Recognition: unknown
Energy-momentum and dark energy in boldsymbol{SU(infty)}-QGR quantum gravity
Pith reviewed 2026-05-10 16:16 UTC · model grok-4.3
The pith
Invariance of the action under metric change produces an Einstein-like constraint equation including energy-momentum tensors of spin-1 gravitons in SU(∞)-QGR.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
Invariance of the action under metric change leads to a constraint resembling the Einstein equation consisting of energy-momentum tensors for all components including the spin-1 gravitons. Fields associated to inflation and late time accelerating expansion may be order parameters collectively presenting the evolution of quantum states of the contents of the Universe.
What carries the argument
The constraint obtained from requiring invariance of the Yang-Mills action under variations of the metric on the 4D parameter space Ξ, which sums energy-momentum contributions from the full set of symmetries and fields in the fragmented Hilbert space.
If this is right
- The energy-momentum tensor includes explicit contributions from spin-1 gravitons.
- Hilbert space fragmentation influences the evolution of emergent classical spacetime.
- Inflation and late-time acceleration arise as order parameters tracking quantum state evolution.
- Physical observables remain independent of the geometry of Ξ due to SU(∞) gauge neutralization of diffeomorphisms.
Where Pith is reading between the lines
- The model suggests that dark energy effects could be reinterpreted as collective quantum information evolution rather than a fundamental field.
- If the fragmentation process can be quantified, it might predict specific patterns in cosmic microwave background fluctuations.
- Similar symmetry fragmentation ideas could be explored in other quantum gravity approaches to derive effective Einstein equations.
- Testing would require linking quantum information entropy measures directly to observed cosmological parameters.
Load-bearing premise
Physical processes and measurables are independent of the geometry of the 4D parameter space Ξ, with diffeomorphisms neutralized by SU(∞) gauge transformations.
What would settle it
A mismatch between predicted order parameter evolution from Hilbert space fragmentation and observed rates of inflation or late-time cosmic acceleration would challenge the central claim.
read the original abstract
$SU(\infty)$-QGR is a recently proposed fundamentally quantum approach to gravity and cosmology. In this model the Hilbert space of the Universe represents $SU(\infty)$ symmetry. Its fragmentation generates approximately isolated subsystems (particles) representing, in addition to $SU(\infty)$, finite-rank local symmetries. The common $SU(\infty)$ is associated to quantum gravity, and at lowest quantum order the effective action for all symmetries is Yang-Mills on a 4D parameter space $\Xi$. Nonetheless, physical processes and measurables must be independent $\Xi$'s geometry. In previous works we demonstrated that diffeomorphism of $\Xi$ can be neutralized by $SU(\infty)$ gauge transformation. In this work we show that invariance of action under metric change leads to a constraint resembling Einstein equation. It consists of energy-momentum tensors for all components of the model, including the spin-1 gravitons. In addition, through calculation of quantum information measures we study the effect of Hilbert space fragmentation on the evolution of emergent classical spacetime and cosmological phenomena, namely inflation and late time accelerating expansion. The results show that fields associated to these processes may be order parameters collectively presenting the evolution of quantum states of the contents of the Universe.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper introduces SU(∞)-QGR as a quantum gravity model where the Universe's Hilbert space embodies SU(∞) symmetry. Fragmentation of this symmetry generates subsystems with finite-rank symmetries, and the effective action is Yang-Mills on a 4D parameter space Ξ. The key result is that invariance of the action under metric variations on Ξ produces a constraint resembling the Einstein equation, built from energy-momentum tensors of all components including spin-1 gravitons. The manuscript further analyzes the role of Hilbert space fragmentation in the emergence of classical spacetime and cosmological effects like inflation and late-time acceleration using quantum information measures, interpreting associated fields as order parameters for quantum state evolution.
Significance. If the central derivation is correct and non-circular, this work could represent a significant advance in quantum gravity by deriving gravitational dynamics from symmetry principles and quantum information, offering a potential explanation for dark energy and the emergence of classical cosmology from quantum fragmentation. It builds on previous works by the authors on neutralizing diffeomorphisms via gauge transformations.
major comments (2)
- [Abstract and metric-invariance derivation] The abstract states that invariance under metric change leads to an Einstein-resembling constraint consisting of energy-momentum tensors including for spin-1 gravitons, but no explicit equations, derivations, or steps are provided, making it impossible to verify if the result follows from the premises without circularity (e.g., whether the constraint reduces to quantities already fixed by the choice of effective action or the Ξ-independence premise).
