forbidden.
“Thus, this class of models should provide a good testing ground as to whether, in the context of perturbation the- ory, quantum fields can attain violations of ANEC which are classically forbidden.”
Quote in the paperNot a substantial claimMay combine two claims. The quote only partly states this claim.
Interpretationreasoning§ 0 (M). Then G(f, g)A purely classical theory, where gravity is coupled to a statistical ensemble of scalar field configurations, would differ from this version of semiclassical gravity only in two respects: first, the term 〈Tab〉ω0 would be absent from Eq. (2.22); second, the quantum mechanical positivity condition on F arising from Eq. (2.16) is less restrictive than the corresponding classical positivity condition.
“We remark that a purely classical theory, where gravity is coupled to a statistical ensemble of scalar field con- figurations, would differ from this version of semiclas- sical gravity only in the following two respects. First, in the classical theory, the term 〈Tab〉ω0 would be ab- sent from Eq. (2.22).”
Quote in the paperNot a substantial claimClassified as probably not a substantial claim.
Interpretationreasoning§ 0 (M). Then G(f, g)Since the expected stress tensor 〈Tab〉ω has a linear dependence on the two-point distribution, G, associated with ω, we have, for any Hadamard state, ω, 〈Tab〉ω = 〈Tab〉ω0 + 〈Tab〉F.
“Since the expected stress tensor 〈Tab〉ω has a linear dependence on the two-point distribution, G, associated with ω, we have, for any Hadamard state, ω, 〈Tab〉ω = 〈Tab〉ω0 + 〈Tab〉F .”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Premisereasoning§ II. SEMICLASSICAL GRAVITY WITHThe exact status and domain of applicability of the semiclassical equation (2.6) is far from clear, due mainly to the fact that we do not have a complete, more fundamental theory of quantum gravity from which Eq. (2.6) could be derived.
“However, as is well known, the exact status and domain of applicability of this equation is far from clear, due mainly to the fact that we do not have a complete, more fundamental the- ory of quantum gravity from which Eq. (2.6) could be derived.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Premisecitation§ II. SEMICLASSICAL GRAVITY WITHIn the second scheme, the semiclassical Einstein equation (2.6) is formally derived from a fully quantum treatment by imagining that there are N decoupled scalar fields present - all of which are in the same quantum state - and then taking the limit N → ∞, with GN = (constant) [58].
“In the second scheme the semiclassical Einstein equa- tion (2.6) is formally derived from a fully quantum treat- ment by imagining that there are N decoupled scalar fields present — all of which are in the same quantum state — and then taking the limit N → ∞, with GN = (constant) (see, e.g., Ref. [58]).”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [58]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
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Interpretationreasoning§ II. SEMICLASSICAL GRAVITY WITHOne might expect that if N is sufficiently large, Eq. (2.6) would be a good approximation up to the curvature scale corresponding to the effective Planck length in the rescaled theory, L ∼ L_p,eff = √N L_p.
“Thus, one might expect that if N is sufficiently large, Eq. (2.6) would be a good approximation up to the cur- vature scale corresponding to the effective Planck length in the rescaled theory, L ∼ Lp,eff = √ NLp.”
Quote in the paperNot a substantial claimClassified as probably not a substantial claim. May combine two claims.
Premisecitation§ AbstractIf ANEC holds, then traversable wormholes cannot occur; in spacetimes in which ANEC is satisfied, the topological censorship theorem rules out traversable wormholes.
“If ANEC holds, then traversable wormholes cannot occur.”
- Also stated in: § I. INTRODUCTION AND SUMMARY · plain
“For example, in spacetimes in which ANEC is satisfied, the topological censorship theorem of Friedman, Schle- ich and Witt [2] rules out traversable wormholes.”
Quote in the paperSubstantial claim0 of 1 sources checked- cites [2]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- Also stated in: § I. INTRODUCTION AND SUMMARY · plain
Probably not a substantial claim: may not pass S3 (load-bearing).
Premisecitation§ II. SEMICLASSICAL GRAVITY WITHFor at least some positive values of ξ, it seems likely that ANEC can be violated [49].
“However, for at least some positive values of ξ, it seems likely that ANEC can be violated [49].”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [49]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
May combine two claims.
Interpretationreasoning§ III. PERTURBATION THEORY ABOUT FLATIf the ANEC integral is to be non-negative generally, it must vanish at first order for pure states, but not necessarily for mixed states.
“This has the implication, which we discussed in the introduction, that if the ANEC integral is to be non-negative gener- ally, it must vanish at first order for pure states, but not necessarily for mixed states.”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Interpretationreasoning§ II. SEMICLASSICAL GRAVITY WITHThe ambiguity (2.10) in 〈T̂ab〉 resulting from the need to introduce a lengthscale is subsumed by the more general ambiguity given by Eq. (2.9).
“Note that the ambiguity (2.10) in 〈T̂ab〉 resulting from the need to introduce a lengthscale is subsumed by the more general ambiguity given by Eq. (2.9).”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S2 (checkable). May combine two claims.
Interpretationreasoning§ I. INTRODUCTION AND SUMMARYThis provides evidence in favor of the second (or first) of the three possibilities discussed in Sec. IA.
“This provides evidence in favor of the second (or first) of the three possibilities discussed in Sec. IA.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing). May combine two claims.
Interpretationnone given§ 0 (M). Then G(f, g)Eq. (2.15) is equivalent to the statement that F is symmetric and real-valued.
“Furthermore, Eq. (2.15) is equivalent to the statement that F is symmetric and real-valued.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing). May combine two claims.
Premisecitation§ II. SEMICLASSICAL GRAVITY WITHThere are at least two different approximation schemes by which the semiclassical equation (2.6) can be formally derived, and these give rise to distinct viewpoints on the range of validity of this equation [50].
“There are at least two different approximation schemes by which the semiclassical equation (2.6) can be formally derived, and these give rise to distinct viewpoints on the range of validity of this equation [50].”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [50]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
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Premisecitation§ II. SEMICLASSICAL GRAVITY WITHThis ambiguity is assumed to be only a two parameter ambiguity [60,61], because in general spacetimes there are only two independent conserved local curvature tensors of dimensions (length)^−4.
