REVIEW 2 minor 2 cited by
Formation of shell-crossing singularities in effective gravitational collapse models with bounded and unbounded polymerizations
T0 review · 0 major / 2 minor · reviewed 2026-05-10 · grok-4.3
Pith's one-line read Polymerized collapse models with bounded functions form shell-crossing singularities for any inhomogeneous dust profile, while unbounded functions allow avoidance as in classical gravity.
desk verdict This paper finds that bounded polymerization in asymmetric bounce models makes shell-crossing singularities unavoidable for inhomogeneous dust, while unbounded polymerization in no-bounce models allows avoidance for decreasing profiles, like classical LTB. 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 polymerization functions appearing in the effective equations of motion for Lemaître-Tolman-Bondi dust collapse, distinguished by whether they remain bounded (producing a bounce) or are unbounded (producing no bounce).
What would settle it
A numerical solution of the effective evolution equations for a concrete inhomogeneous decreasing dust profile in the asymmetric bouncing model that evolves to a regular future without any shell-crossing singularity would falsify the unavoidability result.
Extended reading notes
Core claim
In the asymmetric bouncing model, which belongs to the class of bounded polymerization functions, shell-crossing singularities are unavoidable for inhomogeneous dust profiles. In contrast, for models without a bounce and with unbounded polymerization functions, no shell-crossing singularities form for inhomogeneous, decreasing dust profiles — a situation that resembles classical theory, in which shell-crossing singularities can also be avoided by a suitable choice of initial data.
Load-bearing premise
The effective LTB models with the chosen bounded and unbounded polymerization functions faithfully capture the relevant quantum gravity corrections without additional higher-order terms or backreaction effects that could alter the singularity formation outcome.
Editorial extensions
If this is right
- Shell-crossing singularities become unavoidable in any bounded-polymerization bouncing model of inhomogeneous dust collapse.
- Unbounded polymerization models recover the classical possibility of avoiding shell-crossing singularities by choosing suitable decreasing initial profiles.
- The presence or absence of a bounce in the effective dynamics controls whether singularities of this type can be evaded through initial-data choices.
- The conclusions for the asymmetric bounce extend earlier findings obtained for symmetric bouncing models to a broader class of bounded polymerization functions.
Reading between the lines
- Similar unavoidability may appear in other effective models whose quantum corrections introduce bounded modifications to the gravitational dynamics.
- Resolving the central singularity via a bounce may therefore shift rather than eliminate singular behavior in the inhomogeneous case.
- Direct numerical integration of the full set of effective equations for chosen initial data offers a concrete way to test the analytic claims about profile evolution.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The manuscript extends prior work on shell-crossing singularities (SCS) in effective polymerized Lemaître-Tolman-Bondi (LTB) dust collapse to an LQG-inspired asymmetric bouncing model (bounded polymerization functions) and to Bardeen/Hayward-inspired models (unbounded polymerization functions, no bounce). It reports that SCS remain unavoidable for inhomogeneous dust profiles in the asymmetric bouncing case, while in the unbounded no-bounce models SCS are avoided for inhomogeneous decreasing dust profiles, reproducing the classical LTB behavior in which suitable initial data can prevent SCS.
Significance. If the reported outcomes hold under the chosen effective equations, the work isolates the role of bounded versus unbounded polymerization in determining whether quantum corrections force SCS or permit classical-like avoidance in inhomogeneous collapse. This distinction supplies a concrete diagnostic for selecting effective models in quantum-corrected gravitational dynamics and clarifies the conditions under which bounce-inducing corrections generically produce singularities that classical theory can evade.
minor comments (2)
- Abstract: the specific functional forms of the bounded and unbounded polymerization functions (and the precise LTB metric ansatz) are not stated; a one-sentence definition or reference to the defining equations would allow readers to reproduce the setup without consulting prior papers.
- The manuscript should include a brief statement of the numerical integration scheme, convergence tests, and error tolerances used to track the shell-crossing condition, as these details are essential for assessing the robustness of the reported avoidance or unavoidability of SCS.
Simulated Author's Rebuttal
We thank the referee for their careful reading of the manuscript and for the positive assessment of its significance. The referee's summary accurately reflects our main findings on the distinction between bounded polymerization in the asymmetric bouncing model (where SCS remain unavoidable) and unbounded polymerization in the non-bouncing models (where SCS can be avoided for suitable decreasing initial profiles). We are pleased that the work is viewed as providing a diagnostic for effective models in quantum-corrected gravity.
