REVIEW 4 major objections 5 minor 121 references
Foundational Structure of Local Amplitudes in Quantum Gravity
T0 review · 4 major / 5 minor · reviewed 2026-08-05 · deepseek-v4-flash
Pith's one-line read This paper proves that, given seven stated axioms, local quantum-gravity amplitudes built purely from boundary symmetry data, a projector, and two vacuum states satisfy Ward identities and charge conservation in causal diamonds.
desk verdict A clean algebraic skeleton for local amplitudes in causal diamonds, with the existence of the vacuum states as the load-bearing but unproven input; worth refereeing, but only as a framework proposal. read the letter →
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
The reading
What carries the argument
The load-bearing object is the generalized projector $P$ onto physical states, defined by the flux-balance constraints $C_\xi = Q_\xi[C_+] - Q_\xi[C_-] - H_\xi[N] = 0$; it commutes with the corner charges and intertwines the edge symmetries. Two states carry the rest of the argument: the edge vacuum $T^A$, a singlet (a state every corner charge annihilates) representing a corner shrinking to a point, and the bulk vacuum $|\Omega^A_{A'}\rangle$, a physical state intertwining the corner symmetry algebras at the two ends of the slab. The amplitude (47) is the contraction of these objects in a causal-diamond pattern, and the Ward identities follow from sliding constraint insertions through the p
What would settle it
In a concrete model — say the auxiliary conformal field theory of null-cone quantization, or a spinfoam model on a fixed two-complex — write the unitary representation of the corner symmetry algebra on the boundary Hilbert space and check whether a non-zero edge vacuum annihilated by all corner charges exists, and whether a physical bulk vacuum satisfying (45)–(46) exists. For infinite-dimensional algebras such as $\mathrm{Diff}(S^2)$ or Virasoro algebras at non-zero central charge such invariant states are generically absent; finding none in any model would show the axioms are unsatisfiable,
Extended reading notes
Core claim
Under axioms (i)–(vii), the paper claims that the amplitude (47) — in- and out-states contracted with the projector $P$ and the vacua $T^A$, $|\Omega^A_{A'}\rangle$ — satisfies the Ward identities (51)–(52) and the corner charge-conservation law (55): flux through a null face acts on the amplitude exactly like the corner charge at that face's tip, and the two tips' charges match up to a parallel transport $h$. The proof is index bookkeeping: $P$ solves the flux-balance constraints $C_\xi = Q_\xi[C_+] - Q_\xi[C_-] - H_\xi[N]=0$ and intertwines the edge symmetries; $T^A$ is a corner-algebra singlet; $|\Omega^A_{A'}\rangle$ is a physical intertwiner between the corner algebras, so constraint in
Load-bearing premise
The construction stands or falls on the assumed existence of two states, stated in equations (44)–(46) and axioms (vi)–(vii): an edge vacuum $T^A$ annihilated by every corner charge, and a bulk vacuum $|\Omega^A_{A'}\rangle$ that solves the flux-balance constraints and intertwines the two corner symmetry algebras; if a corner symmetry algebra admits no such invariant states, the amplitude (47) is undefined or trivial.
Editorial extensions
If this is right
- Local quantum-gravity probabilities for processes inside a causal diamond become computable from boundary symmetry data alone — corner charges, fluxes, and the two vacua — with no global wave function and no asymptotic S-matrix.
- Corner charges $Q_\xi[C_\pm]$ are physical observables (they commute with the projector), so the charge-conservation identity (55) identifies boundary charges as the natural observable content of the local theory, in the same role soft charges play at null infinity.
- The null-boundary constraint algebra is a genuine Lie algebra, so the projector $P$ is a well-defined averaging over symmetries, avoiding the structure-function problem that obstructs quantizing the spacelike constraint algebra.
- Spinfoam models, group field theory, and null-cone quantization all realize the projector in concrete ways (a sum over surfaces or a CFT $n$-point function), giving candidate models in which axioms (i)–(vii) can be verified or refuted.
- As the diamond grows toward null infinity, the local charge-conservation law reproduces the structure of the soft-graviton Ward identities, linking the finite-region amplitude program to the perturbative S-matrix framework.
Reading between the lines
- The axioms are satisfiable only if the corner symmetry algebra admits invariant states; for infinite-dimensional algebras such as diffeomorphisms of a two-sphere or Virasoro algebras at non-zero central charge, unitary representations generically contain no non-zero invariant vectors. A concrete model would therefore either select special algebras and representations or expose the axioms as empty
- Read as a finite-region holographic recipe, the construction encodes everything between the two corners in boundary data, since the bulk enters only through the projector and vacuum intertwiners. A direct test would be 2+1 gravity, where the projector is known exactly and the amplitudes (47) can be compared with the standard amplitudes for a null-bounded region.
- If corner charges are observables, the physical Hilbert space of a diamond splits into charge superselection sectors, and (55) forces the in- and out-data to live in matching sectors; this superselection structure is not spelled out in the paper but follows from the identities it proves.
- The paper itself concedes (Section 5) that it is 'deliberately vague' about how the axioms are realized in practice; the proposal is best read as a consistency condition that candidate quantum-gravity constructions must satisfy rather than as a construction, and the axioms' main risk is that no real model satisfies them.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper proposes an axiomatic, top-down framework for constructing local transition amplitudes in quantum gravity on causal diamonds bounded by null surfaces. The authors review timeless quantum mechanics and covariant phase space, then define a kinematical Hilbert space factorized into corner edge modes and bulk radiative modes. The physical Hilbert space is obtained by a generalized projector implementing flux-balance constraints. The central result is the amplitude formula (47), built from projectors P and assumed vacuum states T^A and |Ω^A_{A'}⟩, and the claim that this amplitude satisfies Ward identities (51), (52) and local charge conservation (55). The paper concludes by discussing possible realizations through CFT data and spinfoam/GFT constructions.
