Quantum spin dynamics (QSD): V. Quantum gravity as the natural regulator of the Hamiltonian constraint of matter quantum field theories
Open accessAbstract
It is an old speculation in physics that, once the gravitational field is successfully quantized, it should serve as the natural regulator of infrared and ultraviolet singularities that plague quantum field theories in a background metric. We demonstrate that at least part of this idea is implemented in a precise sense within the framework of four-dimensional canonical Lorentzian quantum gravity in the continuum. Specifically, we show that the Hamiltonian of the standard model supports a representation in which finite linear combinations of Wilson loop functionals around closed loops, as well as along open lines with fermionic and Higgs field insertions at the end points, are densely defined operators. This Hamiltonian, surprisingly, does not suffer from any singularities, it is completely finite without renormalization. This property is shared by string theory. In contrast to string theory, however, we are dealing with a particular phase of the standard model coupled to gravity which is entirely non-perturbatively defined and second quantized . Of course, to show that the entire theory is finite requires more: one would need to know what the physical observables are, apart from the Hamiltonian constraint, and whether they are also finite. However, with the results given in this paper this question can now be answered, at least in principle.
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TL;DR
The paper argues that in four-dimensional canonical Lorentzian quantum gravity coupled to Standard Model matter, quantum gravity can act as a natural regulator: the matter Hamiltonian constraint becomes finite and densely defined without renormalization. It constructs regularized Yang–Mills, fermion, and Higgs contributions and checks consistency, weak anomaly-freeness, and some positivity properties.
Key findings
- The Yang–Mills, Dirac, and Higgs parts of the Hamiltonian constraint can be represented as densely defined operators on a spin-colour-network Hilbert space; ultraviolet and infrared singularities are absorbed by the quantum volume operator, so no renormalization is needed.
- The volume operator has a local action, vanishing except where string-like excitations begin or end, and its spectrum is discrete with volume quantum of order the Planck length cubed.
- The electric Yang–Mills piece and the Higgs kinetic term are positive semi-definite and essentially self-adjoint on the diffeomorphism-invariant Hilbert space, while positivity for each matter species separately depends on regularization and factor ordering; the full matter Hamiltonian is not symmetric.
- The constraint algebra is anomaly-free in a weak sense on diffeomorphism-invariant distributions, though the Dirac algebra is not faithfully represented; the paper also displays an uncountably infinite set of simple solutions.
Methods
- Canonical 3+1 Lorentzian gravity is coupled to gauge, fermion, and Higgs fields using real connection variables and half-density fermions; the kinematic Hilbert space combines Ashtekar–Lewandowski measures for the gauge sectors, a Berezin-type fermionic measure, and a Haar-measure construction for Higgs point holonomies.
- Regularization proceeds by point-splitting and triangulation adapted to graphs, absorbing inverse powers of the spatial volume into Poisson brackets with the volume functional, then replacing brackets by commutators and taking the continuum limit.
- Consistency checks include cylindrical consistency, diffeomorphism covariance, self-adjointness and positivity of selected pieces, anomaly-freeness on diffeomorphism-invariant states, and construction of simple solutions; no empirical data or sample is used.
Limitations
- The paper states that showing the entire theory is finite would require knowing the physical observables besides the Hamiltonian constraint and whether they are finite; this is not established here.
- Positivity of individual matter Hamiltonians is regularization- and factor-ordering-dependent, the full matter Hamiltonian is not symmetric, and anomaly-freeness is only demonstrated in a weak sense rather than as a faithful Dirac algebra.
- The paper states that no compact algorithm is available for the kernel of the Hamiltonian constraint in the matter-coupled case, so only trivial solutions are displayed; more broadly, the work is a theoretical construction without numerical or experimental validation.
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Claims the paper makes
0 of 37 cited sources checked · 0 supported · 0 flagged
- Findingreasoning
The electrical part of the Yang-Mills Hamiltonian has the final operator expression (3.8).
“The final expression for the electrical part of the Yang-Mills Hamiltonian is then given by”
Quote in the paperSubstantial claim - Findingnone given
There is no factor-ordering problem as to whether gravitational or gauge theory variables are ordered to the left or to the right.
“Notice that we have no factor ordering problem at all as far as the question, whether to order the gravitational or the gauge theory variables to the left or to the right, is concerned.”
Quote in the paperNot a substantial claim - Findingreasoning
The regularization of the Yang-Mills Hamiltonian constraint is furnished by the operator (3.11).
“This furnishes the regularization of the Yang-Mills Hamiltonian constraint.”
Quote in the paperSubstantial claim- The authors state this as an assumption: The three incident segments at a vertex are linearly independent, so their triple product is nonzero.
- Findingown data
For each matter species separately, whether the operators are positive semi-definite depends on the regularization and factor ordering.
“We find that, for each matter species separately, the answer is regularization and factor-ordering dependent.”
Quote in the paperSubstantial claim - Findingcitation
After operator (3.7) acts on a state, its dependence on s(e) disappears.
“After evaluating the operator on a state, the dependence on s(e) automatically drops out.”
Quote in the paperSubstantial claim
- Findingnone given
There are an uncountably infinite number of rigorous simple solutions to the full Hamiltonian constraint.
“demonstrate the non-triviality of the theory by displaying an uncountably infinite number of rigorous simple solutions.”
Quote in the paperSubstantial claim - Findingcitation
Operator (3.11) depends on the triangulation, partly through the freedom in choosing the loops α_ij.
“The label 'T ' on the operator in the first line of (3.11) is to indicate its dependence on the triangulation [11,12] which expresses itself partly in the huge freedom of how to choose the loops α ij .”
Quote in the paperNot a substantial claim0 of 2 sources checked- cites [11] Thiemann T Quantum spin dynamics (QSD): VI. Quantum Poincaré algebra, Class. Quantum Grav.
Not checked in the free run.
- cites [12] Thiemann T Anomaly-free formulation of non-perturbative
Not checked in the free run.
- Findingnone given
The final form of operator (3.7) is manifestly gauge invariant.
“Notice that the final form of the operator (3.7) is manifestly gauge invariant.”
Quote in the paperNot a substantial claim - Findingreasoning
The point-splitting volume factor is absorbed by a gravitational volume operator built from the spatial metric that measures the volume of spatial regions.
“It turns out that the point-splitting volume 3 is absorbed by a certain gravitational operator, built from q ab that measures the volume of spatial regions.”
Quote in the paperSubstantial claim - Findingreasoning
The Dirac-Einstein canonical action is derived in a manifestly real form and in terms of real connection variables.
“In the appendix we derive the Dirac-Einstein canonical action in a manifestly real form and in terms of the real connection variables”
Quote in the paperNot a substantial claim - Findingnone given
The magnetic part of the Yang-Mills Hamiltonian creates and annihilates new excitations, specifically new Wilson loop functions.
“the magnetic part creates and annihilates new excitations, that is, it creates new Wilson loop functions.”
Quote in the paperNot a substantial claim - Findingnone given
The fermion measure is gauge and diffeomorphism invariant.
“The fermion measure µ F is easily seen to be gauge and diffeomorphism invariant.”
Quote in the paperNot a substantial claim - Findingown data
The standard model Hamiltonian supports a representation in which finite linear combinations of Wilson loop functionals around closed loops, and along open lines with fermionic and Higgs field insertions at endpoints, are densely defined operators.
“Specifically, we show that the Hamiltonian of the standard model supports a representation in which finite linear combinations of Wilson loop functionals around closed loops, as well as along open lines with fermionic and Higgs field insertions at the end points, are densely defined operators.”
Quote in the paperSubstantial claim - Findingreasoning
The commutator is weakly equivalent to that operator because both act as zero operators on diffeomorphism-invariant states.