“This ambiguity is assumed to be only a two parameter ambiguity [60,61], because in general spacetimes there are only two independent con- served local curvature tensors of dimensions (length)−4”
Quote in the paperNot a substantial claim0 of 2 sources checked- cites [60]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- cites [61]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- The authors state this as an assumption: The ambiguity in the expected stress tensor is only a two parameter ambiguity.
Probably not a substantial claim: may not pass S4 (based).
Interpretationnone given§ II. SEMICLASSICAL GRAVITY WITHOur results concerning ANEC will be valid for all values of α and β.
“However, our results concerning ANEC will be valid for all values of α and β.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S2 (checkable), S3 (load-bearing).
Interpretationreasoning§ II. SEMICLASSICAL GRAVITY WITHIn our view, the existence of higher order corrections to Eq. (2.6) depends on whether or not one justifies that equation in terms of a one-loop approximation or by the invocation of a 1/N limit.
“In our view, the existence of higher order corrections to Eq. (2.6) de- pends on whether or not one justifies that equation in terms of a one-loop approximation or by the invocation of a 1/N limit.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Premisecitation§ II. SEMICLASSICAL GRAVITY WITHThese difficulties do not appear in two dimensional models, for the reasons explained in Ref. [45].
“These difficulties do not appear in two dimensional models, for the reasons ex- plained in Ref. [45]”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [45]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
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Premisecitation§ II. SEMICLASSICAL GRAVITY WITHIf we assume that the prescription for obtaining the expected stress tensor satisfies the axioms discussed in Ref. [45], then the expected stress tensor is unique up the addition of local, conserved curvature tensors.
“If we assume that the prescription for obtaining the expected stress tensor satisfies the axioms discussed in Ref. [45], then the expected stress tensor is unique up the addition of local, conserved curvature tensors.”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [45]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- The authors state this as an assumption: The prescription for obtaining the expected stress tensor satisfies the axioms discussed in Ref. [45].
Probably not a substantial claim: may not pass S2 (checkable).
Interpretationreasoning§ II. SEMICLASSICAL GRAVITY WITHWe would expect effects which are non-perturbative in h̄ could be important at these scales.
“In other words, we would expect effects which are non-perturbative in h̄ could be important at these scales.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Premisecitation§ I. INTRODUCTION AND SUMMARYANEC holds in Minkowski spacetime for free scalar fields and electromagnetic fields.
“Early investigations showed that it holds in Minkowski spacetime for free scalar fields and electromagnetic fields [16–18]”
Quote in the paperNot a substantial claim0 of 3 sources checked- cites [16]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- cites [17]
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- cites [18]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
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Premisecitation§ I. INTRODUCTION AND SUMMARYThe positivity of the ANEC integral along future complete null geodesics is sufficient to prove some singularity theorems.
“Finally, the positivity of the ANEC integral along future complete null geodesics is sufficient to prove some singularity theorems [40].”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [40]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
Classified as probably not a substantial claim. May combine two claims.
Premisecitation§ I. INTRODUCTION AND SUMMARYFord and Roman have derived constraints on the average over time of the energy density measured at a particular point by inertial observers in flat spacetime, and argued their results can be extrapolated to curved spacetime so as to constrain certain types of traversable wormhole spacetimes to be Planck scale.
“More recently, Ford and Roman have derived constraints on the average over time of the energy density measured at a particular point by inertial observers [24] in flat spacetime, and they have argued that their results can be extrapolated to curved spacetime so as to constrain certain types of traversable wormhole spacetimes to be”
Quote in the paperSubstantial claim0 of 2 sources checked- cites [24]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- cites [14]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
Classified as probably not a substantial claim.
Interpretationreasoning§ II. SEMICLASSICAL GRAVITY WITHThe appropriate right hand side for Eq. (2.6) must be of the form 〈T̂ab〉 = 〈T̂ab〉point split + αAab + βBab.
“Thus, if we denote by 〈T̂ab〉point split the stress tensor given by the point splitting algorithm (briefly reviewed in the next subsection), then the appropriate right hand side for Eq. (2.6) must be of the form 〈T̂ab〉 = 〈T̂ab〉point split + αAab + βBab.”
Quote in the paperSubstantial claim- The authors state this as an assumption: The prescription for obtaining the expected stress tensor satisfies the axioms discussed in Ref. [45].
- The authors state this as an assumption: The ambiguity in the expected stress tensor is only a two parameter ambiguity.
Probably not a substantial claim: may not pass S3 (load-bearing), S4 (based). May combine two claims.
Interpretationnone given§ I. INTRODUCTION AND SUMMARYAnalogous arguments apply to spacetimes with negative asymptotic mass and with compactly generated chronology horizons.
“Analogous arguments apply to spacetimes with negative asymptotic mass and with compactly generated chronology horizons.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Premisecitation§ I. INTRODUCTION AND SUMMARYANEC holds in generic, curved, two-dimensional spacetimes.
“and also in generic, curved, 2D spacetimes [18].”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [18]
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Interpretationnone given§ II. SEMICLASSICAL GRAVITY WITHHigher loop contributions would modify Eq. (2.6) by terms proportional to quadratic and higher powers of h̄.
“In either case, higher loop contributions would modify Eq. (2.6) by terms proportional to quadratic and higher powers of h̄.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Interpretationreasoning§ 0 (M). Then G(f, g)F(x, y) satisfies the wave equation (2.3) in each variable.
“In addition, F (x, y) satisfies the wave equa- tion (2.3) in each variable”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing), S4 (based).
Interpretationnone given§ 0 (M). Then G(f, g)Fin satisfies a positivity condition which ensures that Gin is the two-point distribution of a state in Minkowski spacetime.
“It satisfies a positivity condition which ensures that Gin is the two-point distribution of a state in Minkowski space- time.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Premisecitation§ II. SEMICLASSICAL GRAVITY WITHThis required scaling of G contrasts sharply with the situation in the classical theory, where the amplitude, Φ, of the scalar field may be scaled in an arbitrary manner independently of the scaling of the metric tensor [63].
“Note that this required scaling of G contrasts sharply with the situation in the classical theory, where the am- plitude, Φ, of the scalar field may be scaled in an arbi- trary manner independently of the scaling of the metric tensor [63].”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [63]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
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Interpretationreasoning§ 0 (M). Then G(f, g)The Hadamard condition on G corresponds simply to the statement that F(x, y) is a smooth function on M×M.