Circularity Check
No significant circularity; results are direct model comparisons
full rationale
The paper compares shell-crossing singularity formation across specific effective LTB models: the asymmetric bouncing model (bounded polymerization) versus Bardeen/Hayward models (unbounded polymerization, no bounce). Claims are that SCS are unavoidable for inhomogeneous dust in the bounded bounce case but avoidable for decreasing profiles in the unbounded case, resembling classical LTB. No self-definitional reductions, fitted inputs renamed as predictions, or load-bearing self-citations appear in the derivation chain. The analysis proceeds from the chosen effective equations to numerical/analytical outcomes without circular equivalence to inputs. The noted weakest assumption is a generic limitation of effective models rather than an internal circularity.
Assumptions & free parameters
Cite this review
Pith. "Pith review of Formation of shell-crossing singularities in effective gravitational collapse models with bounded and unbounded polymerizations." pith.science (2026). https://pith.science/paper/2604.13716
@misc{pith2026260413716,
author = {Pith},
title = {Pith review of: Formation of shell-crossing singularities in effective gravitational collapse models with bounded and unbounded polymerizations},
year = {2026},
howpublished = {\url{https://pith.science/paper/2604.13716}},
note = {Machine review of arXiv:2604.13716}
}
read the original abstract
We extend the investigation into the formation of shell-crossing singularites (SCS) in effective polymerized LTB models to the LQG-inspired asymmetric bounce model, as well as to effective LTB models based on the solutions of Bardeen and Hayward, in which no bounce occurs. While the asymmetric bouncing model belongs to the class of bounded polymerization functions, the latter models feature unbounded polymerization functions. Our results show that, similar to the symmetric bouncing model, for the asymmetric bouncing model SCS are unavoidable for inhomogeneous dust profiles. In contrast, for models without a bounce and with unbounded polymerization functions, no SCS form for inhomogeneous, decreasing dust profiles -- a situation that resembles classical theory, in which SCS can also be avoided by a suitable choice of initial data.
Figures
Forward citations
Cited by 2 Pith papers
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Reference graph
Works this paper leans on
-
[1]
We introduce the areal radius of the dust shellR=R(t, x) = √ Ex and using Einstein’s field equations it follows thatRsatisfies the following evolution equation ˙R2 =E(x) + 2GM(x) R ,(II.3) whereGis the gravitational constant andM(x) the Misner-Sharp mass measuring the total grav- itational mass confined inside a shell. From the form of the evolution equat...
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[2]
Initial decreasing profiles As indicated in the previous section, for initial decreasing profiles SCS can arise only in the post- bounce phase. Sincef(η −) is a local minimum for the entire function, but a global minimum in the 9 restricted domain 2α∆γ2/3< η < η B (see Fig. 2), this means that a SCS forms after the bounce if M(x)s ′(x) M ′(x) ≥ γ(Γ2 − + 1...
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[3]
In particular, we focus on the region where∂ xρ0 >0
Initial increasing profiles As a second case we consider initial profiles with a global maximum at somex >0. In particular, we focus on the region where∂ xρ0 >0. As discussed previously, the condition for the formation of SCS in (III.3) can be fulfilled only in the pre-bounce phase, and sincef(η +) is a global maximum in the restricted temporal domainη > ...