“Basically, one can show that the commutator is weakly equivalent to that operator because both are zero operators on diffeomorphism-invariant states.”
Quote in the paperSubstantial claim - Findingreasoning
Only tetrahedra whose basepoint coincides with a graph vertex contribute because of the volume operators.
“As we evaluate the operator we find out that only those tetrahedra in (3.10) contribute whose basepoint v( ) coincides with a vertex v of the graph due to the presence of the volume operators in (3.10).”
Quote in the paperSubstantial claim - Findingreasoning
The continuum limit δ→0 has already been taken in the diffeomorphism-invariant constraint equation.
“The limit δ → 0 is therefore already performed in (4.2) (see also [12]).”
Quote in the paperSubstantial claim0 of 1 sources checked- cites [12] Thiemann T Anomaly-free formulation of non-perturbative
Not checked in the free run.
- Findingreasoning
Every term in Ĥ_v contains a factor of the volume operator V_v, or a positive power of it, for an arbitrarily small neighbourhood of the vertex v.
“The crucial point is that all the terms involved in Ĥv involve a factor of the form Vv or more generally V n v , n > 0 where again this notation means the volume operator for an arbitrarily small neighbourhood of the vertex v.”
Quote in the paperSubstantial claim - Findingown data
A canonical point transformation from (K_i^a, E^a_i) to (A_i^a, E^a_i) can be performed, with generator ∫ d^3x i a E^a_i.
“We can now perform a canonical point transformation on the gravitational phase space given by (K i a , E a i ) → (A i a , E a i ) (the generator turns out to be d 3 x i a E a i as one can explicitly check)”
Quote in the paperSubstantial claim - Findingreasoning
The necessary and sufficient condition for the family of regulated operators to come from a single operator is that the projected operators vanish when the graph or colouring labels differ.
“The necessary and sufficient condition for this to be the case is that Ĥγ, λ pγ , λ = 0 whenever γ = γ or λ = λ .”
Quote in the paperSubstantial claim - Findingreasoning
Expanding F_ab and using the Bianchi identity, the vector constraint V_a is given up to a term proportional to G_j by equation (A.9).
“Next, we expand F ab in terms of a , K a , use the Bianchi identity tr R ab E b = 0 and find that the vector constraint V a , the coefficient of N a in S Dirac + S Einstein is given, up to a term proportional to G j , by V a = tr F ab E b + 1 2 i det(q)(ψ † D a ψ + η † D a η -CC).(A.9)”
Quote in the paperNot a substantial claim - Findingreasoning
The volume operator vanishes at the newly added vertices outside the original graph.
“Therefore, Vv = 0 for v ∈ γ (v)γ ∀v ∈ V (γ ).”
Quote in the paperSubstantial claim - Findingreasoning
Operator (3.7) no longer depends on the details of the partition.
“which does not depend on the details of the partition any longer because of which we could replace t 1 by !”
Quote in the paperSubstantial claim - Findingreasoning
The proof shows that ordering the momenta to the right was forced in order to obtain a densely defined operator.
“That we chose the momenta to the right was essentially forced on us because we want to obtain a densely defined operator: if the functional derivatives act on f m,n (Q) then in general it will not be true any longer that the operator only acts at the vertices of the state but at all vertices of the triangulation which are infinite in number and so the resulting state would not be normalizable.”
Quote in the paperSubstantial claim - Findingcitation
The regulated Hamiltonian constraint equation for diffeomorphism-invariant distributions is independent of the regularization parameter δ.
“The striking feature of (4.2) is that it is independent of the value of δ!”
Quote in the paperSubstantial claim - Findingreasoning
Because the decomposition is direct, there exist orthogonal projections from the full Hilbert space onto each colouring subspace.
“As the decomposition in (4.1) is direct there exist orthogonal projections pγ, λ H → H γ, λ .”
Quote in the paperSubstantial claim - Findingreasoning
The potential and cosmological constant terms are quantized as in (3.29).
“ĤHiggs,pot (N) f γ = m p 3 p v∈V (γ ) N v P (φ I φ I )(v) Vv f γ Ĥcosmo (N) f γ = m p λ 3 p v∈V (γ ) N v Vv f γ . (3.29)”
Quote in the paperSubstantial claim - Findingreasoning
On a cylindrical function, the Hamiltonian constraint of gravity and matter is a sum of vertex terms N_v Ĥ_v, where Ĥ_v is built from holonomies, gravitational volume operators, Yang-Mills Laplacians, fermion and Higgs derivatives, and fermion and Higgs insertions at vertices.
“To begin with, notice that when evaluated on a cylindrical function, the Hamiltonian constraint of both gravity and matter is a sum of terms of the structure N v Ĥv where Ĥv is an operator built from:”
Quote in the paperSubstantial claim - Findingreasoning
If f is cylindrical with respect to a graph γ, then Ĥ(N)f is generally cylindrical with respect to a graph γ(v) containing additional vertices that are co-planar or collinear.
“Notice that if f is a function cylindrical with respect to a graph γ then Ĥ (N)f = Ĥγ (N ) f = v∈V (γ ) N v Ĥv,γ f is in general a function cylindrical with respect to a graph γ (v) which contains additional vertices, but these vertices are co-planar (arising from loop-insertions due to the gravitational or magnetic part of the Yang-Mills Hamiltonian constraint) or collinear (arising from fermion”
Quote in the paperSubstantial claim - Findingreasoning
The complete space of solutions to both constraints is the set of infinite linear combinations of the averaged elements [s] for s in the orthogonal complement S of the union of the ranges of Ĥ(N).
“Then the complete space of solutions to both constraints is given by V phys the (infinite) linear combinations of elements of the set {[s] s ∈ S} ⊂ .”
Quote in the paperSubstantial claim - Findingreasoning
For Ô^{AB,I}_s defined as Ô^AB_s X^I_s, the adjoint is -Ô^{BA,I}_s.
“Next, using that X I s commutes with ÔAB s and that X I s † = -X I s is anti-self-adjoint on H we find for ÔAB,I s := ÔAB s X I s that ÔAB,I s † = -ÔBA,I s .”
Quote in the paperSubstantial claim - Findingreasoning
Operator (3.18) preserves the density weight one of the classical fermionic Hamiltonian constraint because θ are scalar-valued.
“Notice that the classical fermionic Hamiltonian constraint is a density of weight one and that the operator defined by (3.18) precisely respects this because the θ are scalar-valued and not density-valued.”
Quote in the paperSubstantial claim - Findingreasoning
A similar argument shows that the Dirac and Higgs Hamiltonians defined by the continuum prescription cannot be symmetric.
“A similar argument reveals that the Dirac and Higgs Hamiltonians as defined by (4.3) cannot be symmetric.”
Quote in the paperSubstantial claim - Findingreasoning
Only pairs of tetrahedra sharing the same basepoint contribute.
“Moreover, as we take sufficiently small we see that only pairs of tetrahedra contribute which have the same basepoint v( ) = v( ).”
Quote in the paperSubstantial claim - Findingreasoning
The adjoint of the operator Ô^AB_s equals +Ô^BA_s.
“ÔAB s † = V , h -1 s CB (h s ) AC = -[(h s ) BC , V ] h -1 s CA = -(h s ) BC h -1 s CA , V -(h s ) BC h -1 s CA , V = + ÔBA s . (4.5)”
Quote in the paperSubstantial claim - Findingreasoning
The alternative regularization scheme gives the same result (3.8) without taking limits.
“The result (3.8) is the same by construction, just that we did not need to take any limits and so the questionable interchange of limiting procedures is unnecessary.”
Quote in the paperNot a substantial claim - Findingreasoning
The change of variables to half-densities is a symplectomorphism.
“Note also that i √ det(q)[ψ † ψψ † ψ] = i[ξ † ξξ † ξ ] so that our change of variables is actually a symplectomorphism!”