“However, the Hadamard condition on G now corresponds simply to the statement that F (x, y) is a smooth function on M×M .”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Interpretationnone given§ 0 (M). Then G(f, g)If we modify the prescription for calculating GH by truncating the series after say four terms instead of three terms, then the regularized two-point function f(x, y) will be altered, but the value (2.19) of 〈Tab(x)〉point split will not be changed.
“Note that if we modify the prescription for cal- culating GH by truncating the series after say four terms instead of three terms, then the regularized two-point function f(x, y) will be altered, but the value (2.19) of 〈Tab(x)〉point split will not be changed.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Premisecitation§ I. Introduction and SummaryIn the note in proof section of Ref. [18], violations of ANEC for pure states were obtained at first order in deviation from flatness.
“In the”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [18]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
May combine two claims.
Interpretationreasoning§ 1 + x4/Λ4T_vac(D) is not the convex hull of T_vac(D_P) but is larger than it.
“Tvac(D) is not the convex hull of Tvac(DP ) but is larger than it.”
Quote in the paperSubstantial claimClassified as probably not a substantial claim.
Interpretationreasoning§ II. SEMICLASSICAL GRAVITY WITHThe failure of the classical stress-energy tensor to satisfy pointwise energy conditions when ξ ≠ 0, and its possible failure to satisfy the classical ANEC condition for positive values of ξ, indicates that this class of field theories may not be suitable for a general study of the validity of ANEC in quantum field theory in curved spacetime.
“The failure of the classical stress-energy tensor (2.4) to satisfy pointwise energy conditions when ξ 6= 0, and its possible failure to satisfy the classical ANEC condi- tion for positive values of ξ indicates that this class of field theories may not be suitable for a general study of the validity of ANEC in quantum field theory in curved spacetime.”
Quote in the paperSubstantial claimClassified as probably not a substantial claim. May combine two claims.
Interpretationreasoning§ 1 + x4/Λ4Although the paper proves positivity of a smeared ANEC integral in perturbation theory, it does not have an obvious candidate for a smeared ANEC conjecture outside of this context.
“Thus, although we prove the positivity of a smeared ANEC integral in the context of perturbation theory, we do not even have an obvious candidate for a”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Premisecitation§ I. INTRODUCTION AND SUMMARYUnder the same hypotheses as ANEC, the Penrose-Sorkin-Wolgar positive mass theorem shows that the asymptotic mass must be positive.
“Under the same hypotheses, the Penrose-Sorkin-Wolgar positive mass theorem shows that the asymptotic mass must be positive [41].”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [41]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
Classified as probably not a substantial claim.
Premisenone given§ C. The semiclassical equationsThe expected value of the stress tensor in any state is determined via the point splitting procedure from a knowledge of only the two-point function, G(x, y) = 〈Φ̂(x)Φ̂(y)〉ω.
“However, as we discuss further below, the expected value of the stress tensor in any state is deter- mined via the point splitting procedure from a knowledge of only the two-point function, G(x, y) = 〈Φ̂(x)Φ̂(y)〉ω.”
Quote in the paperSubstantial claimClassified as probably not a substantial claim.
Premisecitation§ AbstractANEC can be violated in curved spacetimes if one is allowed to choose the spacetime and quantum state arbitrarily, without imposition of the semiclassical Einstein equation.
“it is known that ANEC can be violated in curved spacetimes if one is allowed to choose the spacetime and quantum state arbitrarily, without imposition of the semiclassical Einstein equation”
Quote in the paperSubstantial claim0 of 2 sources checked- cites [18]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- cites [42]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
May combine two claims.
Interpretationreasoning§ 1 + x4/Λ4The linearity of the evolution law for states breaks down as a result of the coupling to the classical metric, and this arises only at second order in perturbation theory.
“One reason for this (which may be viewed as an artifact of semiclassical theory) is that the linearity of the evolution law for states breaks down as a result of the coupling to the classical metric. This arises only at second order in perturbation theory.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Interpretationreasoning§ II. SEMICLASSICAL GRAVITY WITHα and β are dimensionless coefficients which can be regarded as free parameters.
“Here α and β are dimensionless coefficients which can be regarded as free parameters.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Premisecitation§ 2 given byNon-runaway solutions can be characterized as those satisfying the integro-differential equation given in Jackson [73].
“integro-differential equation given in Jackson [73]”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [73]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
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Interpretationreasoning§ 1 − ǫ2ω2Although the reduction of order algorithm is uniquely defined for any equation of form (4.18) for a given choice of variables, ambiguities can be introduced by making a τ-dependent change of variables.
“ambiguities in the algorithm can be introduced by mak-”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing). May combine two claims.
Interpretationcitation§ 2 given byCompletely parallel remarks apply to the semiclassical Einstein equation (2.6) if one justifies it via the one-loop approximation, so that there are unknown corrections of order hbar^2.
“there are unknown corrections of order h̄2 [76].”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [76]
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Premisenone given§ 1 − ǫ2ω2The given equation of motion is believed to accurately describe phenomena with sufficiently large length and/or time scales, e.g., τ* ≫ τ for Eq. (4.4) or L ≫ Lp for Eqs. (2.6) and (3.38).
“ciently large length and/or time scales, e.g., τ∗ ≫ τ for”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Premisecitation§ IV. DEALING WITH THE PATHOLOGICALThe Abraham-Lorentz equation of motion for a classical charged point particle including radiation reaction has exponentially growing runaway solutions.
“which also has exponentially growing,”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [36]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
May combine two claims. The quote only partly states this claim.
Interpretationreasoning§ 2 given byThe restriction L >~ cτ and unknown correction terms of order O(τ^2) in the radiation reaction force should occur in any theory where classical electromagnetic fields are coupled to other degrees of freedom with a continuous distribution of charge.
“with a continuous distribution of charge.”
Quote in the paperNot a substantial claimMay combine two claims. The quote only partly states this claim.
Interpretationnone given§ 2 given byThere are situations where the higher order corrections x^(j) for all j≥2 are not sensitive to the higher order corrections to the equation of motion, and where physically meaningful solutions to Eq. (4.4) can be obtained which go well beyond approximation (4.8) and predict large radiation reaction effects.
