Recognition: unknown
Regular ultracompact objects with anti-de Sitter cores as polymerized vacuum solutions
Pith reviewed 2026-05-07 06:47 UTC · model grok-4.3
The pith
Polymerized vacuum solutions generate regular black holes with anti-de Sitter cores uniquely determined by mass.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
Regular black hole solutions and their horizonless counterparts achieve regularization via an anti-de Sitter core. These geometries emerge as polymerized vacuum solutions that admit a Birkhoff-type theorem and are uniquely determined by their mass. Using an auxiliary relational dust clock and the absence of gravitational waves in spherical symmetry, the structural ultralocality permits decomposition into independent shell degrees of freedom. The dust field acts as a reference clock for deparameterization and does not source the vacuum geometries. This tightly constrains the Lemaitre-Tolman-Bondi shell Hamiltonian to a factorized form and the static vacuum metric function to a universal form.
What carries the argument
The factorized Lemaitre-Tolman-Bondi shell Hamiltonian obtained after dust-clock deparameterization, which forces the static vacuum metric function into a universal expression independent of the shell details.
If this is right
- Every solution is fixed by the single mass parameter.
- The geometries obey a Birkhoff-type theorem in spherical symmetry.
- The presence of a bounce is encoded in the full dynamics but can be missed in finite-order truncations.
- A four-dimensional covariant completion of the Lagrangian belongs to generalized extended mimetic gravity models.
Where Pith is reading between the lines
- These universal metric functions could serve as concrete templates for the interior structure of compact objects that remain regular at small radii.
- Matching the derived metric to strong-field observations would directly constrain the allowed polymerization scale.
- Lifting the ultralocal decomposition to axisymmetric or rotating cases would test whether the same mass-only uniqueness persists.
- The embedding into mimetic gravity suggests these solutions can be studied within a wider family of modified gravity actions without new matter fields.
Load-bearing premise
The dust field functions purely as a non-sourcing reference clock for deparameterization, together with ultralocality that decouples the shell dynamics into independent degrees of freedom.
What would settle it
Explicit derivation of the physical Hamiltonian in the specific polymerization model, followed by direct comparison of the resulting static metric function against the claimed universal expression that produces an anti-de Sitter core.
Figures
read the original abstract
We present a systematic derivation of regular black hole solutions - and their horizonless counterparts - that achieve regularization via an anti-de Sitter core. These geometries emerge as polymerized vacuum solutions inspired by loop quantum gravity, constituting effective quantum gravity configurations that admit a Birkhoff-type theorem and are uniquely determined by their mass. Using an auxiliary relational dust clock, together with the absence of gravitational waves in spherical symmetry, we exploit the structural ultralocality of the system to decompose the dynamics into independent shell degrees of freedom. The dust field acts as a reference clock for deparameterization and does not source the vacuum geometries considered here. These assumptions tightly constrain the Lemaitre-Tolman-Bondi shell Hamiltonian to a factorized form and the static vacuum metric function to a universal expression. We examine the possibility of a bounce and analyze how its presence is encoded, or missed, in finite-order effective truncations of the full model. The procedure for deriving the explicit physical Hamiltonian is described for a generic case before specializing to a specific model of interest. Finally, we construct a four-dimensional covariant completion of the spatially covariant Lagrangian, showing that it belongs to the class of generalized extended mimetic gravity models.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper claims to systematically derive regular ultracompact objects (black holes and horizonless configurations) with anti-de Sitter cores as polymerized vacuum solutions in an effective loop quantum gravity framework. Using a relational dust clock for deparameterization, spherical symmetry, and ultralocality to decompose into independent LTB shells, the authors obtain a factorized shell Hamiltonian leading to a universal static metric function uniquely determined by mass, admitting a Birkhoff-type theorem. They analyze how bounces are encoded or missed in finite-order truncations and construct a 4D covariant completion belonging to generalized extended mimetic gravity.
Significance. If the central claims hold, this work offers a structured relational approach to generating regular geometries from polymerized Hamiltonians, with the dust deparameterization and mimetic gravity embedding providing a controlled way to obtain effective metrics without ad hoc matter sources. The truncation analysis serves as a useful caution for approximate effective models. Strengths include the explicit procedure for the physical Hamiltonian (generic to specific model) and the covariant completion, which could facilitate phenomenological applications in quantum gravity.
major comments (3)
- [Abstract and generic Hamiltonian procedure] Abstract and the section describing the generic-to-specific Hamiltonian derivation: the central uniqueness and vacuum claims require an explicit factorized LTB shell Hamiltonian and the universal metric expression. These are asserted but not displayed, preventing verification that the AdS core emerges without tuning and that the polymerization scale does not enter as an extra parameter in the final geometry.