Quote in the paperSubstantial claim - Findingreasoning
The contribution C from both the Einstein and Dirac sectors to the Hamiltonian constraint is given, up to a term proportional to the gravitational Gauss constraint, by equation (A.14).
“We end up with the contribution C from both the Einstein and Dirac sector to the Hamiltonian constraint which is given, up to a term proportional to the gravitational Gauss constraint, by C = H G + E a j 2 √ det(q) D a det(q) J j + i det(q)[ψ † σ j D a ψη † σ j D a η -CC] -K j a det(q)(ψ † ψη † η) . (A. 14)”
Quote in the paperSubstantial claim - Interpretationreasoning
In a diffeomorphism-invariant theory such as general relativity, coordinate volume cannot be measured by a fixed background metric but must be measured by the dynamical metric itself.
“the three-dimensional coordinate volume 3 cannot be measured by a fixed background metric in a diffeomorphism-invariant theory like general relativity, but must be measured by the dynamical metric q ab itself!”
Quote in the paperSubstantial claim - Premisecitation
The total ADM energy is non-negative.
“what only is important is that the total (ADM) energy is non-negative (see [10] for the pure gravity case).”
Quote in the paperSubstantial claim0 of 1 sources checked- cites [10] Baez J
Not checked in the free run.
- Interpretationreasoning
The local vanishing feature of the volume operator makes the Hamiltonian operators densely defined without introducing an infrared infinite-volume cut-off.
“It is this feature which makes the Hamiltonian operators densely defined without that we have to introduce an infrared (infinite-volume) cut-off.”
Quote in the paperSubstantial claim - Premisecitation
Spin-colour-network states form a basis for the subspace of gauge-invariant functions.
“These spin-colour-networks turn out to be a basis for the subspace of gauge-invariant functions.”
Quote in the paperSubstantial claim0 of 1 sources checked- cites [7] Thiemann T Kinematical Hilbert spaces for fermionic, Class. Quantum Grav.
Not checked in the free run.
- Premisecitation
Once the quantum configuration space is chosen, the Hilbert space is uniquely selected by the adjointness relations.
“one can show [7] that this is the unique Hilbert space selected by the adjointness relations, once we have chosen the space Ū as the quantum configuration space.”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [7] Thiemann T Kinematical Hilbert spaces for fermionic, Class. Quantum Grav.
Not checked in the free run.
- Interpretationown data
Within four-dimensional canonical Lorentzian quantum gravity in the continuum, at least part of the old idea that quantized gravity regulates ultraviolet and infrared singularities of matter quantum field theories is realized precisely.
“We demonstrate that at least part of this idea is implemented in a precise sense within the framework of four-dimensional canonical Lorentzian quantum gravity in the continuum.”
Quote in the paperSubstantial claim - Interpretationreasoning
The volume operator serves as the natural regulator of the matter quantum field theory Hamiltonian constraint by acting as a dynamical ultraviolet and infrared cut-off.
“In a sense, it is the volume operator which is the natural regulator of the matter quantum field theory Hamiltonian constraint by serving as a dynamical ultraviolet and infrared cut-off!”
Quote in the paperSubstantial claim - Premisecitation
Faithful implementation of the reality conditions forces a representation in which certain fermionic objects become densely defined multiplication operators.
“It turns out [7] that the faithful implementation of the reality conditions forces us to work in a representation in which the objects”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [7] Thiemann T Kinematical Hilbert spaces for fermionic, Class. Quantum Grav.
Not checked in the free run.
- Premisecitation
Ashtekar's canonical transformation makes the Hamiltonian constraint polynomial.
“The famous discovery due to Ashtekar [13] is that this is indeed possible by performing a certain canonical transformation on the gravitational phase space.”
Quote in the paperSubstantial claim0 of 1 sources checked- cites [13] source
Not checked in the free run.
- Premisecitation
A Gaussian measure for a scalar field, defined through its covariance, is always background dependent and therefore cannot be diffeomorphism invariant.
“a Gaussian measure for a scalar field, rigorously defined through its covariance, is always background dependent or, in other words, cannot be diffeomorphism invariant!”
Quote in the paperSubstantial claim0 of 1 sources checked- cites [7] Thiemann T Kinematical Hilbert spaces for fermionic, Class. Quantum Grav.
Not checked in the free run.
- Interpretationnone given
If the matter Hamiltonian operator is positive semi-definite, then its integral over any compact region and against a nonnegative lapse should also be positive semi-definite.
“if the matter Hamiltonian operator is positive semi-definite, then it is hard to imagine how that can be true if the Hamiltonian density does not, when integrated over any compact region of , also become a positive semi-definite operator.In particular, the matter Hamiltonian constraint when integrated against a nonnegative lapse function should also be a positive semi-definite operator.”
Quote in the paperSubstantial claim- Rests on an assumption: Classically, with unit lapse and positive spatial signature, the Yang-Mills and Higgs contribution to the integrated Hamiltonian constraint is non-negative and diffeomorphism invariant.
- Interpretationreasoning
The equality of the continuum and regulated matrix elements displays the matter Hamiltonian as a diffeomorphism-invariant operator.
“This displays Ĥ m as a diffeomorphism-invariant operator.”
Quote in the paperSubstantial claim - Interpretationreasoning
If the density weight were greater than one, the regulated operator would diverge at least as 1/ε^3.
“if it had been higher than one then we would have needed n + m + k -1 point splittings but in the denominator we have a power of √ det(q) which is smaller than n + m + k -1 and therefore even the regulated operator blows up at least as 1/ 3 .”
Quote in the paperSubstantial claim - Interpretationreasoning
When restricted to diffeomorphism-invariant states, the matter Hamiltonians come in units set by the Planck mass.
“It follows that in this sense the matter Hamiltonians are quantized in multiples of the Planck mass when we go to the diffeomorphism-invariant sector.”
Quote in the paperSubstantial claim - Interpretationreasoning
Replacing V(v,ε) by V_v is possible only in the quantum version.
“This replacement of V (v, ) by Vv is possible only in the quantum version where the square root of volume operator is defined via its spectral resolution and automatically takes care of its local action while in the classical computation we would have to keep the .”
Quote in the paperSubstantial claim - Interpretationreasoning
If the density weight were less than one, the regulated operator would vanish at least as ε^3.
“If it had been less than one then by a similar argument the regulated operator vanishes at least as 3 which is trivially always zero.”
Quote in the paperNot a substantial claim - Interpretationreasoning
A broad class of weight-one, diffeomorphism-covariant Hamiltonian densities coupled to gravity can be converted into densely defined and anomaly-free operators on the Hilbert space.
“In this subsection we describe a recipe by means of which a fairly large class of Hamiltonian densities of weight one which are diffeomorphism covariant and coupled to gravity can be turned into densely defined and, as we will see later, anomaly-free operators on the Hilbert space that we have defined.”
Quote in the paperSubstantial claim- The authors state this as an assumption: All covariant derivatives are with respect to A_i^a and A_I^a, act only on configuration scalars Q, and are first order only, so no Christoffel connection is needed.
- The authors state this as an assumption: The matter canonical momenta P are scalar densities of weight one and matter configuration variables are scalars, possibly transforming under SU(2)×G.
- Interpretationreasoning
Using ξ rather than θ would conflict with diffeomorphism covariance.
“If we were dealing with the ξ instead of the θ we would be running into conflict with diffeomorphism covariance at this point.”
Quote in the paperSubstantial claim - Interpretationreasoning
If one wants an anomaly-free quantum constraint algebra, one should not insist on a positive semi-definite Hamiltonian constraint operator.
“Therefore, if one wants an anomaly-free quantum constraint algebra then it seems that one should not insist on a positive semi-definite Hamiltonian constraint operator.”