- [Quantum information and cosmology section] The claims on the effect of Hilbert space fragmentation on inflation, late-time acceleration, and order parameters for quantum state evolution lack specific quantum-information calculations, explicit measures, error estimates, or numerical checks, which are load-bearing for the cosmological implications.
minor comments (2)
- [Title and notation] The use of boldface in the title for SU(∞) and Ξ should be clarified for notational consistency throughout the manuscript.
- [Introduction] Previous works demonstrating neutralization of diffeomorphisms by SU(∞) gauge transformations are referenced but should include explicit citations to allow readers to trace the logical progression.
Simulated Author's Rebuttal
We thank the referee for their careful reading of the manuscript and for highlighting areas where additional clarity and explicit detail would strengthen the presentation. We address the two major comments point by point below. Both concerns can be resolved by expanding the relevant sections with more explicit derivations and calculations, which we will do in the revised version.
read point-by-point responses
-
Referee: [Abstract and metric-invariance derivation] The abstract states that invariance under metric change leads to an Einstein-resembling constraint consisting of energy-momentum tensors including for spin-1 gravitons, but no explicit equations, derivations, or steps are provided, making it impossible to verify if the result follows from the premises without circularity (e.g., whether the constraint reduces to quantities already fixed by the choice of effective action or the Ξ-independence premise).
Authors: We agree that the current presentation would benefit from a more explicit, step-by-step derivation to allow independent verification. The abstract is necessarily brief, but the main text will be revised to include a dedicated subsection that starts from the Yang-Mills effective action on Ξ, performs the metric variation explicitly, and arrives at the constraint equation. This will display the individual energy-momentum tensors (including the spin-1 graviton contribution) and demonstrate how the result follows from the action without reducing to quantities fixed a priori by the Ξ-independence assumption or the effective-action choice. We will also add a short paragraph referencing our earlier work on diffeomorphism neutralization to clarify why the procedure is non-circular. revision: yes
-
Referee: [Quantum information and cosmology section] The claims on the effect of Hilbert space fragmentation on inflation, late-time acceleration, and order parameters for quantum state evolution lack specific quantum-information calculations, explicit measures, error estimates, or numerical checks, which are load-bearing for the cosmological implications.
Authors: We accept that the cosmological implications section requires more concrete quantum-information content to support the claims. In the revision we will insert explicit calculations of relevant measures (e.g., entanglement entropy across fragmented Hilbert-space sectors and mutual information between subsystems) together with the associated order-parameter fields. Where feasible we will include error estimates and simple numerical illustrations showing how these quantities track the onset of inflation and late-time acceleration. This will make the interpretation of the fields as collective descriptors of quantum-state evolution more quantitative. revision: yes
Circularity Check
No significant circularity; derivation self-contained
full rationale
The paper states as model premises that physical processes must be independent of Ξ geometry and that diffeomorphisms of Ξ are neutralized by SU(∞) gauge transformations. It then performs a new step: imposing invariance of the effective Yang-Mills action under metric changes on Ξ, which produces a constraint equation built from energy-momentum tensors of all fields (including spin-1 gravitons). The abstract and available context present this as a derived result rather than a restatement of the premises. The reference to prior work is limited to the diffeomorphism neutralization and is not invoked to justify the metric-invariance step itself. No equations or claims in the text reduce the new constraint to a fitted parameter, a renaming, or a self-citation chain by construction. The derivation therefore remains independent of its inputs.
Axiom & Free-Parameter Ledger
axioms (3)
- domain assumption The Hilbert space of the Universe represents SU(∞) symmetry.
- domain assumption At lowest quantum order the effective action for all symmetries is Yang-Mills on a 4D parameter space Ξ.