- [Physical Hamiltonian extraction and vacuum metric function] The vacuum interpretation and mass-only uniqueness (abstract and physical Hamiltonian extraction): polymerization replaces connection components by holonomy functions (sin(μK)/μ), which generically induce non-zero effective stress-energy in the deparameterized equations. The manuscript must explicitly compute the effective T_μν for the claimed solutions and demonstrate it vanishes (or is absorbed consistently with vacuum), as this is load-bearing for the 'polymerized vacuum solutions' and Birkhoff-type theorem statements.
- [Static vacuum metric and Birkhoff-type theorem] Birkhoff-type theorem and uniqueness by mass: the derivation assumes ultralocality and dust as non-sourcing clock. The paper should provide the argument showing that the effective dynamics remain uniquely fixed by mass alone, without the polymerization scale acting as a free parameter, and clarify whether the theorem holds at the effective level or only classically.
minor comments (3)
- [Finite-order effective truncations] In the truncation analysis section, include at least one explicit analytic or numerical comparison between the full polymerized solution and its finite-order approximation to illustrate how the bounce is missed or encoded.
- [Covariant completion] The covariant completion in generalized extended mimetic gravity should display the explicit form of the 4D Lagrangian or action to allow direct comparison with existing mimetic models.
- [Introduction and model setup] Clarify early the notation for the polymerization scale μ and holonomy corrections to improve readability for readers unfamiliar with the specific LQG-inspired setup.
Simulated Author's Rebuttal
We thank the referee for their careful reading of the manuscript and for the constructive comments, which have helped us strengthen the presentation. We address each major point below and have revised the manuscript accordingly to improve clarity and rigor.
read point-by-point responses
-
Referee: [Abstract and generic Hamiltonian procedure] Abstract and the section describing the generic-to-specific Hamiltonian derivation: the central uniqueness and vacuum claims require an explicit factorized LTB shell Hamiltonian and the universal metric expression. These are asserted but not displayed, preventing verification that the AdS core emerges without tuning and that the polymerization scale does not enter as an extra parameter in the final geometry.
Authors: We agree that the explicit expressions should be displayed prominently to facilitate verification. In the revised manuscript we have added a dedicated subsection (in the generic Hamiltonian procedure) that writes out the factorized LTB shell Hamiltonian obtained after imposing ultralocality and dust deparameterization. The resulting static vacuum metric function is now stated explicitly as a universal expression depending only on the mass parameter M; the polymerization scale is absorbed into the definition of the effective mass and does not appear as an independent parameter. This form directly yields the AdS core without additional tuning, as required by the regularity condition at the center. revision: yes
-
Referee: [Physical Hamiltonian extraction and vacuum metric function] The vacuum interpretation and mass-only uniqueness (abstract and physical Hamiltonian extraction): polymerization replaces connection components by holonomy functions (sin(μK)/μ), which generically induce non-zero effective stress-energy in the deparameterized equations. The manuscript must explicitly compute the effective T_μν for the claimed solutions and demonstrate it vanishes (or is absorbed consistently with vacuum), as this is load-bearing for the 'polymerized vacuum solutions' and Birkhoff-type theorem statements.
Authors: We acknowledge that an explicit computation of the effective stress-energy tensor is necessary to substantiate the vacuum claim. In the revised version we have inserted the calculation of the effective T_μν obtained from the polymerized Hamiltonian after deparameterization. For the static solutions satisfying the factorized shell Hamiltonian, the effective stress-energy tensor vanishes identically; the holonomy corrections modify the geometry but do not source additional matter degrees of freedom once the dust clock is used as a non-dynamical reference. This confirms the vacuum interpretation at the effective level and supports the mass-only uniqueness. revision: yes
-
Referee: [Static vacuum metric and Birkhoff-type theorem] Birkhoff-type theorem and uniqueness by mass: the derivation assumes ultralocality and dust as non-sourcing clock. The paper should provide the argument showing that the effective dynamics remain uniquely fixed by mass alone, without the polymerization scale acting as a free parameter, and clarify whether the theorem holds at the effective level or only classically.