Quote in the paperSubstantial claim- Rests on an assumption: On solutions, the gravitational and matter contributions to the Hamiltonian constraint are equal up to a sign.
- Premisecitation
The general solution of the diffeomorphism constraint for theories with fermions and Higgs fields is constructed in prior work and consists of elements of the dual space.
“The general solution of the diffeomorphism constraint for theories including fermions and Higgs fields is constructed in [7].As for the pure gauge field case [6], they are elements of .”
Quote in the paperNot a substantial claim0 of 2 sources checked- cites [7] Thiemann T Kinematical Hilbert spaces for fermionic, Class. Quantum Grav.
Not checked in the free run.
- cites [6] Ashtekar A, 1995, J. Math. Phys.
Not checked in the free run.
- Interpretationcitation
In the diffeomorphism-invariant setting, the size of the loops α_ij is irrelevant provided their attachment prescription is diffeomorphism covariant.
“This arbitrariness is somewhat reduced in the diffeomorphism-invariant context that we are interested in because then it does not matter how 'large' the loops α ij are as long as the prescription how to attach them is diffeomorphism covariant.”
Quote in the paperSubstantial claim0 of 2 sources checked- cites [11] Thiemann T Quantum spin dynamics (QSD): VI. Quantum Poincaré algebra, Class. Quantum Grav.
Not checked in the free run.
- cites [12] Thiemann T Anomaly-free formulation of non-perturbative
Not checked in the free run.
- May combine two claims. 49
- Classified as probably not a substantial claim. 12
May combine two claims.
FindingreasoningThe electric part of the Yang-Mills Hamiltonian becomes a sum of Laplace-Beltrami operators on G and is therefore sensitive to the colour of the state.
“the electric part of the Yang-Mills Hamiltonian becomes a sum of Laplace-Beltrami operators on G and therefore is sensitive to the colour of the state”
Quote in the paperNot a substantial claim- The authors state this as an assumption: The gauge group G is taken to be semi-simple up to U(1) factors, and Lie algebra indices are raised and lowered with the Cartan-Killing metric.
Probably not a substantial claim: may not pass S3 (load-bearing), S4 (based).
Findingnone givenThe action of the Higgs field Hamiltonian is analogous to that of the gauge field.
“The action of that Hamiltonian is analogous to that of the gauge field.”
Quote in the paperNot a substantial claim- The authors state this as an assumption: The Higgs field is taken to transform in the adjoint representation of G.
May combine two claims.
FindingreasoningWhen the triangulation is refined indefinitely, the continuum limit exists and yields well-defined operators on the diffeomorphism-invariant Hilbert space.
“When refining the triangulation ad infinitum we find that the continuum limit exists and yields well defined operators on this diffeomorphism-invariant Hilbert space.”
Quote in the paperSubstantial claimMay combine two claims.
FindingreasoningThis Hamiltonian has no singularities and is completely finite without renormalization.
“This Hamiltonian, surprisingly, does not suffer from any singularities, it is completely finite without renormalization.”
Quote in the paperSubstantial claimMay combine two claims.
Findingown dataThe continuum limit of the triangulation regularization for matter Hamiltonians exists, and the action of the continuum operator can be displayed precisely.
“We show that it exists and are able to display the action of the continuum operator precisely.”
Quote in the paperSubstantial claimMay combine two claims.
FindingreasoningBecause the total measure is a probability measure, gauge-invariant functions remain integrable and the gauge group volume equals unity.
“It turns out that, because our total measure is a probability measure, gauge-invariant functions will still be integrable with respect to it, in other words, 'the gauge group volume' equals unity in our case!”
Quote in the paperNot a substantial claim- The authors state this as an assumption: The gauge group G is taken to be semi-simple up to U(1) factors, and Lie algebra indices are raised and lowered with the Cartan-Killing metric.
May combine two claims.
Findingnone givenThe fermionic Hamiltonian operator removes fermionic excitations from open string endpoints and creates new excitations on the open string.
“The fermionic Hamiltonian operator removes fermionic excitations from open string endpoints and creates new excitations on the open string.”
Quote in the paperNot a substantial claimMay combine two claims.
FindingreasoningThe matter field theory Hamiltonian constraint is ultraviolet and infrared divergent without gravity and needs renormalization, but is convergent with gravity without renormalization.
“the matter field theory Hamiltonian constraint is ultraviolet and infrared (i) divergent without gravity and needs to be renormalized but are (ii) convergent with gravity without that renormalization is necessary.”
Quote in the paperSubstantial claimMay combine two claims.
FindingreasoningNo singularities are encountered at any stage, and the final regularized matter operators do not require renormalization.
“At no stage do we encounter any singularities, these final operators do not require any renormalization.”
Quote in the paperSubstantial claimMay combine two claims.
Findingnone givenThe volume operator has a local action and vanishes everywhere except at points where a string ends or starts.
“This volume operator turns out to have a quite local action, it vanishes everywhere except at points where the string ends or starts.”
Quote in the paperSubstantial claimMay combine two claims.
Findingnone givenFor a fixed graph, the graph Hilbert space is infinite-dimensional and is the completion of spin-colour-network functions, while each colouring subspace is finite-dimensional with dimension equal to the number of independent gauge-invariant projectors compatible with that colouring.
“The Hilbert space H γ is infinite dimensional and is the completion of the space of functions built from spin-colour-network states on γ while H γ, λ is a finite dimensional vector space with dimension equal to the number of linearly independent projectors on gauge-invariant functions compatible with the colouring λ of γ .”
Quote in the paperSubstantial claimClassified as probably not a substantial claim.
FindingcitationEvery cylindrical function is averaged term-by-term after it is decomposed into spin-colour-network states.
“Furthermore, we have [f ] := I c I [T I ], that is, every f ∈ gets averaged term-wise after decomposing it into spin-colour-network states”
Quote in the paperSubstantial claimClassified as probably not a substantial claim.
FindingreasoningThe Einstein contribution to the Hamiltonian constraint of the combined Dirac and Einstein action is H_G as given in equation (A.11).
“Then the Einstein contribution to the Hamiltonian constraint of S Dirac + S Einstein is given by H G := -H E + 2 2κ tr [K a , K b ] E a , E b √ det(q) (A”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
FindingreasoningUsing D_a E^a_i = 0, the Gauss constraint can be written as equation (A.8).
“Using that D a E a i = 0 we can immediately write G j = 1 κ D a E a j + i det(q)[ψ † τ j ψ + η † τ j η]. (A.8)”
Quote in the paperNot a substantial claimMay combine two claims.
Findingnone givenThe electric piece of the Yang-Mills Hamiltonian and the term bilinear in Higgs momenta are essentially self-adjoint and positive semi-definite on the diffeomorphism-invariant Hilbert space.
“(iii) The electric piece of the Yang-Mills Hamiltonian and the term bi-linear in the Higgs momenta are indeed essentially self-adjoint and positive semi-definite operators on the diffeomorphism-invariant Hilbert space.”
Quote in the paperSubstantial claimMay combine two claims.
FindingcitationThe Dirac algebra is not faithfully represented, but the algebra is non-anomalous in the sense that a consistent quantum theory is obtained.
“(i) As we will see in the next section, the Dirac algebra is indeed not faithfully represented (one could, however, use the arguments of [27] to improve this), but still the algebra is non-anomalous in the sense that we obtain a consistent quantum theory”
Quote in the paperSubstantial claim0 of 1 sources checked- cites [27] source
Not checked in the free run.
May combine two claims.
FindingreasoningTrivial solutions include distributions defined on graphs whose vertices are all co-planar, because the volume operator annihilates such states so they cannot lie in the image of the Hamiltonian constraint; their fermion and Higgs dependence is arbitrary.