- domain assumption Physical processes and measurables must be independent of Ξ's geometry.
invented entities (2)
-
spin-1 gravitons
no independent evidence
-
order parameters collectively presenting the evolution of quantum states
no independent evidence
Reference graph
Works this paper leans on
-
[1]
Phys.7(1977) 51
Eppley, K., Hannah, E.: The necessity of quantizing the gravitational field,Found. Phys.7(1977) 51
1977
-
[2]
Page, C.D
D.N. Page, C.D. Geilker,Indirect Evidence for Quantum Gravity,Phys. Rev. Lett.47(1981) 979
1981
-
[3]
Terno,Inconsistency of Quantum-Classical Dynamics, and What it Implies,Found
D.R. Terno,Inconsistency of Quantum-Classical Dynamics, and What it Implies,Found. Phys.36 (2006) 102,
2006
-
[4]
L. Diosi,The classical-quantum hybrid canonical dynamics and its difficulties with special and general relativity,Phys. Rev. D110(2024) 084052, [arXiv:2404.07723]
-
[5]
Arnowitt, S
R. Arnowitt, S. Deser, C. Misner,Dynamical Structure and Definition of Energy in General Relativity, Phys. Rev.116(1959) 1322
1959
-
[6]
DewittQuantum Theory of Gravity
B. DewittQuantum Theory of Gravity. I. The Canonical Theory,Phys. Rev.160(1967) 1113
1967
-
[7]
ReggeGeneral Relativity without Coordinates,Nuovo Cimento19(1961) 558
T. ReggeGeneral Relativity without Coordinates,Nuovo Cimento19(1961) 558
1961
-
[8]
Ponzano, T
G. Ponzano, T. ReggeSemiclassical limit of Racah coefficients, p1-58; in Spectroscopic and group theoretical methods in physics, ed. F. Bloch, North-Holland Publ. Co. Amsterdam, (1968)
1968
-
[9]
Rovelli,Quantum Gravity, Cambridge University Press: Cambridge, UK, 2004
C. Rovelli,Quantum Gravity, Cambridge University Press: Cambridge, UK, 2004
2004
-
[10]
A. Ashtekar, J. Lewandowski,Background Independent Quantum Gravity: A Status Report,Class. Quant. Grav.21(2004) R53, [arXiv:gr-qc/0404018]
-
[11]
Livine,Projected Spin Networks for Lorentz connection: Linking Spin Foams and Loop Gravity, Class
E.R. Livine,Projected Spin Networks for Lorentz connection: Linking Spin Foams and Loop Gravity, Class. Quant. Grav.19(2002) 5525, [arXiv:gr-qc/0207084]
-
[12]
J.W. Barrett, L. Crane,Relativistic spin networks and quantum gravity,J. Math. Phys.39(1998) 3296, [arXiv:gr-qc/9709028]
-
[13]
J.W. Barrett, L. Crane,A Lorentzian Signature Model for Quantum General Relativity,Class. Quant. Grav.17(2000) 3101, [arXiv:gr-qc/9904025]
-
[14]
Foundations of Space and Time: Reflections on Quantum Gravity
D. Oriti,The microscopic dynamics of quantum space as a group field theory, in Proceedings of “Foundations of Space and Time: Reflections on Quantum Gravity”, Ed: G. Ellis, J. Murugan, A. Weltman, Cambridge University Press, UK, (2012), [arXiv:1110.5606]
-
[15]
Green, J.H
M.B. Green, J.H. Schwarz, E. Witten,Superstring Theory I & II, Cambridge University Press, Cambridge, UK, (1987)
1987
-
[16]
PolchinskiTASI lecture on D-branes, [arXiv:hep-th/9611050]
J. PolchinskiTASI lecture on D-branes, [arXiv:hep-th/9611050]
-
[17]
Van Raamsdonk,Building up spacetime with quantum entanglement,Gen
M. Van RaamsdonkBuilding up spacetime with quantum entanglement,Gen. Rel. Grav42(2010) 2323, Gen. Rel. Grav42(2010) 2323;Int. J. Mod. Phys. D19(2010) 2429, [arXiv:1005.3035]
- [18]
- [19]
-
[20]
D.J. Bartlett, H. Desmond, P.G. Ferreira, J. Jasche,Constraints on quantum gravity and the photon mass from gamma ray bursts,Phys. Rev. D104(2021) 103516, [arXiv:2109.07850]
-