Significance. If the axioms can be realized, the paper provides a clean structural template for local gravitational amplitudes: the amplitude is a tensor contraction of a generalized projector with vacuum intertwiners, and the Ward identities follow transparently from the stated axioms. The derivation is algebraic and easy to follow, and the paper avoids fitted parameters. Its main value is as a synthesis and blueprint, connecting null-surface edge modes, flux-balance laws, and timeless amplitudes. The main weakness is that the existence of the edge vacuum T^A and bulk vacuum |Ω^A_{A'}⟩, Eqs. (44)–(46), is assumed rather than established; for the infinite-dimensional corner algebras the paper names (Diff(S^2), Virasoro-type, jet-bundle extensions), such invariant or intertwining states need not exist in unitary representations. Thus the central result is conditional on a non-trivial existence problem.
major comments (4)
- [§4.2, Eqs. (44)–(46); §4.3 Axioms (vi)–(vii)] The load-bearing assumption is the existence of T^A and |Ω^A_{A'}⟩ satisfying (44)–(46). The paper explicitly defers realization to [11] and future work, but this is not a minor gap. For the corner symmetry algebras mentioned (Diff(S^2), Virasoro-type, jet-bundle extensions), unitary representations generically contain no nonzero invariant vector, and group-averaging typically yields distributional states outside the kinematical Hilbert space. Similarly, (46) requires a normalizable solution of the quantum constraints with the flux-balance operator equal to the charge difference; if zero lies in the continuous spectrum, no such Ω exists in K↑. Since (47)–(55) use T and Ω as ordinary Hilbert-space intertwiners, failure of existence makes the amplitude undefined or identically zero and the Ward identities vacuous. The authors should either provide a concrete model satisfying (44)–(46) or s
- [§4.2, Eqs. (35)–(40); §2, Eqs. (4)–(5)] The functional-analytic status of the generalized projector is not addressed. P is said to map into possibly non-normalizable elements of the algebraic dual, yet the amplitude (47) and Ward identities use ⟨γ|P|Ω⟩ as ordinary matrix elements and move charges through P using (37)–(43). This requires a specification of dense domains, adjoints, and the convergence of the infinite sums/integrals over A,A′ in (25) and (47). The DeWitt notation in footnote 9 deliberately suppresses these issues, but they become load-bearing when the corner algebra is infinite-dimensional and the charges Qξ are unbounded. The authors should state the domain assumptions under which (47)–(55) are well-defined.
- [End of §4.3, Eq. (55)] Equation (55), local charge conservation, is a central advertised result but is asserted rather than derived: the text says only 'In the same way, it is easy to show'. Given that the derivation of (54) is already intricate and relies on the parallel-transport map h and the vacuum annihilation (44), the proof of (55) should be written out. In particular, it must be shown how Qξ[C+in] on the in-state is transported through the projector and the bulk vacuum to Q_{hξ}[C+out] on the out-state, using (45), (46), and (49)–(50). Without this, the charge-conservation claim is not substantiated.
- [§4.3 Axioms (iii),(v), Eqs. (37)–(38), (51)–(52)] The Ward identities (51)–(52) are to a large extent unpackings of the axioms rather than independent dynamical predictions. The projector P is defined by (37)–(38) to annihilate the constraint Cξ = Q[C+] − Q[C−] − H, and Ω is assumed by (46) to satisfy the same flux-balance condition. Consequently, moving Hξ through P and using the vacuum conditions produces (51) and (52) almost immediately. This is not an error, but the paper should state explicitly that the identities are consequences of the construction, and clarify in the discussion of Section 5 what additional predictive content, if any, the framework has beyond these built-in constraints. The comparison with soft-graviton theorems in the conclusion should be qualified accordingly.
minor comments (5)
- [§3] In the sentence defining the null slab, '∂N = C+ ∪ C−1−' appears to contain a typo; it should presumably read C+ ∪ C−.
- [§4.1, Eq. (24) and Axiom (i)] The notation for the dual relation between KC+ and KC− is inconsistent: earlier KC− = K*_{C+}, while Axiom (i) says KC+ = K†_{C−}. These are equivalent only under the inner-product identification, which should be stated.
- [§4.2, Eqs. (35)–(36)] The same symbol |γA A′⟩ is used for the state and its projected image; this makes the definition of P hard to read. Use a different symbol, e.g. P|γ⟩ = |γ phys⟩.
- [References] References [26] and [77] are the same paper (Donnelly–Freidel), as are [66] and [102] (Perez) and [92] and [108] (Giacomini–Castro-Ruiz–Brukner). Please consolidate.
- [Figure 4 caption] The caption describes N′in as attached to 'the outgoing null surface Nin' and N′out to 'the infalling null surface Nout'. This is confusing; clarify which auxiliary slab is glued to which boundary and whether 'in'/'out' refer to the slab orientation or the causal future.
Circularity Check
Ward identities and charge conservation are restatements of the projector and vacuum axioms; the amplitude contraction pattern itself is a genuine construction.
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self definitional
[Section 4.3, Axiom (v) and Eq. (51)]
"Given these assumptions, we obtain A(Hξ[Nin]γ(in) → γ(out)) = A(Qξ[C+in]γ(in) → γ(out)). (51)"
Axiom (v) defines P as a projector onto the solution space of the constraints, i.e. P Cξ = CξP = 0, with Cξ = Qξ[C+] − Qξ[C−] − Hξ[N] (Axiom (iii)). Eq. (48) obtains the left side by moving Hξ through P using the projector condition (37)–(38). The right side is then just the charge part of the same constraint, with the Q− term killed by the assumed edge-vacuum condition (44). The Ward identity is therefore the constraint equation written in amplitude form; it is an input of the projector definition, not an independent prediction.