“which go well beyond the approximation (4.8) and pre-”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S2 (checkable), S3 (load-bearing).
Interpretationreasoning§ 1 − ǫ2ω2A good remedy for this difficulty would be to modify the given equation so that it is equivalent to the desired accuracy to the given equation at large length and/or time scales but does not predict pathological behavior at small scales.
“does not predict any pathological behavior at small scales”
Quote in the paperNot a substantial claimClassified as probably not a substantial claim. May combine two claims.
Premisenone given§ 2 given byEq. (4.4) holds only when τ* ≫ τ, whereas Eq. (2.6) and its linearized version Eq. (3.38) have the domain of validity L ≫ Lp.
“Eq. (4.4) holds only when τ∗ ≫ τ , whereas Eq. (2.6) [as”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S2 (checkable), S3 (load-bearing).
Interpretationreasoning§ 1 − ǫ2ω2When additional degrees of freedom have an oscillatory character, there seems little hope of singling out a preferred subclass of solutions on any physical grounds.
“seems little hope of singling out a preferred subclass of”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S2 (checkable), S3 (load-bearing).
Interpretationreasoning§ 2 to the solution will give riseThe situation with regard to the semiclassical Einstein equation is closely analogous.
“equation is closely analogous.”
Quote in the paperNot a substantial claimClassified as probably not a substantial claim.
Interpretationreasoning§ 1 − ǫ2ω2Generically, any solution to the given equation will have some non-vanishing Fourier components which lie outside the equation's domain of validity.
“which lie outside the equation's domain of validity.”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S3 (load-bearing). May combine two claims.
Premisecitation§ 2 given byThe conventional physical solutions of the radiation reaction equation are the six-dimensional space of non-runaway solutions satisfying Eq. (4.6), but these solutions require pre-acceleration at early times to avoid runaway behavior at late times.
“space of non-runaway solutions satisfying Eq. (4.6).”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [74]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
Probably not a substantial claim: may not pass S3 (load-bearing).
Premisenone given§ 2 to the solution will give riseIn Newtonian hydrodynamics, dissipative terms normally have an effect on fluid motion smaller than non-dissipative terms by a factor ∼ε, where ε is the ratio of a microscopic lengthscale to a macroscopic lengthscale.
“non-dissipative terms by a factor ∼ ǫ, where ǫ is the ra-”
Quote in the paperNot a substantial claimThe quote only partly states this claim.
Interpretationreasoning§ 2 given byThe higher-order time derivative term τ x''' is responsible for the existence of runaway solutions, which grow exponentially in time.
“solutions, which grow exponentially in time.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Interpretationreasoning§ 1 − ǫ2ω2The given equation presumably does not predict even qualitatively correct behavior outside of its range of validity.
“qualitatively correct behavior outside of its range of va-”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing). May combine two claims.
Interpretationreasoning§ 2 given byAlthough one would be formally justified in going beyond the first order in hbar approximate perturbative solution, there is little point because Eq. (2.6) is valid only when L ≫ Lp, and in that regime higher order perturbative solutions should merely make tiny additional corrections to the first order perturbative solution.
“der perturbative solutions should merely make tiny addi-”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing). May combine two claims.
Interpretationreasoning§ 2 given byRunaway solutions quickly evolve into a regime where unknown corrections to the radiation reaction force become as large as the radiation reaction force itself, i.e., τ* ∼ τ, and therefore lie outside the domain of validity of the Abraham-Lorentz equation and are normally deemed unphysical.
“deemed to be”
Quote in the paperNot a substantial claimMay combine two claims.
Interpretationreasoning§ IV. DEALING WITH THE PATHOLOGICALThe exponentially growing solutions to the semiclassical equations are spurious, and are not indicative of any physical instability of flat spacetime.
“In partic- ular, from this point of view the exponentially growing solutions to the semiclassical equations are spurious, and are not indicative of any physical instability of flat space- time.”
Quote in the paperSubstantial claim- The authors state this as an assumption: The semiclassical equations are approximate equations with domain of validity L ≫ Lp.
Probably not a substantial claim: may not pass S2 (checkable), S4 (based).
Interpretationnone given§ IV. DEALING WITH THE PATHOLOGICALThis ability of semiclassical theory to accurately describe such phenomena should hold even in the case of finite N when unknown correction terms of order ∼ L4p/L4 appear in the semiclassical Einstein equation.
“Furthermore, this ability of semiclassical theory to accurately describe such phenomena should the hold even in the case of finite N when unknown correction terms of order ∼ L4 p/L4 appear in the semiclassical Einstein equation.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing), S4 (based).
Interpretationnone given§ IV. DEALING WITH THE PATHOLOGICALIn model (4.13), the issue of picking out a preferred physical solution is essentially equivalent to picking out a preferred Green's function for the differential operator appearing in Eq. (4.13).
“lution”
Quote in the paperNot a substantial claimMay combine two claims.
Interpretationreasoning§ 2 to the solution will give riseEven if there were unknown corrections to the semiclassical equations higher order in hbar, these corrections should be qualitatively unimportant in black hole evaporation except near the singularity and near the final moments of evaporation, where they become locally large.
“corrections should be qualitatively unimportant in the”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S3 (load-bearing). May combine two claims.
Premisecitation§ 1 − ǫ2ω2Reduction of order has been used in classical higher derivative theories of gravity by Bel et al. and more recently advocated in semiclassical gravity by Simon.
“gravity by Bel et. al. [86], and more recently it has been”
Quote in the paperNot a substantial claim0 of 2 sources checked- cites [86]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- cites [36]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
Classified as probably not a substantial claim. May combine two claims. The quote only partly states this claim.
Interpretationreasoning§ C. Extraction of a preferred subclass of "physicalThe proposal to admit only perturbatively expandable solutions would appear to be of the correct character, since the perturbative equations have the correct number of degrees of freedom, and the pathological solutions do not have analytic behavior in the small parameter ε at ε=0.
“acter, since the perturbative equations have the correct”
Quote in the paperSubstantial claimThe quote only partly states this claim.
Interpretationreasoning§ 2 given byFor fixed mass m and nonzero charge q, there is always an ambiguity in the radiation reaction force depending on particle structure, of fractional magnitude >~ τ/τ*, where τ* is the timescale over which the acceleration changes.