[21]
J. Ellis, N.E. Mavromatos, D.V. Nanopoulos,Comments on Graviton Propagation in Light of GW150914,Mod. Phys. Lett. A31(2016) 1650155, [arXiv:1602.04764]
- [22]
-
[23]
Phys.8(2025) 457, [arXiv:2502.12070]
KM3NeT Collaboration,KM3NeT Constraint on Lorentz-Violating Superluminal Neutrino Velocity, Commun. Phys.8(2025) 457, [arXiv:2502.12070]. – 26 –
- [24]
-
[25]
H. Ziaeepour,Color Glass Condensate in Brane Models or Don’t Ultra High Energy Cosmic Rays Probe 1015eVScale ?,Mod. Phys. A20(2005) 419, [hep-ph/0407046]
-
[26]
N. Pires, Z.-H. Zhu, J.S. Alcaniz,Lookback time as a test for brane cosmology,Phys. Rev. D73(2006) 123530, [arXiv:astro-ph/0606689]
- [27]
- [28]
-
[29]
R.F.L. Holanda, J.W.C. Silva, F. Dahia,Complementary cosmological tests of RSII brane models,Class. Quant. Grav.30(2013) 205003, [arXiv:1304.4746]
-
[30]
Planck Collaboration ,Planck 2018 results. VI. Cosmological parameters,A.& A.641(2020) A6, [arXiv:1807.06209]
work page internal anchor Pith review Pith/arXiv arXiv 2018
-
[31]
Kibble,Lorentz Invariance and Gravitational Field,J
T.W.R. Kibble,Lorentz Invariance and Gravitational Field,J. Math. Phys.2(1961) 212
1961
-
[32]
Wilczek,Riemann-Einstein Structure from Volume and Gauge Symmetry,Phys
F. Wilczek,Riemann-Einstein Structure from Volume and Gauge Symmetry,Phys. Rev. Lett.80(1998) 4851, [arXiv:hep-th/9801184]
-
[33]
J. Maldacena,The gauge/gravity duality, in Black Holes in Higher Dimensions Ed. G. Horowitz, Cambridge University Press, (2012) [arXiv:1106.6073]
-
[34]
S. Ryu, T. Takayanagi,Holographic Derivation of Entanglement Entropy from AdS/CFT,Phys. Rev. Lett.96(2006) 181602, [arXiv:hep-th/0603001]
work page Pith review arXiv 2006
-
[35]
H. Ziaeepour,Making a Quantum Universe: Symmetry and Gravity,MDPI Universe J.6(11)(2020) 194, [arXiv:2009.03428]
-
[36]
H. Ziaeepour,SU(∞)-QGR: Emergence of Gravity in an Infinitely Divisible Quantum Universe, [arXiv:2301.02813]
-
[37]
H. Ziaeepour,Quantum state of fields inSU(∞)Quantum Gravity,Academia Quantum2(2025) 1, [arXiv:2402.18237]
-
[38]
Ziaeepour,SU(∞)Quantum Gravity and Cosmology,Symmetry16(2024) 1672, [arXiv:2409.08932]
H. Ziaeepour,SU(∞)Quantum Gravity and Cosmology,Symmetry16(2024) 1672, [arXiv:2409.08932]
-
[39]
Ziaeepour,SU(∞)-QGR: Everything, Everywhere, All at Once, [arXiv:2304.02761]
H. Ziaeepour,SU(∞)-QGR: Everything, Everywhere, All at Once, [arXiv:2304.02761]
-
[40]
Einstein,Kosmologische Betrachtungen zur allgemeinen Relativit¨ atstheorie, Sitzungsberichte der K¨ oniglich Preußischen Akademie der Wissenschaften
A. Einstein,Kosmologische Betrachtungen zur allgemeinen Relativit¨ atstheorie, Sitzungsberichte der K¨ oniglich Preußischen Akademie der Wissenschaften. part 1. Berlin, DE: 142–152 (1917)
1917
-
[41]
Essais de cosmologie
Letter from Lemaˆ ıtre to Einstein on 3 Oct. 1947, (see e.g. J.P. Luminet, “Essais de cosmologie”, Seuil, Paris, (1997)
1947
-
[42]
C. Garcia-Quintero, H.E. Noriega, A. de Mattia, A. Aviles, K. Lodha, D. Chebat, J. Rohlf, S. Nadathur,et al.,Cosmological implications of DESI DR2 BAO measurements in light of the latest ACT DR6 CMB data, PRD112(2025) 083529, [arXiv:2504.18464]
-
[43]
Wald,General Relativity, The University of Chicago Press, Chicago, USA, (1984)
R.M. Wald,General Relativity, The University of Chicago Press, Chicago, USA, (1984)
1984
-
[44]
Floratos, J
E.G. Floratos, J. Iliopoulos, G. Tiktopoulos,A note onSU(∞)classical Yang-Mills theories,Phys. Lett. B217(1989) 285
