Cited by 136Noncommutative and Quantum Gravity TheoriesRelativity and Gravitational TheoryBlack Holes and Theoretical Physics

Reconcile Planck-scale discreteness and the Lorentz-Fitzgerald contraction

Open access
Rovelli, Carlo, Speziale, Simone·2003·Physical Review D

Abstract

A Planck-scale minimal observable length appears in many approaches to quantum gravity. It is sometimes argued that this minimal length might conflict with Lorentz invariance, because a boosted observer can see the minimal length further Lorentz contracted. We show that this is not the case within loop quantum gravity. In loop quantum gravity the minimal length (more precisely, minimal area) does not appear as a fixed property of geometry, but rather as the minimal (nonzero) eigenvalue of a quantum observable. The boosted observer can see the same observable spectrum, with the same minimal area. What changes continuously in the boost transformation is not the value of the minimal length: it is the probability distribution of seeing one or the other of the discrete eigenvalues of the area. We discuss several difficulties associated with boosts and area measurement in quantum gravity. We compute the transformation of the area operator under a local boost, propose an explicit expression for the generator of local boosts, and give the conditions under which its action is unitary.

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Written from the paper’s full text.

TL;DR

In loop quantum gravity, the Planck-scale minimal area is not a fixed property of geometry but the minimal nonzero eigenvalue of a quantum area observable. The authors argue that a boosted observer sees the same minimal area eigenvalue, while the probability distribution over discrete area eigenvalues changes continuously under the boost.

Key findings

  • The minimal nonzero area \(A_0\) observed by one observer remains the same minimal nonzero area for a boosted observer; what changes under the boost is the probability distribution of seeing one or another discrete area eigenvalue.
  • The area operators \(A\) and \(A'\) associated with two relatively boosted observers have nonvanishing Poisson brackets, so the corresponding quantum operators cannot commute; therefore if the area is sharp for one observer, it generally cannot be sharp for the other.
  • The authors compute the transformation of the area operator under a local boost, propose an explicit expression for the generator of local boosts depending on the Hamiltonian constraint, and state that the transformation is unitary if this generator is Hermitian, in which case the spectrum is preserved.
  • They draw an analogy with angular momentum: a rotated observer still sees the same minimal nonzero component \(L_0\), while the distribution of eigenvalues is determined by the rotation group representation theory.

Methods

  • The paper studies general relativity coupled to two particles and a two-dimensional surface (“table”), with two observers \(O\) and \(O'\) crossing at a point \(P\); the area is defined as the intersection of the table worldsheet with each observer’s simultaneity surface, assuming a small surface and negligible curvature/acceleration at \(P\).
  • Coordinates are gauge-fixed to the matter, and the areas \(A\) and \(A'\) are expressed as functions of the metric and canonical Ashtekar variables; the analysis expands in the boost parameter \(\beta\), computing \(A'\) to first and second order and evaluating the Poisson bracket \(\{A,A'\}\).
  • A candidate boost generator is constructed from Lorentz generators and the energy-momentum tensor, with the Minkowski metric replaced by \(g_{\mu\nu}(x)\); its infinitesimal action on \(A\) is checked against the geometric transformation, and unitarity is discussed via Hermiticity of the corresponding quantum operator.

Limitations

  • The paper states that the theory as a whole is not Lorentz invariant; Lorentz invariance can only be recovered locally and/or in sufficiently flat regimes, and the viability of expanding around a macroscopically flat quantum state is regarded as an hypothesis because nonperturbative quantum gravity gives less control over the gravitational field state.
  • The paper states that the detailed calculation of the boosted simultaneity surface position is not reported, and that the actual definition of the node operator \(g_{1a}x^a_n D_n\) in the quantum theory is left to future investigations.
  • Evident from the text: the results rely on perturbative expansion in the boost parameter and on assumptions of small surface size, local flatness, and in part a spatially constant metric simplification, though the authors say the latter is not essential.

Model-written summary. Check it against the paper before relying on it.

Integrity signals

Registry

Crossref · 10.1103/physrevd.67.064019

Cites

Statistics

Nothing to recompute.

Claims the paper makes

0 of 14 cited sources checked · 0 supported · 0 flagged

  • Findingreasoning
    § B. Area in general relativity · p. 4

    The area A(S) of the 2d surface S given by the intersection of two 3d hypersurfaces Σ and T can be written in terms of the one-forms normal to the two hypersurfaces.