“always be an ambiguity in the radiation reaction force”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Interpretationreasoning§ 2 given bySimilar unknown correction terms would appear in Eq. (2.6) if one justifies that equation via the one-loop approximation or takes N finite in the 1/N approximation.
“would appear in Eq. (2.6) if one justifies that equation via”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Interpretationreasoning§ 2 given byThese situations arise when radiation reaction effects are locally small but accumulate secularly, so that they become large at late times.
“but accumulate secularly, so that they become large at”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Premisecitation§ IV. DEALING WITH THE PATHOLOGICALFor a finite charge distribution of physical size L, in the nonrelativistic limit the radiation reaction force is F_react/m = τ ȧ + O[τ ä(L/c)], with τ = (2/3)(q^2/mc^3).
“radiation reaction force on the charge”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [73]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
Probably not a substantial claim: may not pass S3 (load-bearing). May combine two claims.
Interpretationnone given§ C. Extraction of a preferred subclass of "physicalFor the radiation reaction equation, a preferred subclass of exact solutions can be identified by discarding the runaway solutions, although the remaining solutions have the unphysical feature of pre-acceleration.
“remaining solutions have the unphysical feature of”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Premisecitation§ 1 − ǫ2ω2The idea of reduction of order is quite old and has been advocated in the context of the radiation reaction equation by Landau and Lifshitz, Teitelboim, and Ford et al.
“by Landau and Lifshitz [82], Teitelboim [83], and Ford”
Quote in the paperNot a substantial claim0 of 3 sources checked- cites [82]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- cites [83]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- cites [84]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
Probably not a substantial claim: may not pass S3 (load-bearing). May combine two claims.
Interpretationcitation§ 1 − ǫ2ω2The method of self-consistent reduction of order generates a modified, second order equation which is as accurate or nearly as accurate as the original equation, but whose solutions are all well behaved and can be interpreted as physical.
“tion, which is”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [36]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
May combine two claims.
Interpretationreasoning§ 1 − ǫ2ω2Although it is possible to mathematically identify preferred Green's functions, there do not appear to be grounds for arguing that any one is better behaved or more physical than the others.
“ing that any one of these is”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing), S4 (based).
Interpretationnone given§ 2 given byThere are close parallels between the radiation reaction equation and the semiclassical Einstein equation.
“In summary, there are close parallels between the ra-”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing). May combine two claims.
Interpretationcitation§ 1 − ǫ2ω2In the case where additional degrees of freedom have exponentially growing and/or decaying character, non-runaway solutions are a natural candidate for the preferred subclass, although even in this case these physical solutions have unphysical features like pre-acceleration.
“non-runaway solutions are, of course a natural candidate”
Quote in the paperNot a substantial claim0 of 2 sources checked- cites [81]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
- cites [74]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
Classified as probably not a substantial claim.
Interpretationreasoning§ 1 − ǫ2ω2In situations where it is applicable, the reduction of order method achieves this goal.
“the reduction of order method achieves this goal.”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Interpretationreasoning§ 2 to the solution will give riseEffects that are non-perturbative in ε in solutions to hydrodynamic equations will be meaningful when the macroscopic evolution timescale is determined by dissipative effects.
“the macroscopic evolution timescale is determined by dis-”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Interpretationreasoning§ 2 given byThe status of the equation of motion for a nonrelativistic charged particle in a given fixed external electric field E, ẍ = (q/m)E + τ x''', is closely analogous to that of the semiclassical Einstein equation.
“is closely analogous to that of the semiclassical Einstein”
Quote in the paperNot a substantial claimMay combine two claims.
Interpretationreasoning§ 2 to the solution will give riseTherefore none of the approximate perturbative solutions to the heat equation are even qualitatively accurate; non-perturbative effects are vitally important.
“are even qualitatively accurate; non perturbative effects”
Quote in the paperNot a substantial claimThe quote only partly states this claim.
Interpretationreasoning§ 2 given byAn accurate description of the inspiral motion will be provided by an appropriate solution of the exact equation (4.4), provided only that the timescale of the inspiral is much larger than the orbital period, so that radiation reaction effects are locally small.
“appropriate solution of the exact equation (4.4), provided”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Interpretationreasoning§ 2 given byThere is no justification for going beyond the lowest order approximate solution x1(t)=x^(0)(t)+τ x^(1)(t), since unknown terms of order unity appear in the equation for x^(2).
“since unknown terms of order unity appear in the equa-”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing). May combine two claims.
Interpretationreasoning§ 1 − ǫ2ω2The inequivalence of the reduced order equations can occur only at order τ^2 and higher, and thus should not have an important effect on the behavior of solutions in regimes where reduction of order can be justified.
“can occur only at order τ2 and higher, and, thus, should”
Quote in the paperNot a substantial claimClassified as probably not a substantial claim.
Interpretationreasoning§ 1 − ǫ2ω2For some solutions, these Fourier components behave pathologically such that the entire solution is dominated by qualitatively incorrect behavior, as occurs for runaway solutions.
“nated by the qualitatively incorrect behavior, as occurs”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Premisecitation§ 1 − ǫ2ω2Reduction of order is a standard procedure used in the derivation of post-Newtonian equations of motion in classical relativity.
“in the derivation of post-Newtonian equations of motion”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [85]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
Probably not a substantial claim: may not pass S3 (load-bearing).
Interpretationnone given§ 2 given byThe domain of validity of Eq. (4.4) is limited to τ* ≫ τ, similar to the domain of validity L ≫ Lp of the semiclassical Einstein equation.
“is limited to the regime τ∗ ≫ τ , similar to the domain of”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing). May combine two claims.
Interpretationreasoning§ 1 − ǫ2ω2The final reduced order equation is formally as accurate as Eq. (4.18) to order τ but does not contain any new degrees of freedom.
“to order τ , but which does not contain any new”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Interpretationreasoning§ 2 given byEven when Eq. (2.6) is justified via the 1/N approximation and treated as valid to all orders in hbar, the situation is not significantly different.
“Eq. (2.6) as being valid to all orders in h̄, the situation”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S2 (checkable), S3 (load-bearing).