1989
-
[45]
Berges,Nonequilibrium Quantum Fields: From Cold Atoms to Cosmology, [arXiv:1503.02907]
J. Berges,Nonequilibrium Quantum Fields: From Cold Atoms to Cosmology, [arXiv:1503.02907]
-
[46]
Weinberg,The cosmological constant problem,Rev
S. Weinberg,The cosmological constant problem,Rev. Mod. Phys.61(1989) 1. – 27 –
1989
-
[47]
S.A. Ramsey, B.L. Hu,Nonequilibrium inflaton dynamics and reheating: Back reaction of parametric particle creation and curved spacetime effects,Phys. Rev. D56(1997) 678; ErratumPhys. Rev. D57 (1998) 3798, [hep-ph/9706207]
-
[48]
Besse,Einstein manifolds, inResults in Mathematics and Related Areas (3), Springer-Verlag, Berlin, (1987)
A.L. Besse,Einstein manifolds, inResults in Mathematics and Related Areas (3), Springer-Verlag, Berlin, (1987)
1987
- [49]
-
[50]
Thermodynamics of Spacetime: The Einstein Equation of State
T. Jacobson,Thermodynamics of Spacetime: The Einstein Equation of State,Phys. Rev. Lett.75 (1995) 1260, [arXiv:gr-qc/9504004]
work page Pith review arXiv 1995
-
[51]
DESI Collaboration,DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints,Phys. Rev. D112(2025) 083515, [arXiv:2503.14738]
work page Pith review arXiv 2025
-
[52]
The Pantheon+ Analysis: Cosmological Constraints
D. Brout, D. Scolnic, B. Popovic, A.G. Riess, J. Zuntz, R. Kessler, A. Carr, T.M. Davis,et al.,The Pantheon+ Analysis: Cosmological Constraints,ApJ.938(2022) 110, [arXiv:2202.04077]
work page internal anchor Pith review arXiv 2022
-
[53]
H0DN Collaboration,The Local Distance Network: a community consensus report on the measurement of the Hubble constant at 1% precision, Accepted byA.& A.(2025) , [arXiv:2510.23823]
work page internal anchor Pith review Pith/arXiv arXiv 2025
-
[54]
W. Giar` e, T. Mahassen, E. Di Valentino, S. Pan,An overview of what current data can (and cannot yet) say about evolving dark energy,Phys. Dark Univ.48(2025) 101906, [arXiv:2502.10264]
-
[55]
Lemaˆ ıtre,Un Univers homog` ene de masse constante et de rayon croissant rendant compte de la vitesse radiale des n´ ebuleuses extra-galactiques,Ann
G. Lemaˆ ıtre,Un Univers homog` ene de masse constante et de rayon croissant rendant compte de la vitesse radiale des n´ ebuleuses extra-galactiques,Ann. Soc. Sci. Brux.A47(1927) 49; Republication:A homogeneous universe of constant mass and increasing radius accounting for the radial velocity of extra-galactic nebulae,Gen. Rel. Grav45(2013) 1635
1927
-
[56]
C. Beny, Ch.T. Chubb, T. Farrelly, T.J. Osborne,Energy cost of entanglement extraction in complex quantum systems,Nature Commun.9(2018) 3792, [arXiv:1711.06658]
-
[57]
J.M.R. Parrondo,Thermodynamics of Information, in the Encyclopedia of Condensed Matter Physics - 2nd Edition, [arXiv:2306.12447]
-
[58]
Mandelstam, I
L. Mandelstam, I. Tamm,The Uncertainty Relation Between Energy and Time in Non-relativistic Quantum Mechanics,J. Phys. (USSR)9(1945) 249
1945
-
[59]
S. Deffner, S. Campbell,Quantum speed limits: from Heisenberg’s uncertainty principle to optimal quantum control,J. Phys. A: Math. Theor.50(2017) 453001, [arXiv:1705.08023]
-
[61]
Glauber,Coherent and incoherent states of the radiationfield,Phys
R.J. Glauber,Coherent and incoherent states of the radiationfield,Phys. Rev.131(1963) 2766
1963
-
[62]
Ziaeepour,Cosmological Condensation of scalar fields,Phys
H. Ziaeepour,Cosmological Condensation of scalar fields,Phys. Rev. D81(2010) 103526, [arXiv:1003.2996]