-
[4]
B. P. Abbott et al. Observation of Gravitational Waves from a Binary Black Hole Merger.Phys. Rev. Lett., 116(6):061102, 2016. doi:10.1103/PhysRevLett.116.061102
-
[5]
B. Louise Webster and Paul Murdin. Cygnus X-1-a Spectroscopic Binary with a Heavy Companion ? Nature (London), 235(5332):37–38, January 1972. doi:10.1038/235037a0
-
[6]
A. M. Ghez et al. Measuring Distance and Properties of the Milky Way’s Central Supermassive Black Hole with Stellar Orbits.Astrophys. J., 689:1044–1062, 2008. doi:10.1086/592738
-
[7]
First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole,
Kazunori Akiyama et al. First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole.Astrophys. J. Lett., 875:L1, 2019. doi:10.3847/2041-8213/ab0ec7
-
[8]
J. R. Oppenheimer and H. Snyder. On Continued gravitational contraction.Phys. Rev., 56:455–459,
Show all 93 references
-
[9]
doi:10.1103/PhysRev.56.455
-
[10]
Lemaitre
G. Lemaitre. The expanding universe.Annales Soc. Sci. Bruxelles A, 53:51–85, 1933. doi: 10.1023/A:1018855621348
1933 doi
-
[11]
Richard C. Tolman. Effect of imhomogeneity on cosmological models.Proc. Nat. Acad. Sci., 20: 169–176, 1934. doi:10.1073/pnas.20.3.169
1934 doi
-
[12]
H. Bondi. Spherically symmetrical models in general relativity.Mon. Not. Roy. Astron. Soc., 107: 410–425, 1947. doi:10.1093/mnras/107.5-6.410
1947 doi
-
[13]
Gravitational collapse and space-time singularities.Phys
Roger Penrose. Gravitational collapse and space-time singularities.Phys. Rev. Lett., 14:57–59, 1965. doi:10.1103/PhysRevLett.14.57
1965 doi
-
[14]
Joshi, Dipanjan Dey, Pankaj S
Ashok B. Joshi, Dipanjan Dey, Pankaj S. Joshi, and Vivekkumar R. Tank. Tidal forces in collapsing compact objects.Phys. Rev. D, 110(12):124066, 2024. doi:10.1103/PhysRevD.110.124066
2024 doi
-
[15]
What is a shell crossing singularity?J
Peter Szekeres and Anthony Lun. What is a shell crossing singularity?J. Austral. Math. Soc. B, 41: 167–179, 1999. doi:10.1017/S0334270000011140
1999 doi
-
[16]
M¨ uller zum Hagen, P
H. M¨ uller zum Hagen, P. Yodzis, and H.J. Seifert. On the occurrence of naked singularities in general relativity. II.Commun. Math. Phys., 37:29–40, 1974. doi:10.1007/BF01646032. 13
1974 doi
-
[17]
Hellaby and K
C. Hellaby and K. Lake. Shell crossings and the Tolman model.Astrophys. J., 290:381, 1985. doi: 10.1086/162995
1985 doi
-
[18]
Brien C. Nolan. Dynamical extensions for shell crossing singularities.Class. Quant. Grav., 20:575–586,
-
[19]
doi:10.1088/0264-9381/20/4/302
-
[20]
Shock waves in classical dust collapse.Phys
Viqar Husain and Hassan Mehmood. Shock waves in classical dust collapse.Phys. Rev. Res., 7(3): 033215, 2025. doi:10.1103/b317-86qs
2025 doi
-
[21]
Expansion of a thin shell around a void in expanding universe
Kei-ichi Maeda and Humitaka Sato. Expansion of a thin shell around a void in expanding universe. Progress of Theoretical Physics, 70(3):772–782, 1983. doi:10.1143/PTP.70.772
1983 doi
-
[22]
Weak solutions in Einstein theory and beyond.Phys
Francesco Fazzini and Hassan Mehmood. Weak solutions in Einstein theory and beyond.Phys. Rev. D, 112(6):064064, 2025. doi:10.1103/6mrq-f9qc
2025 doi
-
[23]
Quantum Oppenheimer-Snyder and Swiss Cheese Models.Phys
Jerzy Lewandowski, Yongge Ma, Jinsong Yang, and Cong Zhang. Quantum Oppenheimer-Snyder and Swiss Cheese Models.Phys. Rev. Lett., 130(10):101501, 2023. doi:10.1103/PhysRevLett.130.101501
2023 doi
-
[24]
Fate of quantum black holes.Phys
Viqar Husain, Jarod George Kelly, Robert Santacruz, and Edward Wilson-Ewing. Fate of quantum black holes.Phys. Rev. D, 106(2):024014, 2022. doi:10.1103/PhysRevD.106.024014
2022 doi
-
[25]