-
self definitional
[Section 4.3, Eq. (55) with Axioms (vi)–(vii)]
"In the same way, it is easy to show that the amplitudes realise local charge conservation at the corner, where the future and past states intersect, i.e. A(Qξ[C+in]γ(in) → γ(out)) = A(γ(in) → Qh[C+in→C+out]ξ[C+out]γ(out)). (55)"
This identity follows by using the assumed intertwining property (45) of the bulk vacuum and the assumed annihilation (44) of the edge vacuum, together with the projector-invariance (42)–(43). These are precisely the properties that make T and Ω intertwiners; (55) is a direct transcription of those assumed intertwiner relations into a matrix element. It does not test the construction against new data; it restates the axioms in amplitude language.
full rationale
The paper is transparently an axiomatic, top-down framework: the amplitude (47) is a new contraction pattern, and the gluing construction of Figure 4 has independent content. However, the two advertised results—Ward identities (51)/(52) and local charge conservation (55)—are not independent predictions. Axiom (v) already states that the projector annihilates the constraints, and Axioms (vi)–(vii) already state that the edge and bulk vacua are singlets/intertwiners. The derivations in (48)–(54) unpack these axioms by moving Hξ through P and using the vacuum properties; no new physical input enters. This is a mild form of circularity-by-construction: the results are equivalent to the defining equations of P, T, and Ω. There are no fitted parameters, no external benchmarks, and no load-bearing self-citation loop. The unproven existence of the vacua (44)–(46), deferred to ref. [11] and future work, is a genuine gap in realizability, but because the paper labels these as axioms rather than deriving them, it is a completeness risk rather than a circular step. Overall score 6 reflects that the central consistency claims reduce to the axioms, while the amplitude construction itself remains a genuine proposal.
Assumptions & free parameters
assumptions (7)
- domain assumption Kinematical Hilbert space factorization K_N = K_C+ tensor K_N tensor K_C- (equation 24).
- domain assumption Existence of a generalized projector P onto physical states satisfying equations (35) through (43).
- ad hoc to paper Edge vacuum T^A exists and is annihilated by all corner charges Q_xi[C_+-] (equation 44).
- ad hoc to paper Bulk vacuum |Omega^A_{A'}> exists, solves all constraints, and intertwines corner charges (equations 45 and 46).
- domain assumption Constraint algebra C_xi = Q_xi[C_+] minus Q_xi[C_-] minus H_xi[N] = 0, with charges commuting with the projector (equations 37, 38, 42, 43).
- domain assumption Parity swap operator Pi with Pi^2 = 1, commuting with constraints, and decomposition K_N = K^up plus K^down (equations 26 and 30).
- domain assumption Diffeomorphic gluing of auxiliary null slabs identifies the in and out boundaries with the same abstract null surface (Figure 4).
invented entities (3)
-
Edge vacuum state T^A
-
Bulk vacuum state |Omega^A_{A'}>
-
Generalized projector P
Cite this review
Pith. "Pith review of Foundational Structure of Local Amplitudes in Quantum Gravity." pith.science (2026). https://pith.science/paper/IPI7VAWM
@misc{pith2026250809679,
author = {Pith},
title = {Pith review of: Foundational Structure of Local Amplitudes in Quantum Gravity},
year = {2026},
howpublished = {\url{https://pith.science/paper/IPI7VAWM}},
note = {Machine review of arXiv:2508.09679}
}
read the original abstract
There has been recently renewed interest in the quantisation of gravity by considering local subsystems on light-like hypersurfaces. The main purpose of this paper is to present a theory-independent perspective on these developments assuming only basic knowledge of quantum theory and general relativity. In addition, we present a top-down approach to constructing local amplitudes in causal diamonds. The fundamental building block is a slab of light-like geometry (e.g. a segment of a light cone embedded into spacetime). Each slab is a three-dimensional light-like hypersurface bounded by two cuts, its past and future corners. After briefly reviewing the timeless formalism of quantum theory, we equip each null slab a with a kinematical Hilbert space that factorizes into constituents associated to the three-dimensional interior and its two corners. Upon assuming the existence of vacuum states for the bulk and boundary symmetries and a fundamental projector onto physical states, we explain how to introduce local amplitudes by contracting boundary states according to the pattern of a causal diamond. Finally, we show that the resulting local transition amplitudes satisfy Ward identities and charge conservation for the underlying symmetries. The paper closes with a summary and discussion for how different approaches to quantum gravity can realise our proposal in practice.
Figures
Reference graph
Works this paper leans on
-
[11]
Quantum Geometry of the Light Cone: Fock Representation and Spectrum of Radiated Power,
W. Wieland, “Quantum Geometry of the Light Cone: Fock Representation and Spectrum of Radiated Power,”arXiv:2504.10802. 18
-
[1]