    “Here we show that A ( S ) can be written in terms of the one-forms n Σ µ and n T µ normal to the two hypersurfaces.”
    • Also stated in: § B. Area in general relativity · p. 5 · plain
      “This expression gives us the area directly as a function of surface S , the metric and the normals to the table worldsheet and the observer's simultaneity surface.”
    Quote in the paperSubstantial claim
  • Findingreasoning
    § IV. NON COMMUTATIVITY · p. 8

    The Poisson brackets between A and A' do not vanish.

    “Since the Poisson brackets between A and A ′ do not vanish, the commutator of the corresponding quantum operator cannot vanish either.”
    • Also stated in: § VI. DISCUSSION AND CONCLUSIONS · p. 11 · boosted
      “We have shown that these two observables have nonvanishing Poisson brackets, which implies that the corresponding quantum operators cannot commute.”
    Quote in the paperSubstantial claim
  • Findingreasoning
    § A. The basic idea · p. 1

    The area operators A and A' associated to measurements by relatively boosted observers do not commute.

    “Now, our main point is the technical observation that A and A ′ do not commute:”
    • Also stated in: § A. The basic idea · p. 2 · boosted
      “In this paper, we prove equation (1).”
    Quote in the paperSubstantial claim
    • Rests on an assumption: A field operator does not commute with itself at different times.
  • Findingreasoning
    § IV. NON COMMUTATIVITY · p. 7

    Even if the dynamics of the gravitational field in these coordinates is assumed unaffected by matter, the right-hand side of the Poisson bracket {A,A'} does not vanish.

    “However, one can easily see that even if we assume that in these coordinates the dynamics of the gravitational field is unaffected by the matter, the r.h.s. does not vanish.”
    Quote in the paperSubstantial claim
  • Findingnone given
    § B. Area in general relativity · p. 5

    The normal one-form of the table worldsheet T does not depend on the metric.

    “It does not depend on the metric.”
    Quote in the paperNot a substantial claim
  • May combine two claims. 12
  • Classified as probably not a substantial claim. 14
  • May combine two claims.

    Findingreasoning
    § A. Coordinate choice · p. 6

    gμν(x) does not depend on α at t=0, while its time derivative does.

    “( g µν ( x ) does not depend on α at t = 0, while its time derivative does.)”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S3 (load-bearing).

    Findingreasoning
    § A. Coordinate choice · p. 6

    The relative velocity of the particle X with respect to the center of the table is α.

    “Therefore the relative velocity of the particle X with respect to the center of the table is α .”
    Quote in the paperNot a substantial claim
  • Classified as probably not a substantial claim.

    Findingnone given
    § A. The system · p. 4

    A and A' are diffeomorphism invariant functions of g, X, X', T.

    “The quantities A and A ′ are diffeomorphism invariant functions of g , X , X ′ an T .”
    Quote in the paperSubstantial claim
  • Classified as probably not a substantial claim.

    Interpretationreasoning
    § A. Coordinate choice · p. 6

    In the present context, the dynamics is entirely captured by the value of the gravitational field.

    “In the present context, we have chosen to attach coordinates to the matter (particles and table). Therefore the dynamics is entirely captured by the value of the gravitational field.”
    Quote in the paperSubstantial claim
  • Probably not a substantial claim: may not pass S3 (load-bearing).

    Interpretationnone given
    § A. Coordinate choice · p. 5

    In the chosen gauge, the only remaining degrees of freedom are the ones in the metric tensor gμν(x).

    “With these coordinates, namely in this gauge, the only remaining degrees of freedom are the ones in the metric tensor g µν ( x ).”
    Quote in the paperNot a substantial claim
  • May combine two claims.

    Interpretationreasoning
    § I. INTRODUCTION · p. 1

    In loop quantum gravity, a boosted observer O' does not observe a Lorentz contracted A0; the minimal nonzero area O' can observe is still A0.

    “Here we show that in loop quantum gravity a boosted observer O ′ does not observe a Lorentz contracted A 0 . The minimal (nonzero) area that the boosted observer O ′ can observe is still A 0 .”
    • Also stated in: § Reconcile Planck-scale discreteness and the Lorentz-Fitzgerald contraction · p. 1 · plain
      “The boosted observer can see the same observable spectrum, with the same minimal area.”
    Quote in the paperSubstantial claim
  • Probably not a substantial claim: may not pass S3 (load-bearing).

    Interpretationreasoning
    § A. The system · p. 4

    A and A' are physical quantities that are in principle observable using appropriate measuring devices.