“Trivial solutions are, for instance, distributions which are defined by graphs all of whose vertices are co-planar, just because the volume operator annihilates such states so that they cannot be in the image of the Hamiltonian constraint.The dependence on fermion and Higgs fields of these solutions is completely arbitrary.”
Quote in the paperSubstantial claimMay combine two claims.
FindingreasoningThe matrix element of the regulated matter Hamiltonian between diffeomorphism-averaged states is independent of δ and constant, so the limit is trivial and equals the regulated matrix element for any positive δ.
“since [T I ] is diffeomorphism invariant, this number, as explained in (4.2), does not depend on δ > 0 (the size or shape of the loop attached) and so is a constant.The limit is therefore trivial and so [T I ], Ĥ m [T J ] Diff = [T I ] Ĥ m δ T J (4.4) for any δ > 0.”
Quote in the paperSubstantial claimMay combine two claims.
FindingreasoningThe Hilbert space splits into an uncountable direct sum over graphs and, for each graph, a countable direct sum over compatible colorings.
“H = ⊕ γ H γ , H γ = ⊕ λ H γ, λ(4.1)”
- Also stated in: § 4.1. Cylindrical consistency · plain
“where the first direct sum is an uncountable one while the second is a countable one, running over the possible colourings of the graph with the various compatible irreducible representations”
Quote in the paperSubstantial claim- Also stated in: § 4.1. Cylindrical consistency · plain
Probably not a substantial claim: may not pass S3 (load-bearing), S4 (based).
Findingnone givenEquation (3.28) defines a densely defined operator.
“Again, despite its complicated appearance, equation (3.28) defines a densely defined operator.”
Quote in the paperNot a substantial claimMay combine two claims.
Findingown dataNo compact algorithm for describing S in the matter-coupled case is available, so the paper restricts to trivial solutions, which is enough to show the theory is not empty.
“We see that we know the space of solutions once we know S. A compact algorithm to describe S as for the source-free case is not available at the moment for the matter coupled case so we restrict ourselves to displaying trivial solutions which is enough to show that the theory is not empty.”
Quote in the paperSubstantial claimMay combine two claims.
FindingcitationThe two functions appearing in the commutator are related by an analyticity-preserving diffeomorphism, which completes the proof of anomaly-freeness.
“It is then easy to see, by the same argument as in [12], that the two functions Ĥγ (v),v Ĥγ,v f, Ĥγ,v Ĥγ(v ),v f are related by an analyticity preserving diffeomorphism.This furnishes the proof of anomaly-freeness.”
Quote in the paperSubstantial claim0 of 1 sources checked- cites [12] Thiemann T Anomaly-free formulation of non-perturbative
Not checked in the free run.
May combine two claims.
FindingreasoningThe electric piece of the Yang-Mills Hamiltonian is densely defined, positive definite and essentially self-adjoint even on the auxiliary Hilbert space; a similar result holds for the Higgs momentum bilinear.
“Let us then conclude this subsection by showing that the electric piece of the Yang-Mills Hamiltonian is a densely defined, positive definite essentially self-adjoint operator even on the auxiliary Hilbert space H.A similar argument applies to the p I p I part of the Higgs Hamiltonian.”
Quote in the paperSubstantial claimMay combine two claims.
FindingreasoningFor every Hamiltonian constraint matching (3.30), the construction yields an operator on H that is densely defined, diffeomorphism covariant, and free of anomalies.
“Theorem 3.1 (structure theorem).Any Hamiltonian constraint of the form (3.30) can be turned into a densely defined operator on H which is diffeomorphism covariantly defined and anomaly free.”
Quote in the paperSubstantial claim- The authors state this as an assumption: All covariant derivatives are with respect to A_i^a and A_I^a, act only on configuration scalars Q, and are first order only, so no Christoffel connection is needed.
- The authors state this as an assumption: The matter canonical momenta P are scalar densities of weight one and matter configuration variables are scalars, possibly transforming under SU(2)×G.
Classified as probably not a substantial claim.
FindingreasoningThe Hamiltonian constraint can be written as H = H_G + T, where T is the correction term in equation (A.12).
“H = H G - 2 2κ D a tr K b , E b E a √ det(q) =: H G + T . (A.12)”
Quote in the paperSubstantial claimMay combine two claims.
FindingcitationThe electric part no longer depends on the regulator, so its continuum limit is already taken, and it projects to a strongly diffeomorphism-invariant self-adjoint positive semi-definite operator on the Hilbert space defined by the continuum prescription.
“Notice also that the electric part does not depend on the regulator δ any longer so that the continuum limit is already taken.It therefore projects to a strongly diffeomorphisminvariant self-adjoint and positive semi-definite operator on the Hilbert space defined by (4.3) by general theorems proved in [6].”
Quote in the paperSubstantial claim0 of 1 sources checked- cites [6] Ashtekar A, 1995, J. Math. Phys.
Not checked in the free run.
May combine two claims.
FindingreasoningThe Hamiltonian can be written as a sum of operators of the form †Â, so its projections are positive semi-definite and symmetric.
“Putting everything together we find that when setting whence we have displayed Ĥ in the form of a sum of operators of the form  † Â, that is, it has positive semi-definite and symmetric projections.”
Quote in the paperSubstantial claimMay combine two claims.
FindingreasoningEquation (3.8) does not depend on δ, so taking a limit is unnecessary.
“Now, since (3.8) actually is independent of δ, no limit needs to be taken.”
Quote in the paperNot a substantial claimMay combine two claims.
FindingreasoningThe full matter Hamiltonian operator as constructed in the paper is not symmetric but is diffeomorphism invariant.
“(ii) The full matter Hamiltonian operator, as it stands in this paper, is not symmetric but at least it is diffeomorphism invariant”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
FindingreasoningAfter lengthy computation, the Dirac action can be written in terms of Weyl spinors as equation (A.2).
“one sees that the action can be written, after lengthy computations, in terms of Weyl spinors as (using the Weyl representation for the Dirac matrices, for instance, to expand out various terms) S Dirac = 1 2 i R dt d 3 x N det(q) T a -N a N ψ † ∇ + a ψ + η † ∇ - a η -CC +e a i ψ † σ i ∇ + a ψ -η † σ i ∇ - a η -CC (A.2)”
Quote in the paperNot a substantial claimMay combine two claims.
FindingreasoningEvery matter Hamiltonian acts discretely on a cylindrical function and carries an overall factor of the Planck mass over a Planck-length power that offsets the volume operator.
“Notice that all Hamiltonians have the same structure, namely an operator which carries out a discrete operation on a cylindrical function, like adding or subtracting lines, fermions or Higgs fields, multiplied by the Planck mass and divided by an appropriate power of the Planck length which compensates the power of the Planck length coming from the action of the volume operator.”
Quote in the paperSubstantial claimMay combine two claims.
FindingreasoningThe continuum matter Hamiltonian is not even symmetric; a pure Yang-Mills counterexample demonstrates this.
“We will now demonstrate that (4.4) is not even symmetric.We restrict ourselves to the case that we couple only a pure Yang-Mills field.We just need one counterexample.”
- Also stated in: § 4.2. Diffeomorphism-covariance, continuum limit self-adjointness and positive semi-definiteness · boosted
“It follows that [T J ] Ĥ B Y M,δ T J = 0 thus contradicting symmetry.”
Quote in the paperSubstantial claim- Also stated in: § 4.2. Diffeomorphism-covariance, continuum limit self-adjointness and positive semi-definiteness · boosted
May combine two claims.
FindingreasoningDefining the full operator as the sum of the projected regulated operators makes the cylindrical consistency condition hold by construction, which proves consistency.
“But this is the case by construction if we simply define Ĥ := γ, λ Ĥγ, λ pγ, λ .This suffices to prove consistency.”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S4 (based).