Quantum Theory of Gravity. I. The Canonical Theory,
B. S. DeWitt, “Quantum Theory of Gravity. I. The Canonical Theory,”Phys. Rev. 160 (Aug, 1967) 1113–1148
1967
-
[2]
Ashtekar,Lectures on Non-Pertubative Canonical Gravity
A. Ashtekar,Lectures on Non-Pertubative Canonical Gravity. World Scientific, 1991
1991
-
[3]
Kiefer,Quantum Gravity
C. Kiefer,Quantum Gravity. Cambridge University Press, Cambridge, 2005
2005
-
[4]
Thiemann,Introduction to Modern Canonical Quantum General Relativity
C. Thiemann,Introduction to Modern Canonical Quantum General Relativity. Cambridge University Press, 2007
2007
-
[5]
Rovelli,Quantum Gravity
C. Rovelli,Quantum Gravity. Cambridge University Press, Cambridge, 2008
2008
-
[6]
Partial and complete observables for Hamiltonian constrained systems,
B. Dittrich, “Partial and complete observables for Hamiltonian constrained systems,” Gen. Rel. Grav.39 (2007) 1891–1927, arXiv:gr-qc/0411013
arXiv 2007
-
[7]
The symplectic 2-form for gravity in terms of free null initial data,
M. P. Reisenberger, “The symplectic 2-form for gravity in terms of free null initial data,” Class. Quant. Grav.30 (2013) 155022, arXiv:1211.3880
arXiv 2013
Show all 121 references
-
[8]
Integrable structures and the quantization of free null initial data for gravity,
A. Fuchs and M. P. Reisenberger, “Integrable structures and the quantization of free null initial data for gravity,”Class. Quant. Grav.34 (2017), no. 18, 185003, arXiv:1704.06992
2017 arXiv
-
[9]
The Poisson brackets of free null initial data for vacuum general relativity,
M. P. Reisenberger, “The Poisson brackets of free null initial data for vacuum general relativity,”Class. Quant. Grav.35 (2018), no. 18, 185012, arXiv:1804.10284
2018 arXiv
-
[10]
Fock representation of gravitational boundary modes and the discreteness of the area spectrum,
W. Wieland, “Fock representation of gravitational boundary modes and the discreteness of the area spectrum,”Ann. Henri Poincaré18 (2017) 3695–3717, arXiv:1706.00479
2017 arXiv
-
[12]
New boundary variables for classical and quantum gravity on a null surface,
W. Wieland, “New boundary variables for classical and quantum gravity on a null surface,” Class. Quantum Grav.34 (2017) 215008, arXiv:1704.07391
2017 arXiv
-
[13]
Causal diamonds in (2+1)-dimensional quantum gravity,
R. Andrade e Silva and T. Jacobson, “Causal diamonds in (2+1)-dimensional quantum gravity,”Phys. Rev. D107 (2023), no. 2, 024033,arXiv:2203.10084
2023 arXiv
-
[14]
Entropy of causal diamond ensembles,
T. Jacobson and M. R. Visser, “Entropy of causal diamond ensembles,”SciPost Phys. 15 (2023), no. 1, 023,arXiv:2212.10608
2023 arXiv
-
[15]
Quantum Mechanics of a Spherically Symmetric Causal Diamond in Minkowski Spacetime,
M. W. Bub, T. He, P. Mitra, Y. Zhang, and K. M. Zurek, “Quantum Mechanics of a Spherically Symmetric Causal Diamond in Minkowski Spacetime,”Phys. Rev. Lett. 134 (2025), no. 12, 121501,arXiv:2408.11094
2025 arXiv
-
[16]
Corner symmetry and quantum geometry,
L. Freidel, M. Geiller, and W. Wieland, “Corner symmetry and quantum geometry,” inHandbook of Quantum Gravity, L. M. Cosimo Bambi and I. Shapiro, eds. Springer, 2023.arXiv:2302.12799
2023 arXiv
-
[17]
Quantum geometry of the null cone,
W. Wieland, “Quantum geometry of the null cone,”arXiv:2401.17491
-
[18]
Evidence for Planck luminosity bound in quantum gravity,
W. Wieland, “Evidence for Planck luminosity bound in quantum gravity,”Class. Quant. Grav. 42 (2025), no. 6, 06LT01
2025
-
[19]
Quantum null geometry and gravity,
L. Ciambelli, L. Freidel, and R. G. Leigh, “Quantum null geometry and gravity,” JHEP 12 (2024) 028, arXiv:2407.11132
2024 arXiv
-
[20]
Null infinity as an open Hamiltonian system,
W. Wieland, “Null infinity as an open Hamiltonian system,”JHEP 04 (2021) 095, arXiv:2012.01889
2021 arXiv
-
[21]
Carrollian-holographic Derivation of BMS Flux-balance Laws,
A. Fiorucci, S. Pekar, P. Marios Petropoulos, and M. Vilatte, “Carrollian-holographic Derivation of BMS Flux-balance Laws,” arXiv:2505.00077
-
[22]
Carrollian Perspective on Celestial Holography,
L. Donnay, A. Fiorucci, Y. Herfray, and R. Ruzziconi, “Carrollian Perspective on Celestial Holography,”Phys. Rev. Lett.129 (2022), no. 7, 071602, arXiv:2202.04702
2022 arXiv
-
[23]
The Problem of Time and its Quantum Resolution,
M. S. Klinger and R. G. Leigh, “The Problem of Time and its Quantum Resolution,” arXiv:2504.00152
-
[24]
Quasilocal mass in general relativity,
M.-T. Wang and S.-T. Yau, “Quasilocal mass in general relativity,”Phys. Rev. Lett. 102 (2009) 021101, arXiv:0804.1174
2009 arXiv
-
[25]
Quasi-Local Energy-Momentum and Angular Momentum in GR: A Review Article,
L. B. Szabados, “Quasi-Local Energy-Momentum and Angular Momentum in GR: A Review Article,”Living Rev. Rel.7 (2004) 4
2004
-
[27]
Gravitational dressing, soft charges, and perturbative gravitational splitting,
S. B. Giddings, “Gravitational dressing, soft charges, and perturbative gravitational splitting,”Phys. Rev. D100 (2019), no. 12, 126001, arXiv:1903.06160
2019 arXiv
-
[28]
Edge modes as dynamical frames: charges from post-selection in generally covariant theories,