Interpretationreasoning§ 2 to the solution will give riseThe above type of situation-where non-perturbative effects in a small parameter are large but can be reliably calculated even though the equation is known only to first order in that parameter-actually occurs quite commonly in physics.
“curs quite commonly in physics.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S4 (based).
Interpretationreasoning§ 2 to the solution will give riseIt should be possible to calculate these effects reliably from the semiclassical equations provided only that R ≫ Lp everywhere in the region of interest, where R is the local radius of curvature.
“sical equations provided only that R ≫ Lp everywhere”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Interpretationreasoning§ 2 given bySolutions of type (4.8) would not be of much interest, since one could not expect Eq. (4.8) to be a good approximation whenever τ x^(1)(t) becomes of order x^(0)(t), because unknown higher order corrections should also be comparably large.
“to be a good approximation whenever τx(1)(t) becomes”
Quote in the paperNot a substantial claimMay combine two claims.
Interpretationreasoning§ X. (4.21)The reduced order equation for Eq. (4.25) is not hyperbolic and presumably would not have a well posed initial value formulation.
“In particular, the resulting re- duced order equation is not hyperbolic, and presumably would not have a well posed initial value formulation.”
Quote in the paperNot a substantial claimMay combine two claims.
Interpretationreasoning§ X. (4.21)Applying the reduction of order algorithm to Eq. (3.59) yields an equation that should be as accurate as Eq. (3.59) at long wavelengths but has none of the pathological behavior at short wavelengths.
“we may apply the reduction of order algorithm directly to this equa- tion to obtain an equation which should be as accurate as Eq. (3.59) at long wavelengths but which has none of the pathological behavior at short wavelengths.”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Premisereasoning§ VI. THE ANEC INTEGRAL IN FIRST ORDERThe functions f and g cannot be chosen arbitrarily but must satisfy the positivity condition (2.16).
“The functions f and g cannot be chosen arbitrarily but must satisfy the positivity condition (2.16)”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Interpretationnone given§ ACKNOWLEDGMENTSThe exact solutions to Eq. (3.38) are closely analogous to the solutions of the Klein-Gordon equation with negative mass squared.
“The exact solutions to Eq. (3.38) are closely analogous to the solutions of the Klein-Gordon equation with neg- ative mass squared”
Quote in the paperNot a substantial claimMay combine two claims.
Interpretationreasoning§ X. (4.21)The reduction of order procedure is applicable to the perturbation analysis and solves the problem of extra degrees of freedom and pathological solutions possessed by the unmodified equations.
“the reduction of order proce- dure is applicable to our perturbation analysis and, in a completely satisfactory manner, it solves the problem of the existence of extra degrees of freedom and patho- logical solutions possessed by the unmodified equations.”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Interpretationreasoning§ 1 , eThus, Fourier transform methods may be used to solve the reduced order semiclassical equations.
“Thus, we may use Fourier trans- form methods to solve the (reduced order) semiclassical equations.”
Quote in the paperNot a substantial claimMay combine two claims.
Premisecitation§ 1 + |xT |4a is positive for the scalar field considered, for all values of the curvature coupling, and is also positive for neutrino and Maxwell fields.
“As previously mentioned, a is positive for the scalar field we are considering, for all values of the curvature cou- pling [c.f.,Eq. (3.34) above], and is also positive for neu- trino and Maxwell fields [48].”
Quote in the paperSubstantial claim0 of 1 sources checked- cites [48]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
Probably not a substantial claim: may not pass S3 (load-bearing).
Interpretationreasoning§ X. (4.21)The slight loss of accuracy is unimportant because the effect of O(h̄^3) corrections should be negligible in the long wavelength limit.
“this slight loss of accuracy is unimportant since – for the reasons explained in Sec. IV B above – the effect of O(h̄3) corrections should be negligible in the long wave- length limit.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S4 (based). May combine two claims.
Interpretationnone given§ V. THE GENERALIZED ANEC INTEGRALIn the limit Λ→∞, Λ_L,Λ_T→0, the generalized ANEC integral, when it exists, should be independent of these arbitrary choices and for sufficiently well behaved stress tensors should reduce to the usual ANEC integral.
“when it exists, should be independent of these arbitrary choices, and for sufficiently well behaved stress tensors should reduce to the usual ANEC integral.”
Quote in the paperNot a substantial claimMay combine two claims.
Interpretationreasoning§ X. (4.21)In circumstances where the reduction procedure does not eliminate all higher spatial derivatives, it will in general necessitate breaking Lorentz covariance, yielding inequivalent reduced order equations for different choices of time coordinate.
“the reduction procedure will, in general, necessitate breaking Lorentz covariance, i.e., one will obtain inequivalent re- duced order equations by carrying out the procedure with respect to different choices of time coordinate.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing). May combine two claims.
Interpretationnone given§ ACKNOWLEDGMENTSSolutions to the semiclassical equation (3.38) have a very similar character to solutions of the negative-mass-squared Klein-Gordon equation and can be divided into oscillatory and exponential pieces.
“We explicitly display these solutions to the negative mass squared Klein Gordon equation because the solu- tions to the semiclassical equation (3.38) have a very similar character. In particular these solutions can be divided into”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Interpretationnone given§ V. THE GENERALIZED ANEC INTEGRALThe second term in Eq. (5.11) can be thought of as reflecting the fact that the metric perturbations cause a change in the geodesic.
“The second term in Eq. (5.11) can be thought of as re- flecting the fact that the metric perturbations cause a change in the geodesic.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Interpretationreasoning§ VI. THE ANEC INTEGRAL IN FIRST ORDERExpanding this result in 1/α^2 and lnα/α^2 provides an alternative demonstration of the results of this section for solutions of the reduced order equation in the long wavelength limit, at least for λ>λ_crit.
“expanding this result in 1/α2 and lnα/α2 provides an alternative demon- stration of the results of this section for solutions of the reduced order equation in the long wavelength limit, at least for λ > λcrit.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Interpretationreasoning§ X. (4.21)The reduced order equation (4.20) is slightly less accurate than the original equation.
“Therefore, the reduced order equation (4.20) is slightly less accurate than the original equation.”
Quote in the paperNot a substantial claimMay combine two claims.
Interpretationreasoning§ VII. PURE INCOMING STATES AND THEThe condition Â=0 imposes constraints on ω̄(2)_in, which in turn imposes constraints on ω̄(1)_in sufficient to ensure that the second term in Eq. (7.7) vanishes.