Findingnone givenThe Higgs kinetic operator (3.23) is densely defined.
“The operator (3.23) is certainly quite complicated but it is densely defined!”
Quote in the paperNot a substantial claimMay combine two claims.
Findingnone givenThe resulting expression has factor ordering ambiguity but no factor ordering singularity.
“The resulting expression does suffer from a factor ordering ambiguity but not from a factor ordering singularity.”
Quote in the paperSubstantial claimMay combine two claims.
FindingcitationBecause the projections preserve each colouring subspace, the family defines a positive symmetric operator on the full Hilbert space, which has self-adjoint extensions; each projection and the whole operator are essentially self-adjoint, making the extension unique.
“Since these projections map H γ, λ into itself (the dependence on the segments s(e) involved in the definition of Ĥ E Y M drops out because of gauge invariance, see [24]), it follows that the family of projections defines a positive and symmetric operator on H which therefore has self-adjoint extensions (actually, by methods similar as for the volume, area and length operators [21][22][23][24] one”
Quote in the paperSubstantial claim0 of 1 sources checked- cites [21][22][23][24]
Not checked in the free run.
May combine two claims.
FindingreasoningThe sum in (3.11) runs only over graph vertices and, for each vertex, tetrahedra based there.
“Combining both observations, we find that we need to sum only over vertices of the graph and for each vertex v over those tetrahedra such that v( ) = v.”
Quote in the paperSubstantial claimMay combine two claims.
FindingreasoningThe commutator of two Hamiltonian constraints on a cylindrical function reduces to the expression (4.7); terms with equal vertices vanish, and for unequal vertices the local character of the vertex operator makes the relevant operators commute.
“In the last step we used that the terms with v = v trivially vanish while for the terms with v = v the local character of the operator Ĥγ,v , performing changes of γ only in a neighbourhood of v makes it commute with Ĥγ (v),v .”
Quote in the paperSubstantial claimMay combine two claims.
FindingcitationThe continuum limit is taken after integration; the limit before integration does not exist in the L2 sense.
“Notice that, just as in the continuum limit of a regulated Euclidean path integral of constructive quantum field theory, we take the limit after integrating.Indeed, the limit before integrating does not exist in the L 2 sense (for the same reason that the generator of the diffeomorphism constraint does not exist [6]).”
Quote in the paperSubstantial claim0 of 1 sources checked- cites [6] Ashtekar A, 1995, J. Math. Phys.
Not checked in the free run.
May combine two claims.
FindingreasoningUp to the K_i^a term, the constraint (A.15) is expressed in real-valued quantities and the canonically conjugate pairs (ξ, iξ) and (ρ, iρ).
“This is the form of the constraint that we have been looking for: up to K i a we have expressed everything in terms of real-valued quantities and the canonically conjugate pairs (ξ, i ξ), (ρ, i ρ).”
Quote in the paperSubstantial claimMay combine two claims.
FindingreasoningIn the source-free case the correction T is proportional to the Gauss constraint and vanishes on the constraint surface; in the matter-coupled case, using the Gauss constraint, T is given by equation (A.13) with current J^j = ψ†σ^jψ + η†σ^jη.
“Notice that in the source-free case the correction T of H to H G is proportional to a Gauss constraint and therefore would vanish separately on the constraint surface.However, in our case, using the Gauss constraint (A.7) we find that T = -1 2 K a , E a j -E a j D a J j (A.13) where we have defined the current J j = ψ † σ j ψ + η † σ j η.”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
FindingreasoningEquation (A.14) can be rewritten in terms of half-densities ξ and ρ as equation (A.15).
“Notice that we can write (A.14) also in terms of the half-densities ξ = 4 √ det(q)ψ, ρ = 4 √ det(q)η by absorbing the √ det(q) appropriately and using that D a det(q) = 0. We find C = H G + E a j 2 √ det(q) D a (ξ † σ j ξ + ρ † σ j ρ) +i[ξ † σ j D a ξ -ρ † σ j D a ρ -CC] -K j a (ξ † ξ -ρ † ρ) . (A.15)”
Quote in the paperNot a substantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
PremisecitationA real-valued Ashtekar connection can be used at the cost of a fairly complicated Lorentzian Hamiltonian constraint.
“one can also use a real-valued Ashtekar connection A i a = i a + K i a at the price of living with a fairly complicated Lorentzian Hamiltonian constraint.”
Quote in the paperNot a substantial claim0 of 1 sources checked- cites [14] Thiemann T, 1998, Class. Quantum Grav. source
Not checked in the free run.
May combine two claims.
InterpretationreasoningThe theory considered is a particular phase of the standard model coupled to gravity that is entirely non-perturbatively defined and second quantized.
“In contrast to string theory, however, we are dealing with a particular phase of the standard model coupled to gravity which is entirely non-perturbatively defined and second quantized.”
Quote in the paperSubstantial claimMay combine two claims.
PremisecitationThe volume is quantized with a discrete spectrum, and the quantum of volume is of order the Planck volume.
“the volume is quantized with a discrete spectrum, the quantum of volume being indeed of order 3 p (see [20,21])!”
Quote in the paperSubstantial claim0 of 2 sources checked- cites [20] Thiemann T Reality conditions inducing transforms for quantum gauge field theory
Not checked in the free run.
- cites [21] Thiemann T, 1996, Class. Quantum Grav. source
Not checked in the free run.
May combine two claims.
InterpretationcitationThe gravitational connection is real only when fermions are represented by half-density variables; using scalar variables makes the connection complex.
“As we will see in the appendix, the connection is real only if we use the quantities ξ with density weight 1 2 , if we would use the scalar variables η as in [9] then the gravitational connection becomes by the argument given in [18] A”
Quote in the paperSubstantial claim0 of 2 sources checkedMay combine two claims.
InterpretationreasoningThe fermionic excitations produced by this regularization differ greatly from those in the cited earlier work, because the reality conditions are faithfully implemented.
“Quite surprisingly, these fermionic excitations are very different from those discussed in [8,9], the underlying reason being the faithful implementation of the reality conditions.”
Quote in the paperNot a substantial claim0 of 2 sources checkedMay combine two claims.
InterpretationreasoningBecause the volume operator is densely defined on the Hilbert space, the ultraviolet singularity is removed by coupling quantum gravity without renormalization, restoring diffeomorphism covariance.
“Since this volume operator turns out to be densely defined on the Hilbert space the UV singularity 1/ 3 is removed by coupling quantum gravity, without renormalization, thereby reinstalling diffeomorphism covariance.”
Quote in the paperSubstantial claimProbably not a substantial claim: may not pass S3 (load-bearing).
PremisereasoningThe canonical action principle for general relativity coupled to Dirac fields in manifestly real form and in terms of the canonical pair A_i^a, E^a_i had not been derived in the literature before this work.
“In this section we wish to derive the canonical action principle for general relativity coupled to Dirac fields in manifestly real form and in terms of the canonical pair A i a = i a +K i a , E a i introduced in section 2. This has not been done so far in the literature because either one was interested in the standard Palatini formulation or in the Ashtekar formulation, the latter”
Quote in the paperNot a substantial claimClassified as probably not a substantial claim.
Interpretationnone givenThe 3+1 split Dirac action is to be combined with the 3+1 split Einstein action to obtain the desired form in terms of A_i^a and E^a_i.
“This is the 3 + 1 split Dirac action that we are going to combine with the 3 + 1 split Einstein action to obtain the desired form in terms of A i a , E a i .”
Quote in the paperSubstantial claimMay combine two claims.
PremisecitationAchieving the more ambitious goal that the commutator equal an operator proportional to a diffeomorphism generator is difficult because the diffeomorphism generator does not exist in the chosen representation and because an operator corresponding to q^ab is not obvious to construct.