Rainbow Oppenheimer-Snyder collapse and the entanglement entropy production.Phys
Micha l Bobula and Tomasz Paw lowski. Rainbow Oppenheimer-Snyder collapse and the entanglement entropy production.Phys. Rev. D, 108(2):026016, 2023. doi:10.1103/PhysRevD.108.026016
2023 doi
-
[26]
Nonsingular collapse of a spherical dust cloud.Phys
Asier Alonso-Bardaji and David Brizuela. Nonsingular collapse of a spherical dust cloud.Phys. Rev. D, 109(6):064023, 2024. doi:10.1103/PhysRevD.109.064023
2024 doi
-
[27]
Duque, and Dennis Hartmann
Martin Bojowald, Erick I. Duque, and Dennis Hartmann. Covariant Lemaˆ ıtre-Tolman-Bondi collapse in models of loop quantum gravity.Phys. Rev. D, 111(6):064002, 2025. doi:10.1103/PhysRevD.111.064002
2025 doi
-
[28]
Geometry of the black-to-white hole transition within a single asymptotic region.Phys
Muxin Han, Carlo Rovelli, and Farshid Soltani. Geometry of the black-to-white hole transition within a single asymptotic region.Phys. Rev. D, 107(6):064011, 2023. doi:10.1103/PhysRevD.107.064011
2023 doi
-
[29]
Status of Birkhoff’s theorem in the polymerized semiclassical regime of loop quantum gravity.Phys
Luca Cafaro and Jerzy Lewandowski. Status of Birkhoff’s theorem in the polymerized semiclassical regime of loop quantum gravity.Phys. Rev. D, 110(2):024072, 2024. doi:10.1103/PhysRevD.110.024072
2024 doi
-
[30]
Quantum induced shock dynamics in gravitational collapse: insights from effective models and numerical frameworks
Hongguang Liu and Dongxue Qu. Quantum induced shock dynamics in gravitational collapse: insights from effective models and numerical frameworks. 4 2025
2025
-
[31]
Quantum geometry and the Schwarzschild singularity.Class
Abhay Ashtekar and Martin Bojowald. Quantum geometry and the Schwarzschild singularity.Class. Quant. Grav., 23:391–411, 2006. doi:10.1088/0264-9381/23/2/008
2006 doi
-
[32]
Loop quantum black hole.Class
Leonardo Modesto. Loop quantum black hole.Class. Quant. Grav., 23:5587–5602, 2006. doi: 10.1088/0264-9381/23/18/006
2006 doi
-
[33]
Boehmer and Kevin Vandersloot
Christian G. Boehmer and Kevin Vandersloot. Loop Quantum Dynamics of the Schwarzschild Interior. Phys. Rev. D, 76:104030, 2007. doi:10.1103/PhysRevD.76.104030
2007 doi
-
[34]
Loop quantization of spherically symmetric midisuperspaces and loop quantum geometry of the maximally extended Schwarzschild spacetime
Dah-Wei Chiou, Wei-Tou Ni, and Alf Tang. Loop quantization of spherically symmetric midisuperspaces and loop quantum geometry of the maximally extended Schwarzschild spacetime. 12 2012
2012
-
[35]
Quantum black holes in Loop Quantum Gravity
Rodolfo Gambini, Javier Olmedo, and Jorge Pullin. Quantum black holes in Loop Quantum Gravity. Class. Quant. Grav., 31:095009, 2014. doi:10.1088/0264-9381/31/9/095009
2014 doi
-
[36]
Spherically symmetric canonical quantum gravity.Phys
Suddhasattwa Brahma. Spherically symmetric canonical quantum gravity.Phys. Rev. D, 91(12):124003,
-
[37]
doi:10.1103/PhysRevD.91.124003
-
[38]
Emergence of the product of constant curvature spaces in loop quantum cosmology.Class
Naresh Dadhich, Anton Joe, and Parampreet Singh. Emergence of the product of constant curvature spaces in loop quantum cosmology.Class. Quant. Grav., 32(18):185006, 2015. doi:10.1088/0264- 9381/32/18/185006
2015 doi
-
[39]
Inhomogeneities, loop quantum gravity corrections, constraint algebra and general covariance.Class
Rakesh Tibrewala. Inhomogeneities, loop quantum gravity corrections, constraint algebra and general covariance.Class. Quant. Grav., 31:055010, 2014. doi:10.1088/0264-9381/31/5/055010
2014 doi
-
[40]
Non-singular black holes and the Limiting Curvature Mechanism: A Hamiltonian perspective.JCAP, 05:072, 2018