“The key idea that we now use is that this condition im- poses constraints on ω̄ (2) in , which in turn imposes con- straints on ω̄ (1) in sufficient to ensure that the second term in Eq. (7.7) vanishes.”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Interpretationreasoning§ X. (4.21)It is not obvious if and/or how the reduction of order procedure could be applied to the full nonlinear semiclassical Einstein equation.
“Thus, it is not obvious if and/or how the reduction of order procedure could be applied to the full, nonlinear semiclassical Einstein equation.”
Quote in the paperNot a substantial claimMay combine two claims.
Interpretationreasoning§ X. (4.21)If the incoming gravitational radiation satisfies condition (3.49), then for all solutions of the equation h^(1)_ab ∝ h̄, and the first term in Eq. (4.22) can be neglected.
“Now if we as- sume that the incoming gravitational radiation satisfies the condition (3.49), then for all solutions of the equa- tion, h (1) ab ∝ h̄ [c.f., Eq. (3.52) above], and the first term in Eq. (4.22) can be neglected.”
Quote in the paperNot a substantial claim- The authors state this as an assumption: The incoming gravitational radiation satisfies condition (3.49).
May combine two claims.
Interpretationreasoning§ 1 + |xT |4In the limit of no smearing (ΛT→0, S(xT)→δ2(xT)), B can be negative and therefore for sufficiently large α the ANEC integral can be negative.
“Therefore, we find that (i) in the limit of no smearing [i.e., ΛT → 0, S(xT ) → δ2(xT )], B can be negative and therefore for sufficiently large α, the ANEC integral can be negative”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Interpretationreasoning§ 1 , eTherefore solutions of the wave equation can be represented by functions of β and of the two-dimensional vector k_T.
“Therefore solutions of the wave equation can be rep- resented by functions of β and of the two dimensional vector kT .”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S2 (checkable), S4 (based).
Interpretationnone given§ X. (4.21)Eqs. (4.20) and (4.23) appear to provide a completely satisfactory solution to the problem of extracting physical predictions from perturbative semiclassical gravity.
“Eqs. (4.20) and (4.23) appear to provide a completely satisfactory solution to the problem of extracting physical predictions from per- turbative semiclassical gravity.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Interpretationreasoning§ 1 =The critical value of ΛT is of order of the Planck length.
“It is clear on dimen- sional grounds that the critical value of ΛT is of order of the Planck length.”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
Interpretationreasoning§ 0 and k2 = k2The analysis of solutions in S can be used as a mathematical tool to establish a positivity result for solutions of the reduced order equations.
“In other words, we can use the analysis of the solutions in S as a mathematical tool to to establish a positivity result for solutions of the reduced order equa- tions.”
Quote in the paperNot a substantial claimMay combine two claims.
Interpretationreasoning§ 1 =The violations of ANEC are non-perturbative in 1/α^2, or equivalently in hbar.
“In other words, the violations of ANEC are non-perturbative in 1/α2, or equivalently in h̄.”
Quote in the paperSubstantial claimClassified as probably not a substantial claim.
Premisecitation§ 1 + (µK)p+1Visser argues that the expected stress tensor far from the horizon will likely be approximately the same as the stress tensor for the static vacuum state outside a spherical star with radius close to its Schwarzschild radius.
“However, Visser argues that the expected stress tensor far from the horizon will likely be approximately the same as the stress tensor for the static vacuum state outside a spherical star with radius close to its Schwarschild radius.”
Quote in the paperSubstantial claimClassified as probably not a substantial claim.
Premisecitation§ 1 + (µK)p+1Visser has shown that the expected stress tensor of a scalar field in the Boulware vacuum outside a Schwarzschild black hole violates ANEC.
“As mentioned in the Introduction, in a very recent pa- per Visser [43] has shown that the expected stress ten- sor of a scalar field in the Boulware vacuum outside a Schwarzschild black hole violates ANEC.”
Quote in the paperSubstantial claim0 of 1 sources checked- cites [43]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
Probably not a substantial claim: may not pass S3 (load-bearing).
Premisecitation§ ACKNOWLEDGMENTSThis portion of the general solution was obtained by Horowitz.
“This portion of the general solution was obtained by Horowitz [48].”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [48]
Couldn’t be matched to a paper in Crossref, so it can’t be checked.
May combine two claims.
Interpretationreasoning§ 1 + (µK)p+1If L≫Lp, the quantum stress tensor can be treated as a small perturbation, and a leading-order approximation to the self-consistent solution is given by Eq. (E3).
“Therefore if L ≫ Lp, the quantum stress tensor can be treated as a small perturbation, and a leading or- der approximation to the self consistent solution will be given by”
Quote in the paperSubstantial claim
The authors state this as an assumption.
The state is sufficiently regular and the approach to flatness of the spacetime occurs at a sufficiently rapid rate that G(x, y) asymptotically approaches the two-point function Gin(x, y) of a state in Minkowski spacetime.
“First, we assume that the state is sufficiently reg- ular and that the approach to flatness of the spacetime occurs at a sufficiently rapid rate that G(x, y) asymp- totically approaches the two-point function Gin(x, y) of a state, ωin, in Minkowski spacetime (M,ηab).”
The authors state this as an assumption.
The prescription for obtaining the expected stress tensor satisfies the axioms discussed in Ref. [45].
“If we assume that the prescription for obtaining the expected stress tensor satisfies the axioms discussed in Ref. [45]”
The authors state this as an assumption.
The ambiguity in the expected stress tensor is only a two parameter ambiguity.
“This ambiguity is assumed to be only a two parameter ambiguity [60,61]”
The authors state this as an assumption.
Eq. (2.6) is not adequate for describing phenomena where wavelengths comparable to Lp occur.
“However, as already indicated above, we will not view Eq. (2.6) (or any other known equation) as adequate for describing phenomena where wavelengths comparable to Lp occur.”
The authors state this as an assumption.
The free parameters α and β are of order unity at the Planck scale, which translates to λ ∼ Lp and β ∼ 1.
“Note that our assumption discussed in Sec. II B that α and β are “of order unity at the Planck scale” translates into the assumption that λ ∼ Lp β ∼ 1.”