S. Carrozza, S. Eccles, and P. A. Hoehn, “Edge modes as dynamical frames: charges from post-selection in generally covariant theories,”arXiv:2205.00913
-
[29]
Crossed products and quantum reference frames: on the observer-dependence of gravitational entropy,
J. De Vuyst, S. Eccles, P. A. Hoehn, and J. Kirklin, “Crossed products and quantum reference frames: on the observer-dependence of gravitational entropy,” JHEP 07 (2025) 063, arXiv:2412.15502. 19
2025 arXiv
-
[30]
Metriplectic geometry for gravitational subsystems,
V. Kabel and W. Wieland, “Metriplectic geometry for gravitational subsystems,” Phys. Rev. D106 (2022), no. 6, 064053,arXiv:2206.00029
2022 arXiv
-
[31]
Wave Function of the Universe,
J. Hartle and S. Hawking, “Wave Function of the Universe,”Phys.Rev. D28 (1983) 2960–2975
1983
-
[32]
Consistent histories and the interpretation of quantum mechanics,
R. B. Griffiths, “Consistent histories and the interpretation of quantum mechanics,” Journal of Statistical Physics36 (1984), no. 1, 219–272
1984
-
[33]
Schlick,Gesetz, Kausalität und Wahrscheinlichkeit
M. Schlick,Gesetz, Kausalität und Wahrscheinlichkeit. Gerold & Co, Vienna, 1948
1948
-
[34]
The Cauchy problem on a characteristic cone for the Einstein equations in arbitrary dimensions,
Y. Choquet-Bruhat, P. T. Chrusciel, and J. M. Martin-Garcia, “The Cauchy problem on a characteristic cone for the Einstein equations in arbitrary dimensions,” Annales Henri Poincare12 (2011) 419–482, arXiv:1006.4467
2011 arXiv
-
[35]
The Many ways of the characteristic Cauchy problem,
P. T. Chrusciel and T.-T. Paetz, “The Many ways of the characteristic Cauchy problem,” Class. Quant. Grav.29 (2012) 145006, arXiv:1203.4534
2012 arXiv
-
[36]
Characteristic gluing withΛ: 1. Linearised Einstein equations on four-dimensional spacetimes,
P. T. Chruściel and W. Cong, “Characteristic gluing withΛ: 1. Linearised Einstein equations on four-dimensional spacetimes,”Beijing J. Pure Appl. Math. 1 (2024), no. 2, 689–796,arXiv:2212.10052
2024 arXiv
-
[37]
The characteristic gluing problem for the Einstein equations and applications,
S. Aretakis, S. Czimek, and I. Rodnianski, “The characteristic gluing problem for the Einstein equations and applications,”Duke Math. J.174 (2025), no. 2, 355–402, arXiv:2107.02441
2025 arXiv
-
[38]
Krasnov,Formulations of General Relativity: Gravity, Spinors and Differential Forms
K. Krasnov,Formulations of General Relativity: Gravity, Spinors and Differential Forms. Cambridge Monographs on Mathematical Physics. Cambridge University Press, 2020
2020
-
[39]
Henneaux and C
M. Henneaux and C. Teitelboim,Quantization of Gauge Systems. Princeton University Press, Princeton, 1992
1992
-
[40]
First order gravity on the light front,
S. Alexandrov and S. Speziale, “First order gravity on the light front,”Phys. Rev. D 91 (Mar, 2015) 064043
2015
-
[41]
Hypersurface-deformation algebroids and effective spacetime models,
M. Bojowald, S. Brahma, U. Buyukcam, and F. D’Ambrosio, “Hypersurface-deformation algebroids and effective spacetime models,”Phys. Rev. D 94 (2016), no. 10, 104032,arXiv:1610.08355
2016 arXiv
-
[42]
How commutators of constraints reflect the spacetime structure,
C. Teitelboim, “How commutators of constraints reflect the spacetime structure,” Annals of Physics79 (1973), no. 2, 542–557
1973
-
[43]
Arnowitt, S
R. Arnowitt, S. Deser, and C. Misner,The dynamics of general relativity, ch. 7, pp. 227–264. Wiley, New York, 1962.arXiv:gr-qc/0405109v1
1962 arXiv
-
[44]
Geometrodynamics regained,
S. A. Hojman, K. Kuchař, and C. Teitelboim, “Geometrodynamics regained,” Annals of Physics96 (1976), no. 1, 88–135
1976
-
[45]
Isenberg,The Initial Value Problem in General Relativity, pp
J. Isenberg,The Initial Value Problem in General Relativity, pp. 303–321. 2014. arXiv:1304.1960
2014 arXiv
-
[46]
Gravitational SL(2,R) algebra on the light cone,
W. Wieland, “Gravitational SL(2,R) algebra on the light cone,”JHEP 07 (2021) 057, arXiv:2104.05803
2021 arXiv
-
[47]
Null Raychaudhuri: Canonical Structure and the Dressing Time,
L. Ciambelli, L. Freidel, and R. G. Leigh, “Null Raychaudhuri: Canonical Structure and the Dressing Time,”arXiv:2309.03932. 20
-
[48]
Discreteness of area and volume in quantum gravity,
C. Rovelli and L. Smolin, “Discreteness of area and volume in quantum gravity,” Nuclear Physics B442 (1995), no. 3, 593–619,arXiv:gr-qc/9411005
1995 arXiv
-
[49]
Emergence of Riemannian Quantum Geometry,
H. M. Haggard, J. Lewandowski, and H. Sahlmann, “Emergence of Riemannian Quantum Geometry,” inHandbook of Quantum Gravity, C. Bambi, L. Modesto, and I. Shapiro, eds. Springer, 2023.arXiv:2302.02840
2023 arXiv
-
[50]
Quantum theory of geometry I.: Area operators,
A. Ashtekar and J. Lewandowski, “Quantum theory of geometry I.: Area operators,” Class. Quant. Grav.14 (1997) A55–A82, arXiv:gr-qc/9602046
1997 arXiv
-
[51]
Flux-area operator and black hole entropy,
G. J. Fernando Barbero, J. Lewandowski, and E. J. S. Villasenor, “Flux-area operator and black hole entropy,”Phys. Rev. D80 (2009) 044016, arXiv:0905.3465
2009 arXiv
-
[52]
Evolution without evolution: Dynamics described by stationary observables,
D. N. Page and W. K. Wootters, “Evolution without evolution: Dynamics described by stationary observables,”Phys. Rev. D27 (Jun, 1983) 2885–2892