Jibril Ben Achour, Frederic Lamy, Hongguang Liu, and Karim Noui. Non-singular black holes and the Limiting Curvature Mechanism: A Hamiltonian perspective.JCAP, 05:072, 2018. doi:10.1088/1475- 7516/2018/05/072
2018 doi
-
[41]
Von-Neumann Stability and Singularity Res- olution in Loop Quantized Schwarzschild Black Hole.Class
Alec Yonika, Gaurav Khanna, and Parampreet Singh. Von-Neumann Stability and Singularity Res- olution in Loop Quantized Schwarzschild Black Hole.Class. Quant. Grav., 35(4):045007, 2018. doi: 10.1088/1361-6382/aaa18d
2018 doi
-
[42]
End of a black hole’s evaporation.Phys
Fabio D’Ambrosio, Marios Christodoulou, Pierre Martin-Dussaud, Carlo Rovelli, and Farshid Soltani. End of a black hole’s evaporation.Phys. Rev. D, 103(10):106014, 2021. doi: 10.1103/PhysRevD.103.106014
2021 doi
-
[43]
From black holes to white holes: a quantum gravi- tational, symmetric bounce.Class
Javier Olmedo, Sahil Saini, and Parampreet Singh. From black holes to white holes: a quantum gravi- tational, symmetric bounce.Class. Quant. Grav., 34(22):225011, 2017. doi:10.1088/1361-6382/aa8da8
2017 doi
-
[44]
Quantum Transfiguration of Kruskal Black 14 Holes.Phys
Abhay Ashtekar, Javier Olmedo, and Parampreet Singh. Quantum Transfiguration of Kruskal Black 14 Holes.Phys. Rev. Lett., 121(24):241301, 2018. doi:10.1103/PhysRevLett.121.241301
2018 doi
-
[45]
Quantum extension of the Kruskal spacetime
Abhay Ashtekar, Javier Olmedo, and Parampreet Singh. Quantum extension of the Kruskal spacetime. Phys. Rev. D, 98(12):126003, 2018. doi:10.1103/PhysRevD.98.126003
2018 doi
-
[46]
Effective line elements and black-hole models in canonical loop quantum gravity.Phys
Martin Bojowald, Suddhasattwa Brahma, and Dong-han Yeom. Effective line elements and black-hole models in canonical loop quantum gravity.Phys. Rev. D, 98(4):046015, 2018. doi: 10.1103/PhysRevD.98.046015
2018 doi
-
[47]
Polymer Schwarzschild black hole: An effective metric.EPL, 123(2):20006, 2018
Jibril Ben Achour, Fr´ ed´ eric Lamy, Hongguang Liu, and Karim Noui. Polymer Schwarzschild black hole: An effective metric.EPL, 123(2):20006, 2018. doi:10.1209/0295-5075/123/20006
2018 doi
-
[48]
Mele, and Johannes M¨ unch
Norbert Bodendorfer, Fabio M. Mele, and Johannes M¨ unch. Effective Quantum Extended Spacetime of Polymer Schwarzschild Black Hole.Class. Quant. Grav., 36(19):195015, 2019. doi:10.1088/1361- 6382/ab3f16
2019 doi
-
[49]
Quantum gravity predictions for black hole interior geometry.Phys
Emanuele Alesci, Sina Bahrami, and Daniele Pranzetti. Quantum gravity predictions for black hole interior geometry.Phys. Lett. B, 797:134908, 2019. doi:10.1016/j.physletb.2019.134908
2019 doi
-
[50]
Perspectives on the dynamics in a loop quan- tum gravity effective description of black hole interiors.Phys
Mehdi Assanioussi, Andrea Dapor, and Klaus Liegener. Perspectives on the dynamics in a loop quan- tum gravity effective description of black hole interiors.Phys. Rev. D, 101(2):026002, 2020. doi: 10.1103/PhysRevD.101.026002
2020 doi
-
[51]
Critical collapse of a scalar field in semiclassical loop quantum gravity.Phys
Florencia Benitez, Rodolfo Gambini, Luis Lehner, Steve Liebling, and Jorge Pullin. Critical collapse of a scalar field in semiclassical loop quantum gravity.Phys. Rev. Lett., 124(7):071301, 2020. doi: 10.1103/PhysRevLett.124.071301
2020 doi
-
[52]
Santos, Fu-Wen Shu, and Anzhong Wang
Wen-Cong Gan, Nilton O. Santos, Fu-Wen Shu, and Anzhong Wang. Properties of the spherically symmetric polymer black holes.Phys. Rev. D, 102:124030, 2020. doi:10.1103/PhysRevD.102.124030
2020 doi
-
[53]
Loop Quantum Black Hole Extensions Within the Improved Dynamics.Front