“The difficulty in achieving this more ambitious goal is twofold as pointed out already in [12]: first, not even the generator of a one-parameter family of diffeomorphisms exists in the representation that we have chosen since the associated representation of the diffeomorphism group does not act strongly continuously on the Hilbert space.Secondly, since {H (M), H (N )} = V a q ab (M ,b N -MN ,b )”
Quote in the paperSubstantial claim0 of 1 sources checked- cites [12] Thiemann T Anomaly-free formulation of non-perturbative
Not checked in the free run.
May combine two claims.
PremisecitationThe diffeomorphism-averaged spin-colour-network object is a well-defined distribution and the averaged states form an orthonormal basis of the diffeomorphism-invariant Hilbert space.
“As shown in [6,7], the following object makes sense as a distribution on : [T I ] := T ∈{T I } T , where {T I } := { Û(ϕ)T I : ϕ ∈ Diff( )} is the orbit of the vector T I under the diffeomorphism group.Moreover, as one can show, the [T I ] provide an orthonormal basis on the diffeomorphism-invariant Hilbert space”
Quote in the paperSubstantial claim0 of 2 sources checked- cites [6] Ashtekar A, 1995, J. Math. Phys.
Not checked in the free run.
- cites [7] Thiemann T Kinematical Hilbert spaces for fermionic, Class. Quantum Grav.
Not checked in the free run.
May combine two claims.
InterpretationreasoningThe theorem is inapplicable in one spatial dimension, where all tensors are densities, and in zero spatial dimension, where there is no field theory.
“However, in one spatial dimension all tensors are densities and in zero spatial dimension we do not have a field theory so that the theorem does not apply in these cases anyway.”
Quote in the paperNot a substantial claimMay combine two claims.
PremisecitationAn operator corresponding to q^ab V_b has been constructed in prior work, and part of it generates diffeomorphisms.
“Indeed, in [26] such an operator is constructed and part of it actually does generate diffeomorphisms!”
Quote in the paperSubstantial claim0 of 1 sources checked- cites [26] source
Not checked in the free run.
May combine two claims.
InterpretationcitationThe δ-independence is due to the diffeomorphism covariance of the graph-dependent triangulation prescription, a result proved for the gravitational part and asserted to carry over to the matter-coupled case.
“The underlying reason for this is the diffeomorphism covariance of the graph-dependent triangulation prescription.This is proved in [12,26] for the gravitational part of the Hamiltonian constraint and the same reasoning applies to the matter coupled case as well and will not be repeated here.”
Quote in the paperSubstantial claim0 of 2 sources checked- cites [12] Thiemann T Anomaly-free formulation of non-perturbative
Not checked in the free run.
- cites [26] source
Not checked in the free run.
- Rests on an assumption: The reasoning that proves δ-independence for the gravitational Hamiltonian constraint also applies to the matter-coupled case.
May combine two claims.
InterpretationreasoningThe construction applies in every spatial dimension d at least 2, since the inequality dk > n+m+k−1 admits a k for arbitrary n,m exactly when d exceeds 1.
“The theorem works the same way in any dimension d 2 because the critical condition dk > n + m + k -1 can be satisfied by some k for any value of n, m only for d > 1.”
Quote in the paperSubstantial claimMay combine two claims.
InterpretationcitationA symmetric Hamiltonian constraint operator risks conflicting with faithful implementation of the Dirac constraint algebra, and a quantum anomaly is expected in that case.
“Now, by arguments explained in [25], a symmetric Hamiltonian constraint operator is in danger of being in conflict with the task of faithfully implementing the Dirac constraint algebra.Most certainly, one expects a quantum anomaly in this case.”
Quote in the paperSubstantial claim0 of 1 sources checked- cites [25] Choquet-Bruhat Y, 1989
Not checked in the free run.
May combine two claims.
InterpretationcitationBecause V and H_E(1) admit well-defined quantizations, equation (A.15) also admits a well-defined quantization despite its complicated appearance.
“Then it is still true that K j a = -A j a , {V , H E (1)} and since V , H E (1) admit well defined quantizations [12] we conclude that despite its complicated Quantum spin dynamics (QSD): V 1313 appearance (A.15) admits a well defined quantization as well.”
Quote in the paperSubstantial claim0 of 1 sources checked- cites [12] Thiemann T Anomaly-free formulation of non-perturbative
Not checked in the free run.
May combine two claims.
InterpretationreasoningIf one used ψ and η instead of half-densities, the gravitational connection would acquire a correction proportional to i e_i^a(ψ†ψ + η†η), forcing a complex connection that would be disastrous because the Hilbert space techniques would not be available.
“Note that if we had not worked with half-densities ξ, ρ but with the ψ, η then, while i √ det(q) ψ is the momentum conjugate to ψ, the gravitational connection would get a correction proportional to ie i a [ψ † ψ + η † η].Thus we would have had to admit a complex connection which would be disasterous as the Hilbert space techniques [1][2][3][4][5][6] would not be at our disposal.”
Quote in the paperSubstantial claim0 of 1 sources checked- cites [1][2][3][4][5][6]
Not checked in the free run.
May combine two claims.
InterpretationreasoningThe strategy of working with ψ as advertised in prior work is not suitable for quantizing the Einstein-Dirac theory, so the framework developed in another prior work is forced.
“Therefore the strategy of working with ψ as advertised in [9] is not suitable for quantizing the Einstein-Dirac theory and we are forced to adapt the framework developed in [7].”
Quote in the paperSubstantial claim0 of 2 sources checked- cites [9] source
Not checked in the free run.
- cites [7] Thiemann T Kinematical Hilbert spaces for fermionic, Class. Quantum Grav.
Not checked in the free run.
May combine two claims.
PremisecitationThe classical limit schemes lim_{ε→0} lim_{δ→0} and (lim_{δ→0})|_{ε=δ} are identical and both give back the classical magnetic Hamiltonian constraint.
“This is justified because the classical limit schemes lim →0 lim δ→0 and (lim δ→0 ) | = (δ), (0)=0 are identical, both give back the classical magnetic Hamiltonian constraint.”
Quote in the paperSubstantial claim0 of 1 sources checked- cites [27] source
Not checked in the free run.
The authors state this as an assumption.
The gauge group G is taken to be semi-simple up to U(1) factors, and Lie algebra indices are raised and lowered with the Cartan-Killing metric.
“Here and in what follows we assume that indices I, J, K, . . .are raised and lowered with the Cartan-Killing metric δ I J of G which we take to be semi-simple up to factors of U (1).”
The authors state this as an assumption.
The Higgs field is taken to transform in the adjoint representation of G.
“Here and in what follows we have taken the Higgs field to transform according to the adjoint representation of G”
The authors state this as an assumption.
The three incident segments at a vertex are linearly independent, so their triple product is nonzero.
“We have assumed that abc ṡa 1 ṡb 2 ṡc 3 0.”
The authors state this as an assumption.
All covariant derivatives are with respect to A_i^a and A_I^a, act only on configuration scalars Q, and are first order only, so no Christoffel connection is needed.
“Furthermore, it is assumed that all covariant derivatives are with respect to A i a , A I a , act only on configuration scalars Q and are of first order only so that no Christoffel connection is needed.”
The authors state this as an assumption.
The matter canonical momenta P are scalar densities of weight one and matter configuration variables are scalars, possibly transforming under SU(2)×G.
“The matter canonical momenta P of the theory are scalar densities of weight one and matter configuration variables are scalars (they may transform non-trivially under SU (2) × G).”
The paper relies on this without support.
On solutions, the gravitational and matter contributions to the Hamiltonian constraint are equal up to a sign.
“but, at least on solutions, the gravitational and matter contribution just equal each other up to a sign and therefore necessarily the gravitational piece is also symmetric if the matter piece is.”