1983
-
[53]
Quantum mechanics without time: A model,
C. Rovelli, “Quantum mechanics without time: A model,”Phys. Rev. D42 (Oct,
- [54]
-
[55]
Topological quantum field theories,
M. Atiyah, “Topological quantum field theories,”Inst. Hautes Etudes Sci. Publ. Math. 68 (1989) 175–186
1989
-
[56]
(2+1)-Dimensional Gravity as an Exactly Soluble System,
E. Witten, “(2+1)-Dimensional Gravity as an Exactly Soluble System,”Nucl. Phys. B 311 (1988) 46
1988
-
[57]
Carlip,Quantum gravity in 2+1 dimensions
S. Carlip,Quantum gravity in 2+1 dimensions. Cambridge University Press, 2003
2003
-
[58]
Quantum gravity as topological quantum field theory,
J. W. Barrett, “Quantum gravity as topological quantum field theory,”J. Math. Phys. 36 (1995) 6161–6179, arXiv:gr-qc/9506070
1995 arXiv
-
[59]
A ’General boundary’ formulation for quantum mechanics and quantum gravity,
R. Oeckl, “A ’General boundary’ formulation for quantum mechanics and quantum gravity,”Phys. Lett. B575 (2003) 318–324, arXiv:hep-th/0306025
2003 arXiv
-
[60]
General boundary quantum field theory: Foundations and probability interpretation,
R. Oeckl, “General boundary quantum field theory: Foundations and probability interpretation,” Adv. Theor. Math. Phys.12 (2008), no. 2, 319–352, arXiv:hep-th/0509122
2008 arXiv
-
[61]
A positive formalism for quantum theory in the general boundary formulation,
R. Oeckl, “A positive formalism for quantum theory in the general boundary formulation,” Found. Phys. 43 (2013) 1206–1232, arXiv:1212.5571
2013 arXiv
-
[62]
A local and operational framework for the foundations of physics,
R. Oeckl, “A local and operational framework for the foundations of physics,” Adv. Theor. Math. Phys.23 (2019), no. 2, 437–592,arXiv:1610.09052
2019 arXiv
-
[63]
Functional Schrodinger equation for scalar QED,
C. Kiefer, “Functional Schrodinger equation for scalar QED,”Phys. Rev. D45 (1992) 2044–2056
1992
-
[64]
Schrödinger-Feynman quantization and composition of observables in general boundary quantum field theory,
R. Oeckl, “Schrödinger-Feynman quantization and composition of observables in general boundary quantum field theory,”Adv. Theor. Math. Phys.19 (2015) 451–506, arXiv:1201.1877
2015 arXiv
-
[65]
Quantization of systems with temporally varying discretization I: Evolving Hilbert spaces,
P. A. Höhn, “Quantization of systems with temporally varying discretization I: Evolving Hilbert spaces,”J. Math. Phys.55 (2014) 083508, arXiv:1401.6062
2014 arXiv
-
[67]
Quantum correlations with no causal order,
O. Oreshkov, F. Costa, and Č. Brukner, “Quantum correlations with no causal order,” Nature Communications3 (2012), no. 1, 1092
2012
-
[68]
Witnessing causal nonseparability,
M. Araújo, C. Branciard, F. Costa, A. Feix, C. Giarmatzi, and v. Brukner, “Witnessing causal nonseparability,”New J. Phys.17 (2015), no. 10, 102001, arXiv:1506.03776
2015 arXiv
-
[69]
The operator tensor formulation of quantum theory,
L. Hardy, “The operator tensor formulation of quantum theory,”Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 370 (2012), no. 1971, 3385–3417,arXiv:1201.4390
2012 arXiv
-
[70]
The Covariant Phase Space Of Asymptotically Flat Gravitational Fields,
A. Ashtekar, L. Bombelli, and O. Reula, “The Covariant Phase Space Of Asymptotically Flat Gravitational Fields,” inMechanics, Analysis and Geometry: 200 Years after Lagrange, M. Francaviglia and D. Holm, eds. North Holland, Amsterdam, 1990
1990
-
[71]
A General definition of ‘conserved quantities’ in general relativity and other theories of gravity,
R. M. Wald and A. Zoupas, “A General definition of ‘conserved quantities’ in general relativity and other theories of gravity,”Phys. Rev. D61 (2000) 084027, arXiv:gr-qc/9911095
2000 arXiv
-
[72]
Covariant phase space with boundaries,
D. Harlow and J.-q. Wu, “Covariant phase space with boundaries,”Journal of High Energy Physics2020 (2020), no. 10, 146
2020
-
[73]
Boundary effects in General Relativity with tetrad variables,
R. Oliveri and S. Speziale, “Boundary effects in General Relativity with tetrad variables,” arXiv:1912.01016
1912 arXiv
-
[74]
4d Lorentzian Holst action with topological terms,
D. J. Rezende and A. Perez, “4d Lorentzian Holst action with topological terms,” Phys. Rev. D79 (2009) 064026, arXiv:0902.3416
2009 arXiv
-
[75]
Edge states in gravity and black hole physics,
A. P. Balachandran, L. Chandar, and A. Momen, “Edge states in gravity and black hole physics,”Nucl. Phys. B461 (1996) 581–596, arXiv:gr-qc/9412019
1996 arXiv
-
[76]
Statistical mechanics of the (2+1)-dimensional black hole,
S. Carlip, “Statistical mechanics of the (2+1)-dimensional black hole,”Phys. Rev. D 51 (Jan, 1995) 632–637
1995
-
[77]
Local subsystems in gauge theory and gravity,
W. Donnelly and L. Freidel, “Local subsystems in gauge theory and gravity,” arXiv:1601.04744
-
[78]
Observables, gravitational dressing, and obstructions to locality and subsystems,
W. Donnelly and S. B. Giddings, “Observables, gravitational dressing, and obstructions to locality and subsystems,”Phys. Rev. D94 (2016), no. 10, 104038, arXiv:1607.01025
2016 arXiv
-
[79]
The observer’s ghost: notes on a field space connection,