The authors state this as an assumption.
The semiclassical equations are approximate equations with domain of validity L ≫ Lp.
“we nevertheless view them as approximate equations, with domain of validity is L ≫ Lp.”
The authors state this as an assumption.
The uncalculated term 〈T(2)ab[h(1),h(1)],ωin,0〉 can be neglected in the long-wavelength limit.
“we will eventually pass to an approximation in which this term can be neglected (see subsection III E below).”
The paper relies on this without support.
The long-wavelength limit conditions encompass a wide range of physically interesting and potentially achievable situations.
“These conditions should encom- pass a wide range of physically interesting and potentially achievable situations.”
The authors state this as an assumption.
The electromagnetic self energy ~ q^2/L cannot exceed the externally measured mass-energy mc^2, i.e., the bare mass for a finite distribution of charge is always positive.
“assuming only that the electromagnetic self energy ∼”
The paper relies on this without support.
In semiclassical QED, the expected value of the current operator will not be concentrated at a point but will typically have a width of order L.
“since the expected value of the current operator will not”
The authors state this as an assumption.
The exact equation of motion including all higher order corrections is of the form a = a_ext + τ1 ȧ + α1 τ2^2 ä.
“suppose that the exact”
The authors state this as an assumption.
The incoming gravitational radiation satisfies condition (3.49).
“Now if we as- sume that the incoming gravitational radiation satisfies the condition (3.49)”
The authors state this as an assumption.
λ ∝ √h̄.
“(assuming λ ∝ √ h̄ as discussed in Sec. III E above)”
The paper relies on this without support.
For finite N, the unknown corrections to the right hand side of Eq. (3.38) have the form h̄^2/N L_ab[h^(1)] + h̄^2/N K_ab[ω^(1)_in] + O(h̄^3,1/N^2), where L_ab and K_ab are linear but otherwise unknown functionals.
“let us write the un- known corrections to the right hand side of Eq. (3.38), for finite N , as h̄2 N Lab[h (1)] + h̄2 N Kab[ω (1) in ] +O(h̄3, 1/N2), (4.22) where Lab and Kab are linear but otherwise unknown functionals”
The authors state this as an assumption.
Incoming gravitational radiation does not dominate the first-order metric perturbation.
“We restricted our analysis to the case where incoming gravitational radiation does not dominate the first order metric perturbation.”
“when we assume that incoming gravitational radiation does not dominate the first order metric perturbation.”
The authors state this as an assumption.
The argument for the vanishing of the second term in Eq. (7.7) can be restricted to Fock space states.
“We now restrict attention to the case of Fock space states.”
The authors state this as an assumption.
The second-order vacuum polarization term can be neglected in the long-wavelength expansion.
“As we have explained, the second order vacuum po- larization term 〈T (2) ab [h(1), h(1)], ωin,0〉 is not explicitly known, but arises at sufficiently high order in our long- wavelength expansion that it can be neglected, when we assume that incoming gravitational radiation does not dominate the first order metric perturbation.”
The authors state this as an assumption.
The paper assumes from now on that λ > λcrit.
“We assume from now on that λ > λcrit; however, it is possi- ble that the results in this appendix continue to hold for λ ≤ λcrit.”
The authors state this as an assumption.
The paper assumes that the functions F, ∂F/∂t, ∂F/∂t′, and ∂2F/(∂t∂t′) lie in class V: they are smooth and all their spatial derivatives are L1 on Σ×Σ.
“We assume that all these functions lie in the class V defined in Sec. VI — that is, that they are smooth and that all of their spatial derivatives are L1 on Σ × Σ.”
The paper relies on this without support.
The distance ∆ to the positive mass region is at least of order L.
“Since the distance ∆ to the positive mass region should be >∼ L”
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
Each contradiction between two passages listed here was confirmed by an independent check.
The gauge-transformation generators are reversed
MinorEquation (3.24) makes ξ(2), not ξ(1), the generator at first order in ε. That contradicts the first-order transformation rule in Eq. (3.29).
“ϕε = Dξ(2)(ε) ◦ Dξ(1)(ε2/2). (3.24)”
“T̄ (1) = T (1) + Lξ(1)T (0), (3.29)”
The second-order Einstein tensor uses a first-order state perturbation
MinorEquation (7.1) gives the leading term of the second-order Einstein tensor as the stress tensor of ω̄(1). The second-order equation (4.23) instead gives that leading term as the stress tensor of ω̄(2).
“Ḡ (2) ab = 〈T (0) ab , ω̄ (1) in 〉 +”
“κG (1) ab [ĥ(2)] = 1 α2 〈T (0) ab , ω̄ (2) in 〉 +”
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Sorted by citations
Energy conditions in general relativity and quantum field theory
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Null energy conditions in quantum field theory
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Energy conditions in the Jordan frame
Chatterjee, S., Easson, D. A., & Parikh, M. (2013) · Classical and Quantum Gravity · doi:10.1088/0264-9381/30/23/235031 · Cited by 25 · see citing works
- Authors
- Flanagan, E. E., & Wald, R. M.
- Affiliations
- University of Chicago (US)
- ORCID
- Wald, Robert M.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 1996-11-15
- Volume
- 54
- Issue
- 10
- Pages
- 6233-6283
- ISSN
- 0556-2821 (ISSN-L)
- 1089-4918
- OpenAlex
- W2100880655
- Semantic Scholar
- 130eaf79f17f3462d64b61968d5ad8a5118099f9
- Cited by
- 352
- References
- 64
- Citations by year
- 2026: 10 · 2025: 17 · 2024: 22 · 2023: 9 · 2022: 16 · 2021: 14 · 2020: 32 · 2019: 10 · 2018: 13 · 2017: 6 · 2016: 7 · 2015: 9 · 2014: 15 · 2013: 11 · 2012: 5
- FWCI
- 14.69
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Locations
- Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields (publishedVersion)
- PubMed (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Statistical and Nonlinear Physics › Noncommutative and Quantum Gravity Theories
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Black Holes and Theoretical Physics
- Keywords
- averaged null energy condition, semiclassical gravity, backreaction, renormalized stress-energy tensor, traversable wormholes, massless scalar field, curvature coupling, mixed quantum states, linearized Einstein equations, reduction of order, quantum field theory in curved spacetime
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