    “They are physical quantities that are in principle observable, by using appropriate measuring devices (formed by light pulses, detectors, clocks, and else).”
    Quote in the paperNot a substantial claim
  • Probably not a substantial claim: may not pass S4 (based).

    Interpretationnone given
    § A. The system · p. 3

    The system of the gravitational field, two particles, and a two-dimensional surface provides a minimal setting in which to compare the area observed by two observers boosted with respect to each other.

    “These are the dynamical quantities of the system we consider. They provide a minimal setting in which we can compare the area observed by two observers boosted with respect each other.”
    Quote in the paperNot a substantial claim
  • May combine two claims.

    Interpretationreasoning
    § A. The basic idea · p. 2

    The mean value of the area can be Lorentz contracted, while the minimal nonzero value of the area can remain A0.

    “The mean value of the area can be Lorentz contracted, while the minimal nonzero value of the area can remain A 0 .”
    Quote in the paperSubstantial claim
  • Probably not a substantial claim: may not pass S3 (load-bearing), S4 (based).

    Premisenone given
    § A. The system · p. 4

    Transversal motion does not give rise to Lorentz contraction.

    “(We are not interested in transversal motion because it does not give rise to Lorentz contraction.)”
    Quote in the paperNot a substantial claim
  • Classified as probably not a substantial claim.

    Premisereasoning
    § A. Coordinate choice · p. 5

    The physical, measurable position of an object relative to a reference object is determined by a combination of the coordinate position of matter and the value of the metric tensor.

    “The physical, measurable, position of an object (relative to a reference object) is determined by a combinations of the two.”
    Quote in the paperSubstantial claim
  • Classified as probably not a substantial claim. May combine two claims.

    Premisenone given
    § A. Coordinate choice · p. 5

    The coordinate position of matter and the value of the metric tensor are both gauge dependent quantities due to diffeomorphism invariance.

    “Indeed, it is well known that the coordinate position of matter and the value of the metric tensor are both gauge dependent quantities, due to diffeomorphism invariance.”
    Quote in the paperSubstantial claim
  • May combine two claims.

    Interpretationreasoning
    § A. The velocity of the surface · p. 8

    In general relativity, A becomes a quantum operator because it is a function of the metric, and the velocity V in (51) depends on the metric as well, so V is also an operator in quantum gravity.

    “In general relativity, A becomes a quantum operator because it is a function of the metric, namely a function of the quantum field. But the velocity V that appears in (51) depends on the metric as well. Indeed the V that appears in (51) is not a coordinate velocity, it is a physical velocity, and it depends on g µν as well. Thus V as well is an operator in quantum gravity.”
    Quote in the paperSubstantial claim
  • Probably not a substantial claim: may not pass S3 (load-bearing).

    Premisecitation
    § V. BOOSTS GENERATORS · p. 9

    In a Lorentz invariant theory, the quantities Mμν defined by (53) are constant.

    “In a Lorentz invariant theory, (53) are constant.”
    Quote in the paperNot a substantial claim0 of 1 sources checked
    • cites [11] source

      Not checked in the free run.

  • Probably not a substantial claim: may not pass S3 (load-bearing).

    Premisecitation
    § A. Unitarity · p. 10

    The action of the Hamiltonian constraint smeared with a Lapse N is a sum of terms acting on the nodes of the form given in the cited work.

    “We recall that the action of the Hamiltonian constraint smeared with a Lapse N is a sum of terms acting on the nodes of the form [15,16]”
    Quote in the paperNot a substantial claim0 of 2 sources checked
    • cites [15]

      Not checked in the free run.

    • cites [16]

      Not checked in the free run.

  • Probably not a substantial claim: may not pass S3 (load-bearing).

    Premisecitation
    § A. Unitarity · p. 10

    A basis of area eigenstates is given by spin network states.

    “Recall that a basis of area eigenstates is given by spin network states [13,14].”
    Quote in the paperNot a substantial claim0 of 2 sources checked
    • cites [13]

      Not checked in the free run.

    • cites [14]

      Not checked in the free run.

  • Probably not a substantial claim: may not pass S4 (based).

    Premisenone given
    § VI. DISCUSSION AND CONCLUSIONS · p. 11

    In loop quantum gravity the metric is an operator.

    “In loop quantum gravity the metric is an operator.”
    Quote in the paperNot a substantial claim
  • May combine two claims.