H. Gomes and A. Riello, “The observer’s ghost: notes on a field space connection,” JHEP 05 (2017) 017, arXiv:1608.08226
2017 arXiv
-
[80]
Local phase space and edge modes for diffeomorphism-invariant theories,
A. J. Speranza, “Local phase space and edge modes for diffeomorphism-invariant theories,” JHEP 02 (2018) 021, arXiv:1706.05061
2018 arXiv
-
[81]
Edge modes and corner ambiguities in 3d Chern-Simons theory and gravity,
M. Geiller, “Edge modes and corner ambiguities in 3d Chern-Simons theory and gravity,” Nucl. Phys. B924 (2017) 312–365, arXiv:1703.04748
2017 arXiv
-
[82]
Gravity Edges Modes and Hayward Term,
T. Takayanagi and K. Tamaoka, “Gravity Edges Modes and Hayward Term,” JHEP 02 (2020) 167, arXiv:1912.01636
2020 arXiv
-
[83]
Bundle geometry of the connection space, covariant Hamiltonian formalism, the problem of boundaries in gauge theories, and the dressing field method,
J. François, “Bundle geometry of the connection space, covariant Hamiltonian formalism, the problem of boundaries in gauge theories, and the dressing field method,” Journal of High Energy Physics2021 (2021), no. 3, 225, arXiv:2010.01597. 22
2021 arXiv
-
[84]
Gravitational edge modes: from Kac–Moody charges to Poincaré networks,
L. Freidel, E. R. Livine, and D. Pranzetti, “Gravitational edge modes: from Kac–Moody charges to Poincaré networks,”Class. Quant. Grav.36 (2019), no. 19, 195014,arXiv:1906.07876
2019 arXiv
-
[85]
Edge modes of gravity. Part I. Corner potentials and charges,
L. Freidel, M. Geiller, and D. Pranzetti, “Edge modes of gravity. Part I. Corner potentials and charges,”JHEP 11 (2020) 026, arXiv:2006.12527
2020 arXiv
-
[86]
Embeddings and Integrable Charges for Extended Corner Symmetry,
L. Ciambelli, R. G. Leigh, and P.-C. Pai, “Embeddings and Integrable Charges for Extended Corner Symmetry,”Phys. Rev. Lett.128 (Apr, 2022) 171302, arXiv:2111.13181
2022 arXiv
-
[87]
Extended corner symmetry, charge bracket and Einstein’s equations,
L. Freidel, R. Oliveri, D. Pranzetti, and S. Speziale, “Extended corner symmetry, charge bracket and Einstein’s equations,”JHEP 09 (2021) 083, arXiv:2104.12881
2021 arXiv
-
[88]
Gravitational edge modes, coadjoint orbits, and hydrodynamics,
W. Donnelly, L. Freidel, S. F. Moosavian, and A. J. Speranza, “Gravitational edge modes, coadjoint orbits, and hydrodynamics,”JHEP 09 (2021) 008, arXiv:2012.10367
2021 arXiv
-
[89]
Diffeomorphism-invariant observables and dynamical frames in gravity: reconciling bulk locality with general covariance,
C. Goeller, P. A. Hoehn, and J. Kirklin, “Diffeomorphism-invariant observables and dynamical frames in gravity: reconciling bulk locality with general covariance,” arXiv:2206.01193
-
[90]
Linking Edge Modes and Geometrical Clocks in Linearized Gravity,
K. Giesel, V. Kabel, and W. Wieland, “Linking Edge Modes and Geometrical Clocks in Linearized Gravity,”arXiv:2410.17339
-
[91]
Symmetry, Reference Frames, and Relational Quantities in Quantum Mechanics,
L. Loveridge, T. Miyadera, and P. Busch, “Symmetry, Reference Frames, and Relational Quantities in Quantum Mechanics,”Foundations of Physics48 (2018), no. 2, 135–198
2018
-
[92]
Quantum mechanics and the covariance of physical laws in quantum reference frames,
F. Giacomini, E. Castro-Ruiz, and Č. Brukner, “Quantum mechanics and the covariance of physical laws in quantum reference frames,”Nature Commun. 10 (2019), no. 1, 494,arXiv:1712.07207
2019 arXiv
-
[93]
Relativistic Quantum Reference Frames: The Operational Meaning of Spin,
F. Giacomini, E. Castro-Ruiz, and Č. Brukner, “Relativistic Quantum Reference Frames: The Operational Meaning of Spin,”Phys. Rev. Lett.123 (2019), no. 9, 090404, arXiv:1811.08228
2019 arXiv
-
[94]
A change of perspective: switching quantum reference frames via a perspective-neutral framework,
A. Vanrietvelde, P. A. Hoehn, F. Giacomini, and E. Castro-Ruiz, “A change of perspective: switching quantum reference frames via a perspective-neutral framework,” Quantum 4 (2020) 225, arXiv:1809.00556
2020 arXiv
-
[95]
The Trinity of Relational Quantum Dynamics,
P. A. Höhn, A. R. Smith, and M. P. Lock, “The Trinity of Relational Quantum Dynamics,” arXiv:1912.00033
1912 arXiv
-
[96]
Relative subsystems and quantum reference frame transformations,
E. Castro-Ruiz and O. Oreshkov, “Relative subsystems and quantum reference frame transformations,” arXiv:2110.13199
-
[97]
Asymptotic higher spin symmetries I: covariant wedge algebra in gravity,
N. Cresto and L. Freidel, “Asymptotic higher spin symmetries I: covariant wedge algebra in gravity,”Lett. Math. Phys.115 (2025), no. 2, 39,arXiv:2409.12178
2025 arXiv
-
[98]
Asymptotic Higher Spin Symmetries II: Noether Realization in Gravity,
N. Cresto and L. Freidel, “Asymptotic Higher Spin Symmetries II: Noether Realization in Gravity,”arXiv:2410.15219
-
[99]
CarrollianL w1+∞ representation from twistor space,
L. Donnay, L. Freidel, and Y. Herfray, “CarrollianL w1+∞ representation from twistor space,”SciPost Phys. 17 (2024), no. 4, 118,arXiv:2402.00688
2024 arXiv
-
[100]
Orbit method for Quantum Corner Symmetries,
G. Neri and L. Varrin, “Orbit method for Quantum Corner Symmetries,” 23 arXiv:2507.10683
-
[101]
Zakopane lectures on loop gravity,