Rodolfo Gambini, Javier Olmedo, and Jorge Pullin. Loop Quantum Black Hole Extensions Within the Improved Dynamics.Front. Astron. Space Sci., 8:74, 2021. doi:10.3389/fspas.2021.647241
2021 doi
-
[54]
Quantum Grav- ity of Dust Collapse: Shock Waves from Black Holes.Phys
Viqar Husain, Jarod George Kelly, Robert Santacruz, and Edward Wilson-Ewing. Quantum Grav- ity of Dust Collapse: Shock Waves from Black Holes.Phys. Rev. Lett., 128(12):121301, 2022. doi: 10.1103/PhysRevLett.128.121301
2022 doi
-
[55]
Does the Loop Quantumµ o Scheme Permit Black Hole Formation? Universe, 7(11):406, 2021
Bao-Fei Li and Parampreet Singh. Does the Loop Quantumµ o Scheme Permit Black Hole Formation? Universe, 7(11):406, 2021. doi:10.3390/universe7110406
2021 doi
-
[56]
Under- standing quantum black holes from quantum reduced loop gravity.Phys
Wen-Cong Gan, Geeth Ongole, Emanuele Alesci, Yang An, Fu-Wen Shu, and Anzhong Wang. Under- standing quantum black holes from quantum reduced loop gravity.Phys. Rev. D, 106(12):126013, 2022. doi:10.1103/PhysRevD.106.126013
2022 doi
-
[57]
Effective loop quantum gravity framework for vacuum spherically symmetric spacetimes.Phys
Jarod George Kelly, Robert Santacruz, and Edward Wilson-Ewing. Effective loop quantum gravity framework for vacuum spherically symmetric spacetimes.Phys. Rev. D, 102(10):106024, 2020. doi: 10.1103/PhysRevD.102.106024
2020 doi
-
[58]
Gambini, J
R. Gambini, J. Olmedo, and J. Pullin. Spherically symmetric loop quantum gravity: analysis of improved dynamics.Class. Quant. Grav., 37(20):205012, 2020. doi:10.1088/1361-6382/aba842
2020 doi
-
[59]
Improved effective dynamics of loop-quantum-gravity black hole and Nariai limit.Class
Muxin Han and Hongguang Liu. Improved effective dynamics of loop-quantum-gravity black hole and Nariai limit.Class. Quant. Grav., 39(3):035011, 2022. doi:10.1088/1361-6382/ac44a0
2022 doi
-
[60]
Reduced phase space quantization of black holes: Path integrals and effective dynamics
Cong Zhang. Reduced phase space quantization of black holes: Path integrals and effective dynamics. Phys. Rev. D, 104(12):126003, 2021. doi:10.1103/PhysRevD.104.126003
2021 doi
-
[61]
Generic features of a polymer quantum black hole.Class
Johannes M¨ unch, Alejandro Perez, Simone Speziale, and Sami Viollet. Generic features of a polymer quantum black hole.Class. Quant. Grav., 40(13):135003, 2023. doi:10.1088/1361-6382/accccd
2023 doi
-
[62]
Nonsingular quantum gravitational dynamics of an Lemaˆ ıtre-Tolman-Bondi dust shell model: The role of quantization prescriptions.Phys
Kristina Giesel, Bao-Fei Li, and Parampreet Singh. Nonsingular quantum gravitational dynamics of an Lemaˆ ıtre-Tolman-Bondi dust shell model: The role of quantization prescriptions.Phys. Rev. D, 104 (10):106017, 2021. doi:10.1103/PhysRevD.104.106017
2021 doi
-
[63]
Spherical symmetric gravitational collapse of a dust cloud: Polymerized dynamics in reduced phase space.Phys
Kristina Giesel, Muxin Han, Bao-Fei Li, Hongguang Liu, and Parampreet Singh. Spherical symmetric gravitational collapse of a dust cloud: Polymerized dynamics in reduced phase space.Phys. Rev. D, 107(4):044047, 2023. doi:10.1103/PhysRevD.107.044047
2023 doi
-
[64]
Covariantµ¯-scheme effective dynamics, mimetic gravity, and non- singular black holes: Applications to spherically symmetric quantum gravity.Phys
Muxin Han and Hongguang Liu. Covariantµ¯-scheme effective dynamics, mimetic gravity, and non- singular black holes: Applications to spherically symmetric quantum gravity.Phys. Rev. D, 109(8): 084033, 2024. doi:10.1103/PhysRevD.109.084033
2024 doi
-
[65]