    Interpretationreasoning
    § VI. DISCUSSION AND CONCLUSIONS · p. 11

    The Lorentz transformations considered act on the matter at fixed field, or equivalently on the field leaving the matter fixed, and this is why they are not part of the gauge.

    “The Lorentz transformations we have considered act on the matter at fixed field, or, equivalently, on the field leaving the matter fixed. This is why they are not part of the gauge.”
    Quote in the paperSubstantial claim
  • May combine two claims.

    Premisenone given
    § V. BOOSTS GENERATORS · p. 9

    In gravity, the quantities (53) are formal objects; they are not tensorial, not defined for all values of the fields, not defined on the entire spacelike surface.

    “In gravity, we can still write the quantities (53). These are formal objects. They are not tensorial, not defined for all values of the fields, not defined on the entire spacelike surface.”
    Quote in the paperSubstantial claim
  • May combine two claims.

    Interpretationreasoning
    § VI. DISCUSSION AND CONCLUSIONS · p. 11

    The theory is not invariant under a diffeomorphism that acts on the matter leaving the gravitational field untouched, nor under one that acts on the gravitational field leaving the matter untouched.

    “However, it is not invariant under a diffeomorphism that acts on the matter leaving the gravitational field untouched. Nor under a diffeomorphism that acts on the gravitational field leaving the matter untouched.”
    Quote in the paperSubstantial claim
  • Classified as probably not a substantial claim. May combine two claims.

    Premisenone given
    § V. BOOSTS GENERATORS · p. 10

    The momentum generates spatial translations, and in general relativity spatial translations are generated by the momentum constraint H_a(x).

    “The momentum, generates spatial translations. Spatial translations are generated by the momentum constraint H a ( x ) in general relativity.”
    Quote in the paperSubstantial claim
  • May combine two claims.

    Premisenone given
    § VI. DISCUSSION AND CONCLUSIONS · p. 11

    At the Planck scale, the area is quantized and there is a finite nonzero minimal value.

    “At the Planck scale, this area is quantized and there is a finite nonzero minimal value.”
    Quote in the paperSubstantial claim
  • May combine two claims.

    Interpretationreasoning
    § VI. DISCUSSION AND CONCLUSIONS · p. 11

    In the presence of matter, or in the gauge-fixed coordinates chosen, an active Lorentz transformation rotating the gravitational field is a change of physical state, whereas it would be a gauge transformation in the absence of matter and in arbitrary coordinates.

    “Concretely, we have gauge fixed the coordinate position of the matter, and considered an active Lorentz transformation rotating (in spacetime) the gravitational field. While this would be a gauge transformation in the absence of matter and in arbitrary coordinates, it is, instead, a change of physical state in the presence of matter, or, equivalently, in the gauge fixed coordinates we have chosen.”
    Quote in the paperSubstantial claim
  • May combine two claims.

    Interpretationreasoning
    § A. Unitarity · p. 10

    Assuming the operator M(λ) is hermitian, the finite transformation it generates is unitary, and the spectrum of areas A and A' is the same.

    “This operator is unitary if M ( λ ) is hermitian. This is the condition under which the Lorentz transformation is unitary in the quantum theory. Assuming it is satisfied, the spectrum of the areas A and A ′ is the same.”
    Quote in the paperSubstantial claim
    • The authors state this as an assumption: The quantum operator M(λ) corresponding to the classical observable (61) is well defined in the theory.
    • The authors state this as an assumption: The operator M(λ) is hermitian.
24 of 24
  • The paper relies on this without support.

    A field operator does not commute with itself at different times.

    “a field operator does not commute with itself at different times.”
  • The paper relies on this without support.

    Generically, quantum theory does not predict an observable value; it predicts a probability distribution of possible values.

    “Generically, quantum theory does not predict an observable value: it predicts a probability distributions of possible values.”
  • The paper relies on this without support.

    The theory as a whole is not Lorentz invariant, and a form of Lorentz invariance can only be recovered locally and/or in certain sufficiently flat regimes.

    “The theory as a whole is not Lorentz invariant, and a form of Lorentz invariance can only be recovered locally and/or in certain ('sufficiently flat') regimes.”
  • The paper relies on this without support.

    The area A is a far more complicated function of the basic variables of the theory than L_z.

    “The area A is a far more complicated function of the basic variables of the theory than L z .”
  • The paper relies on this without support.

    Lorentz transformations do not happen at fixed time, so the generators of local Lorentz transformations must know about the dynamics of the theory.