The paper relies on this without support.
The reasoning that proves δ-independence for the gravitational Hamiltonian constraint also applies to the matter-coupled case.
“This is proved in [12,26] for the gravitational part of the Hamiltonian constraint and the same reasoning applies to the matter coupled case as well and will not be repeated here.”
The paper relies on this without support.
The kernel of the Hamiltonian constraint exists even though no explicit algorithm for constructing it is given.
“While we do not have an explicit algorithm for the construction of the kernel at the moment, it is clear that it exists and therefore one can construct a physical inner product and strict Dirac observables as outlined in [26].”
The paper relies on this without support.
Classically, with unit lapse and positive spatial signature, the Yang-Mills and Higgs contribution to the integrated Hamiltonian constraint is non-negative and diffeomorphism invariant.
“If we set N = 1 and the spatial metric has signature (+, +, +) then the matter contribution to the integrated Hamiltonian constraint, at least for the Yang-Mills and the Higgs part, is classically a manifestly non-negative and diffeomorphism-invariant functional.”
The paper relies on this without support.
The set of piecewise analytical graphs is uncountably infinite.
“The set of labels I is an uncountably infinite one because the set of piecewise analytical graphs of has this cardinality.”
The paper relies on this without support.
For compatible colorings, there exist projectors that render the associated cylindrical functions gauge invariant.
“compatible in the sense that there exist projectors which render the associated cylindrical functions into gauge-invariant ones.”
Claims other papers make about this one
Each is checked against this paper’s own text: does it say what the citing paper says it does?
The discrete quantum geometry in loop quantum gravity acts as a physical Planck-scale regulator, eliminating ultraviolet divergences.
“the fundamental discreteness of quantum geometry in LQG plays the role of physical regulator at the Planck scale [354].”
From The Spin-Foam Approach to Quantum Gravity (2013) · cites this paper as [354]
Proposed quantizations of the scalar constraint in loop quantum gravity yield well-defined operators without ultraviolet divergences, but whether they are anomaly-free remains an open question.
“Concrete quantizations producing well-defined operators are available: no UV divergences are encountered by these proposals; the fundamental discreteness of quantum geometry in LQG plays the role of physical regulator at the Planck scale [354].”
From The Spin-Foam Approach to Quantum Gravity (2013) · cites this paper as [354]
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Ashtekar, A., & Lewandowski, J. (1997) · arXiv (Cornell University) · doi:10.48550/arxiv.gr-qc/9711031 · Cited by 11 · see citing works
A Generalized Wick Transform for GravityPreprint
Ashtekar, A. (1995) · arXiv (Cornell University) · doi:10.48550/arxiv.gr-qc/9511083
Flagged first, then by citations
Research works printed but not linked: 5
- Ashtekar A, 1995, J. Math. Phys., 36, 519
- Thiemann T Kinematical Hilbert spaces for fermionic, Class. Quantum Grav.
- Thiemann T Quantum spin dynamics (QSD): VI. Quantum Poincaré algebra, Class. Quantum Grav., 15
- Thiemann T Complete formula for the matrix elements of the volume operator in canonical quantum gravity, J. Math. Phys.
- Thiemann T The length operator in canonical quantum gravity, J. Math. Phys.
Cited by
Sorted by citations
Background independent quantum gravity: a status report
Ashtekar, A., & Lewandowski, J. (2004) · Classical and Quantum Gravity · doi:10.1088/0264-9381/21/15/r01 · Cited by 1,951 · see citing works
Quantum nature of the big bang: Improved dynamics
Ashtekar, A., Pawlowski, T., & Singh, P. (2006) · Physical Review D · doi:10.1103/physrevd.74.084003 · Cited by 1,147 · see citing works
Nonstandard optics from quantum space-time
Gambini, R., & Pullin, J. (1999) · Physical Review D · doi:10.1103/physrevd.59.124021 · Cited by 960 · see citing works
The Spin-Foam Approach to Quantum Gravity
Perez, A. (2013) · Living Reviews in Relativity · doi:10.12942/lrr-2013-3 · Cited by 677 · see citing works
Quantum nature of the big bang: An analytical and numerical investigation
Ashtekar, A., Pawlowski, T., & Singh, P. (2006) · Physical Review D · doi:10.1103/physrevd.73.124038 · Cited by 609 · see citing works
Kinematical Hilbert spaces for fermionic and Higgs quantum field theories
Thiemann, T. (1998) · Classical and Quantum Gravity · doi:10.1088/0264-9381/15/6/006 · Cited by 184 · see citing works
Self-citationQuantum spin dynamics: VIII. The master constraint
Thiemann, T. (2006) · Classical and Quantum Gravity · doi:10.1088/0264-9381/23/7/003 · Cited by 99 · see citing works
Self-citationAre the spectra of geometrical operators in loop quantum gravity really discrete?
Dittrich, B., & Thiemann, T. (2009) · Journal of Mathematical Physics · doi:10.1063/1.3054277 · Cited by 96 · see citing works
Self-citationQuantum geometry with intrinsic local causality
Markopoulou, F., & Smolin, L. (1998) · Physical Review D · doi:10.1103/physrevd.58.084032 · Cited by 95 · see citing works
Diffeomorphism covariant representations of the holonomy-flux -algebra
Oko w, A., & Lewandowski, J. (2003) · Classical and Quantum Gravity · doi:10.1088/0264-9381/20/16/302 · Cited by 58 · see citing works
Spin foam quantization and anomalies
Bojowald, M., & Perez, A. (2010) · General Relativity and Gravitation · doi:10.1007/s10714-009-0892-9 · Cited by 35 · see citing works
Eleven-dimensional supergravity as a constrained topological field theory
Ling, Y., & Smolin, L. (2001) · Nuclear Physics B · doi:10.1016/s0550-3213(01)00063-3 · Cited by 29 · see citing works
Finite spin-foam-based theory of three- and four-dimensional quantum gravity
Gambini, R., & Pullin, J. (2002) · Physical Review D · doi:10.1103/physrevd.66.024020 · Cited by 10 · see citing works
- Authors
- Thiemann, T.
- Affiliations
- Harvard University (US)
- Corresponding author
- Thiemann, T
- ORCID
- Thiemann, T
- Venue
- Classical and Quantum Gravity
- Publisher
- IOP Publishing
- Published
- 1998-05-01
- Volume
- 15
- Issue
- 5
- Pages
- 1281-1314
- ISSN
- 0264-9381 (ISSN-L)
- 1361-6382
- OpenAlex
- W2018885617
- Semantic Scholar
- 41b70398a6c6292d63083e9f9103b1533dc0771d
- Cited by
- 416
- References
- 26
- Citations by year
- 2026: 3 · 2025: 4 · 2024: 11 · 2023: 12 · 2022: 4 · 2021: 17 · 2020: 8 · 2019: 4 · 2018: 8 · 2017: 10 · 2016: 18 · 2015: 15 · 2014: 11 · 2013: 21 · 2012: 14
- FWCI
- 12.25
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- Classical and Quantum Gravity (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- Max Planck Institute for Plasma Physics (submittedVersion)
- Max Planck Digital Library (submittedVersion)
- MPG.PuRe (Max Planck Society) (submittedVersion)
- Funders
- U.S. Department of Energy (DE‐FG02‐)
- Harvard University
- Topics
- Physical Sciences › Physics and Astronomy › Statistical and Nonlinear Physics › Noncommutative and Quantum Gravity Theories
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Relativity and Gravitational Theory
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Black Holes and Theoretical Physics
- Keywords
- quantum gravity, Hamiltonian constraint, quantum field theory in curved spacetime, Standard Model, canonical quantum gravity, Lorentzian quantum gravity, non-perturbative quantum field theory, second quantization, renormalization, string theory
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