Embedding generalized Lemaˆ ıtre-Tolman-Bondi models in polymerized spherically symmetric spacetimes.Phys
Kristina Giesel, Hongguang Liu, Eric Rullit, Parampreet Singh, and Stefan Andreas Weigl. Embedding generalized Lemaˆ ıtre-Tolman-Bondi models in polymerized spherically symmetric spacetimes.Phys. Rev. D, 110(10):104017, 2024. doi:10.1103/PhysRevD.110.104017
2024 doi
-
[66]
Regular black holes 15 and their relationship to polymerized models and mimetic gravity.Phys
Kristina Giesel, Hongguang Liu, Parampreet Singh, and Stefan Andreas Weigl. Regular black holes 15 and their relationship to polymerized models and mimetic gravity.Phys. Rev. D, 111(6):064064, 2025. doi:10.1103/PhysRevD.111.064064
2025 doi
-
[67]
Corrections to the Friedmann Equations from LQG for a Universe with a Free Scalar Field.Phys
Victor Taveras. Corrections to the Friedmann Equations from LQG for a Universe with a Free Scalar Field.Phys. Rev. D, 78:064072, 2008. doi:10.1103/PhysRevD.78.064072
2008 doi
-
[68]
Giesel and T
K. Giesel and T. Thiemann. Algebraic quantum gravity (AQG). IV. Reduced phase space quantisation of loop quantum gravity.Class. Quant. Grav., 27:175009, 2010. doi:10.1088/0264-9381/27/17/175009
2010 doi
-
[69]
Cosmological Effective Hamiltonian from full Loop Quantum Gravity Dynamics.Phys
Andrea Dapor and Klaus Liegener. Cosmological Effective Hamiltonian from full Loop Quantum Gravity Dynamics.Phys. Lett. B, 785:506–510, 2018. doi:10.1016/j.physletb.2018.09.005
2018 doi
-
[70]
Investigation of the gravitational dust collapse of the LQG-inspired effective asymmetric bounce model
Kristina Giesel, Hongguang Liu, and Eric Rullit. Investigation of the gravitational dust collapse of the LQG-inspired effective asymmetric bounce model. 2 2026
2026
-
[71]
Nonsingular general relativistic gravitational collapse
James Bardeen. Nonsingular general relativistic gravitational collapse
-
[72]
Sean A. Hayward. Formation and evaporation of regular black holes.Phys. Rev. Lett., 96:031103, 2006. doi:10.1103/PhysRevLett.96.031103
2006 doi
-
[73]
Shell-crossings and shock formation during gravitational collapse in effective loop quantum gravity.Phys
Francesco Fazzini, Viqar Husain, and Edward Wilson-Ewing. Shell-crossings and shock formation during gravitational collapse in effective loop quantum gravity.Phys. Rev. D, 109(8):084052, 2024. doi:10.1103/PhysRevD.109.084052
2024 doi
-
[74]
Generalized analysis of a dust collapse in effective loop quantum gravity: Fate of shocks and covariance.Phys
Kristina Giesel, Hongguang Liu, Parampreet Singh, and Stefan Andreas Weigl. Generalized analysis of a dust collapse in effective loop quantum gravity: Fate of shocks and covariance.Phys. Rev. D, 110 (10):104016, 2024. doi:10.1103/PhysRevD.110.104016
2024 doi
-
[75]
Lemaitre-Tolman-Bondi collapse from the perspective of loop quantum gravity.Phys
Martin Bojowald, Tomohiro Harada, and Rakesh Tibrewala. Lemaitre-Tolman-Bondi collapse from the perspective of loop quantum gravity.Phys. Rev. D, 78:064057, 2008. doi:10.1103/PhysRevD.78.064057
2008 doi
-
[76]
Reyes, and Rakesh Tibrewala
Martin Bojowald, Juan D. Reyes, and Rakesh Tibrewala. Non-marginal LTB-like models with inverse triad corrections from loop quantum gravity.Phys. Rev. D, 80:084002, 2009. doi: 10.1103/PhysRevD.80.084002
2009 doi
-
[77]
An effective model for the quantum Schwarzschild black hole.Phys
Asier Alonso-Bardaji, David Brizuela, and Ra¨ ul Vera. An effective model for the quantum Schwarzschild black hole.Phys. Lett. B, 829:137075, 2022. doi:10.1016/j.physletb.2022.137075
2022 doi
-
[78]
Discreteness of area and volume in quantum gravity.Nucl