    “Lorentz transformations, unlike rotational symmetry, do not happen at fixed time. Therefore the generators of the (local) Lorentz transformations have to know about the dynamics of the theory, which is highly nontrivial in quantum gravity.”
  • The authors state this as an assumption.

    Other physical objects exist in the universe and can be used to perform measurements.

    “Besides these dynamical quantities, we assume that all sort of other physical objects exist in the universe. These can be used to perform measurements (for instance, light pulses traveling along geodesics, apparatus that detect the arrival of these light pulses, clocks that measure proper time along world lines, recording devices and so on).”
  • The authors state this as an assumption.

    The freedom of choosing the boundary between the observed quantum system and the classical apparatus allows us to treat other physical objects as part of the measuring apparatus.

    “To be precise, we assume that the well known freedom of choosing the boundary between the observed quantum system and the classical apparatus -emphasized by Von Neumann- allows us to do so in this context.”
  • The authors state this as an assumption.

    The dynamics of the system is governed by the Einstein equations and the dynamical equations of the table and the particles.

    “We assume the dynamics of this system to be governed by the the Einstein equations and the dynamical equations of the table and the particles.”
  • The authors state this as an assumption.

    The matter energy-momentum tensor is negligible in the Einstein equations.

    “For simplicity, we assume that the matter energy-momentum tensor is negligible in the Einstein equations, but this is not essential in what follows.”
  • The authors state this as an assumption.

    In the quantum theory, the expansion in small boost parameter and small surface remains valid in regimes where the expectation value of the macroscopic curvature is small.

    “We then assume that in the quantum theory the expansion remains valid in the regimes where the expectation value of the macroscopic curvature is small.”
  • The authors state this as an assumption.

    The curvature at and around P and the acceleration of the particles at P are negligible at the scale of the surface.

    “Second, (in the classical analysis) we assume that the curvature at and around P and the acceleration of the particles at P are negligible at the scale of the surface. That is, we take the surface small enough that we can expand around P and keep the lowest terms only.”
  • The authors state this as an assumption.

    The relative three-velocity of the two observers is tangent to the table.

    “For simplicity, we also assume that the relative three-velocity of the two observers is tangent to the table.”
  • The authors state this as an assumption.

    The metric is spatially constant at t=0.

    “Let us now make the additional assumption that the metric is spatially constant at t = 0.”
  • The authors state this as an assumption.

    The quantum operator M(λ) corresponding to the classical observable (61) is well defined in the theory.

    “We assume that this operator is well defined in the theory.”
  • The authors state this as an assumption.

    The operator M(λ) is hermitian.

    “This operator is unitary if M ( λ ) is hermitian. This is the condition under which the Lorentz transformation is unitary in the quantum theory. Assuming it is satisfied, the spectrum of the areas A and A ′ is the same.”
  • The paper relies on this without support.

    Under a Lorentz transformation, the minimal area does not change, so two observers boosted with respect to each other see the same spectrum.

    “Under a Lorentz transformation, we expect this minimal value not to change. That is, we expect that two observers boosted with respect to each other, see the same spectrum.”
16 of 16

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?

  • A discrete geometry is compatible with Lorentz invariance.

    “on the one hand, discreteness of geometry can coexist with Lorentz invariance [331]”

    From The Spin-Foam Approach to Quantum Gravity (2013) · cites this paper as [331]

The citation lists haven’t been fetched yet

References 18 · Cited by 136

Research works printed but not linked: 1

  1. C. Rovelli, 1995, Nucl. Phys., B456, 734

Authors
Rovelli, C., & Speziale, S.
Venue
Physical Review D
Published
2003-03-27
Volume
67
Issue
6
Pages
064019
ISSN
  • 0556-2821 (ISSN-L)
  • 1089-4918
OpenAlex
W2016972835
Cited by
136
References
18
Citations by year
2026: 2 · 2025: 4 · 2024: 6 · 2023: 3 · 2022: 2 · 2021: 6 · 2020: 5 · 2019: 1 · 2018: 6 · 2017: 6 · 2016: 6 · 2015: 2 · 2014: 4 · 2013: 14 · 2012: 9
FWCI
6.39
Type
journal article
Language
en
Open access
Locations
  • Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • HAL (submittedVersion)
  • CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
  • arXiv (Cornell 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
Planck scale discreteness, minimal length, Lorentz invariance, length contraction, loop quantum gravity, minimal area, area operator, unitarity, quantum gravity

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