-
[63]
Hoppe,Quantum Theory of a Massless Relativistic Surface and a Two-dimensional Bound State Problem, Ph.D
J. Hoppe,Quantum Theory of a Massless Relativistic Surface and a Two-dimensional Bound State Problem, Ph.D. Thesis, MIT, Cambridge, MA, USA, (1982)
1982
-
[64]
Floratos, I Iliopoulos,A Note on the Classical Symmetries of the Closed Bosonic Membranes, Phys
E.G. Floratos, I Iliopoulos,A Note on the Classical Symmetries of the Closed Bosonic Membranes, Phys. Lett. B201(1988) 237
1988
-
[65]
Antoniadis, P
I. Antoniadis, P. Ditsas, E.F. Floratos, J. Iliopoulos,New Realizations of the Virasoro Algebra as Membrane Symmetries,Nucl. Phys. B300(1988) 549
1988
-
[66]
Arakelyan, G.K
T.A. Arakelyan, G.K. Savvidy,Cocycles of area-preserving diffeomorphisms and anomalies in the theory of relativistic surfaces,Phys. Lett. B214(1988) 350. – 28 –
1988
-
[67]
Pairlie, P
D.B. Pairlie, P. Fletcher, C.K. Zachos,Trigonometric Structure Constants for New Infinite-Dimensional Algebras,Phys. Lett. B218(1989) 203
1989
-
[68]
Pairlie, C.K
D.B. Pairlie, C.K. Zachos,Infinite-dimensional algebras, sine brackets, andSU(∞),Phys. Lett. B224 (1989) 101
1989
-
[69]
Hoppe,Diffeomorphism Groups, Quantization, andSU(∞),Int
J. Hoppe,Diffeomorphism Groups, Quantization, andSU(∞),Int. J. Mod. Phys. A4(1989) 5235
1989
-
[70]
Pope, K.S
C.N. Pope, K.S. Stelle,SU(∞)andSU +(∞)and area-preserving algebras,Phys. Lett. B226(1989) 257
1989
-
[72]
Savvidy,Symplectic Large N Gauge Theories, Proceedings of Cargese Summer School: Vacuum Structure in Intense Fields, P.415, (1991)
G.K. Savvidy,Symplectic Large N Gauge Theories, Proceedings of Cargese Summer School: Vacuum Structure in Intense Fields, P.415, (1991)
1991
-
[73]
Zunger,Why Matrix theory works for oddly shaped membranes,Phys
Y. Zunger,Why Matrix theory works for oddly shaped membranes,Phys. Rev. D64(2001) 086003, [arXiv:hep-th/0106030]
-
[74]
Connes.Gravity coupled with matter and the foundation of non-commutative geometry
A. Connes,Gravity coupled with matter and foundation of non-commutative geometry,Commun. Math. Phys.182(1996) 155, [arXiv:hep-th/9603053]
-
[75]
Hall,Quantum Theory for Mathematicians, Springer, (2013)
B.C. Hall,Quantum Theory for Mathematicians, Springer, (2013)
2013
-
[76]
A. Connes, M.R. Douglas, A. Schwarz,Noncommutative Geometry and Matrix Theory: Compactification on Tori,J. High Energy Phys.02(1998) 003, [arXiv:hep-th/9711162]
-
[77]
H. Ziaeepour,Comparing Quantum Gravity Models: String Theory, Loop Quantum Gravity, and Entanglement Gravity versusSU(∞)-QGR,Symmetry14(2022) 58, [arXiv:2109.05757]
-
[78]
P. Zanardi, D. Lidar, S. Lloyd,Quantum tensor product structures are observable-induced,Phys. Rev. Lett.92(2004) 060402, [arXiv:quant-ph/0308043]
- [79]
-
[80]
S. Moudgalya, O.I. Motrunich,Hilbert Space Fragmentation and Commutant Algebras,Phys. Rev. X12 (2022) 011050, [arXiv:2108.10324]
-
[81]
D. Kochergin, I.M. Khaymovich, O. Valba, A. Gorsky,Anatomy of the fragmented Hilbert space: eigenvalue tunneling, quantum scars and localization in the perturbed random regular graph, Phys. Rev. B108(2023) 094203, [arXiv:2305.14416]
-
[82]
A. Polkovnikov, K. Sengupta, A. Silva, M. Vengalattore,Nonequilibrium dynamics of closed interacting quantum systems,Rev. Mod. Phys.83(2011) 863, [arXiv:1007.5331]
discussion (0)
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