Carlo Rovelli and Lee Smolin. Discreteness of area and volume in quantum gravity.Nucl. Phys. B, 442:593–622, 1995. doi:10.1016/0550-3213(95)00150-Q. [Erratum: Nucl.Phys.B 456, 753–754 (1995)]
1995 doi
-
[79]
Quantum theory of geometry
Abhay Ashtekar and Jerzy Lewandowski. Quantum theory of geometry. 1: Area operators.Class. Quant. Grav., 14:A55–A82, 1997. doi:10.1088/0264-9381/14/1A/006
1997 doi
-
[80]
Alternative quantization of the Hamiltonian in loop quantum cosmology II: Including the Lorentz term.Phys
Jinsong Yang, You Ding, and Yongge Ma. Alternative quantization of the Hamiltonian in loop quantum cosmology II: Including the Lorentz term.Phys. Lett. B, 682:1–7, 2009. doi: 10.1016/j.physletb.2009.10.072
2009 doi
-
[81]
Causal structure of nonhomogeneous dust collapse in effective loop quantum gravity.Phys
Micha l Bobula and Tomasz Paw lowski. Causal structure of nonhomogeneous dust collapse in effective loop quantum gravity.Phys. Rev. D, 112(6):064056, 2025. doi:10.1103/z5sz-mcl5
2025 doi
-
[82]
From Principles to Effective Models: A Constructive Framework for Effective Covariant Actions with a Unique Vacuum Solution
Kristina Giesel and Hongguang Liu. From Principles to Effective Models: A Constructive Framework for Effective Covariant Actions with a Unique Vacuum Solution. 12 2025
2025
-
[83]
Lasky, Anthony W
Paul D. Lasky, Anthony W. C. Lun, and Raymond B. Burston. Initial value formalism for dust collapse. 6 2006
2006
-
[84]
Gentle spaghettification in effective LQG dust collapse.Phys
Francesco Fazzini. Gentle spaghettification in effective LQG dust collapse.Phys. Rev. D, 112(2):026029,
-
[85]
doi:10.1103/f7q9-grqb
-
[86]
Non-uniqueness of shockwave evolution in a loop quantum gravity inspired model
Francesco Fazzini. Non-uniqueness of shockwave evolution in a loop quantum gravity inspired model. Phys. Scripta, 100(11):115220, 2025. doi:10.1088/1402-4896/ae1be4
2025 doi
-
[87]
Quantum gravitational stellar evolution beyond shell-crossing singularities
Micha l Bobula and Francesco Fazzini. Quantum gravitational stellar evolution beyond shell-crossing singularities. 1 2026
2026
-
[88]
Ashtekar, J
A. Ashtekar, J. Baez, A. Corichi, and Kirill Krasnov. Quantum geometry and black hole entropy.Phys. Rev. Lett., 80:904–907, 1998. doi:10.1103/PhysRevLett.80.904
1998 doi
-
[89]
Towards Cosmological Dynamics from Loop Quan- tum Gravity.Phys
Bao-Fei Li, Parampreet Singh, and Anzhong Wang. Towards Cosmological Dynamics from Loop Quan- tum Gravity.Phys. Rev. D, 97(8):084029, 2018. doi:10.1103/PhysRevD.97.084029
2018 doi
-
[90]
Emergent de Sitter Epoch of the Quantum Cosmos from Loop Quantum Cosmology.Phys
Mehdi Assanioussi, Andrea Dapor, Klaus Liegener, and Tomasz Paw lowski. Emergent de Sitter Epoch of the Quantum Cosmos from Loop Quantum Cosmology.Phys. Rev. Lett., 121(8):081303, 2018. doi: 10.1103/PhysRevLett.121.081303
2018 doi
-
[91]
Emergent de Sitter epoch of the Loop Quantum Cosmos: a detailed analysis.Phys
Mehdi Assanioussi, Andrea Dapor, Klaus Liegener, and Tomasz Paw lowski. Emergent de Sitter epoch of the Loop Quantum Cosmos: a detailed analysis.Phys. Rev. D, 100(8):084003, 2019. doi: 10.1103/PhysRevD.100.084003. 16
2019 doi
-
[92]
Investigation of the gravitational collapse of the LQG-inspired effective asymmetric bounce model
Kristina Giesel, Hongguang Liu, and Eric Rullit. Investigation of the gravitational collapse of the LQG-inspired effective asymmetric bounce model. to appear
-
[93]
Semiclassical cosmology with polymer matter.Class
Syed Moeez Hassan and Viqar Husain. Semiclassical cosmology with polymer matter.Class. Quant. Grav., 34(8):084003, 2017. doi:10.1088/1361-6382/aa6455
2017 doi
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