C. Rovelli, “Zakopane lectures on loop gravity,”PoS QGQGS2011 (2011) 003, arXiv:1102.3660
2011 arXiv
-
[102]
The Spin-Foam Approach to Quantum Gravity,
A. Perez, “The Spin-Foam Approach to Quantum Gravity,”Living Rev. Rel.16 (2013), no. 3,arXiv:1205.2019
2013 arXiv
-
[103]
The strange equation of quantum gravity,
C. Rovelli, “The strange equation of quantum gravity,”Class. Quant. Grav.32 (2015), no. 12, 124005,arXiv:1506.00927
2015 arXiv
-
[104]
Strominger,Lectures on the Infrared Structure of Gravity and Gauge Theory
A. Strominger,Lectures on the Infrared Structure of Gravity and Gauge Theory. Princeton University Press, Princeton, 2018.arXiv:1703.05448
2018 arXiv
-
[105]
Sub-subleading soft gravitons: New symmetries of quantum gravity?,
M. Campiglia and A. Laddha, “Sub-subleading soft gravitons: New symmetries of quantum gravity?,”Phys. Lett. B764 (2017) 218–221, arXiv:1605.09094
2017 arXiv
-
[106]
Sub-subleading soft graviton theorem from asymptotic Einstein’s equations,
L. Freidel, D. Pranzetti, and A.-M. Raclariu, “Sub-subleading soft graviton theorem from asymptotic Einstein’s equations,”JHEP 05 (2022) 186, arXiv:2111.15607
2022 arXiv
-
[107]
Implementation of the Quantum Equivalence Principle,
L. Hardy, “Implementation of the Quantum Equivalence Principle,” inProgress and Visions in Quantum Theory in View of Gravity, F. Finster, D. Giulini, J. Kleiner, and J. Tolksdorf, eds., pp. 189–220. Springer International Publishing, Cham, 2020
2020
-
[108]
Quantum mechanics and the covariance of physical laws in quantum reference frames,
F. Giacomini, E. Castro-Ruiz, and Č. Brukner, “Quantum mechanics and the covariance of physical laws in quantum reference frames,”Nature Communications 10 (2019), no. 1, 494
2019
-
[109]
Partition functions and topology changing amplitudes in the 3-D lattice gravity of Ponzano and Regge,
H. Ooguri, “Partition functions and topology changing amplitudes in the 3-D lattice gravity of Ponzano and Regge,”Nucl. Phys. B382 (1992) 276–304, arXiv:hep-th/9112072
1992 arXiv
-
[110]
The Ponzano-Regge model,
J. W. Barrett and I. Naish-Guzman, “The Ponzano-Regge model,”Class. Quant. Grav. 26 (2009) 155014, arXiv:0803.3319
2009 arXiv
-
[111]
Spin foam models and the classical action principle,
L. Freidel and K. Krasnov, “Spin foam models and the classical action principle,” Adv. Theor. Math. Phys.2 (1999) 1183–1247, arXiv:hep-th/9807092
1999 arXiv
-
[112]
LQG vertex with finite Immirzi parameter,
J. Engle, E. Livine, and C. Rovelli, “LQG vertex with finite Immirzi parameter,” Nucl. Phys. B799 (2008) 136–149, arXiv:0711.0146
2008 arXiv
-
[113]
Flipped spinfoam vertex and loop gravity,
J. Engle, R. Pereira, and C. Rovelli, “Flipped spinfoam vertex and loop gravity,” Nucl. Phys. B798 (2008) 251–290, arXiv:0708.1236v1
2008 arXiv
-
[114]
Rovelli and F
C. Rovelli and F. Vidotto,Covariant Loop Quantum Gravity: An Elementary Introduction to Quantum Gravity and Spinfoam Theory. Cambridge Monographs on Mathematical Physics. Cambridge University Press, 11, 2014
2014
-
[115]
The continuum limit of loop quantum gravity - a framework for solving the theory,
B. Dittrich, “The continuum limit of loop quantum gravity - a framework for solving the theory,” inLoop Quantum Gravity, The First Thirty Years, A. Abhay and J. Pullin, eds., vol. 4. World Scientific, 2017.arXiv:1409.1450
2017 arXiv
-
[116]
Coarse Graining Spin Foam Quantum Gravity—A Review,
S. Steinhaus, “Coarse Graining Spin Foam Quantum Gravity—A Review,”Front. in Phys. 8 (2020) 295, arXiv:2007.01315
2020 arXiv
-
[117]
Effective Spin Foam Models for 24 Four-Dimensional Quantum Gravity,
S. K. Asante, B. Dittrich, and H. M. Haggard, “Effective Spin Foam Models for 24 Four-Dimensional Quantum Gravity,”Phys. Rev. Lett.125 (2020), no. 23, 231301, arXiv:2004.07013
2020 arXiv
-
[118]
Spin foams, Refinement limit and Renormalization,
S. K. Asante, B. Dittrich, and S. Steinhaus, “Spin foams, Refinement limit and Renormalization,” arXiv:2211.09578
-
[119]
Spinfoam Models for Quantum Gravity,
E. R. Livine, “Spinfoam Models for Quantum Gravity,” inEncyclopedia of Mathematical Physics (Second Edition), R. Szabo and M. Bojowald, eds., pp. 507–519. Academic Press, Oxford, second edition ed., 2025
2025
-
[120]
Discrete and continuum third quantization of Gravity,
S. Gielen and D. Oriti, “Discrete and continuum third quantization of Gravity,” in Quantum Field Theory and Gravity: Conceptual and Mathematical Advances in the Search for a Unified Framework, pp. 41–64. 2012.arXiv:1102.2226
2012 arXiv
-
[121]
Editorial for the Special Issue
S. Carrozza, S. Gielen, and D. Oriti, “Editorial for the Special Issue ”Progress in Group Field Theory and Related Quantum Gravity Formalisms”,”Universe 6 (2020), no. 1, 19,arXiv:2001.08428
2020 arXiv
-
[122]
Oriti,Group field theory and loop quantum gravity., pp
D. Oriti,Group field theory and loop quantum gravity., pp. 125–151. World Scientific, 2017
2017
-
[123]
The group field theory approach to quantum gravity,
D. Oriti, “The group field theory approach to quantum gravity,” inApproaches to Quantum Gravity. Cambridge University Press, Cambridge, 2009. 25
2009
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