Authors: We thank the referee for requesting this clarification. The Birkhoff-type theorem is established at the effective level: ultralocality decomposes the system into independent LTB shells whose individual Hamiltonians, after dust deparameterization, depend only on the mass parameter. The polymerization scale does not enter as a free parameter because the holonomy corrections are constrained by the requirement that the static solution be regular and that the shell Hamiltonian remain factorized; any residual scale dependence is absorbed into the definition of M. We have expanded the relevant section with a step-by-step derivation showing how the effective dynamics are fixed solely by mass, thereby extending the classical Birkhoff theorem to the polymerized vacuum case. revision: yes
Circularity Check
No significant circularity; derivation follows from independent structural assumptions
full rationale
The paper's central claims rest on explicit, external assumptions (spherical symmetry, dust as non-sourcing relational clock, ultralocality permitting LTB shell factorization) that are stated upfront and are not derived from the final metric or AdS-core form. The Birkhoff-type uniqueness by mass is presented as a consequence of these constraints plus the polymerized vacuum equations, without reducing to a self-citation chain, fitted parameter renamed as prediction, or self-definitional loop. No equation is shown to equal its input by construction; the effective Hamiltonian derivation and covariant completion are constructed step-by-step from the stated premises. The polymerization scale and truncation analysis introduce model choices but do not create tautological equivalence. This is a standard non-circular effective-theory construction.
Axiom & Free-Parameter Ledger
free parameters (1)
- polymerization scale
axioms (3)
- standard math Absence of gravitational waves in spherical symmetry
- domain assumption Dust field acts as reference clock and does not source the vacuum geometries
- domain assumption Structural ultralocality of the system
invented entities (2)
-
polymerized vacuum solution
no independent evidence
-
anti-de Sitter core
no independent evidence
Reference graph
Works this paper leans on
-
[1]
In this regime, both the dS and AdS cores exhibit quali- tatively similar behavior. For an appropriate range of param- eters, the collapsing shell reaches an inner turning point at a finite radius and subsequently expands until it encounters an outer turning point, since its energy is insufficient to escape to infinity. The outer turning point corresponds...
-
[2]
S. W. Hawking and G. F. R. Ellis,The Large Scale Structure of Space-Time(Cambridge University Press, 1973)
1973
-
[3]
Penrose, Gravitational Collapse and Space-Time Singulari- ties, Phys
R. Penrose, Gravitational Collapse and Space-Time Singulari- ties, Phys. Rev. Lett.14, 57 (1965)
1965
-
[4]
Witten, Light rays, singularities, and all that, Rev
E. Witten, Light rays, singularities, and all that, Rev. Mod. Phys.92, 45004 (2020)
2020
-
[5]
S. M. Scott and B. E. Whale, The endpoint theorem, Classical Quantum Gravity38, 065012 (2021)
2021
-
[6]
S. M. Scott and B. E. Whale, What actually happens when you approach a gravitational singularity?, Int. J. Mod. Phys. D30, 2142007 (2021)
2021
-
[7]
J. M. Bardeen, Non-singular general relativistic gravitational collapse, in Proceedings of the International Conference GR5 (Tbilisi University Press, Tbilisi, 1968)
1968
-
[8]
S. A. Hayward, Formation and Evaporation of Nonsingular Black Holes, Phys. Rev. Lett.96, 031103 (2006)
2006
-
[9]
Dymnikova, Vacuum nonsingular black hole, Gen
I. Dymnikova, Vacuum nonsingular black hole, Gen. Relativ. Gravit.24, 235 (1992)
1992
-
[10]
J. P. S. Lemos and V . T. Zanchin, Regular black holes: Electri- cally charged solutions, Reissner-Nordstr¨om outside a de Sitter core, Phys. Rev. D83, 124005 (2011)
2011
-
[11]
Bambi and L
C. Bambi and L. Modesto, Rotating regular black holes, Phys. Lett. B721, 329 (2013)
2013
-
[12]
Simpson and M
A. Simpson and M. Visser, Black-bounce to traversable worm- hole, J. Cosmol. Astropart. Phys.02(2019) 042
2019
-
[13]
M. E. Rodrigues and M. V . de S. Silva, Bardeen regular black hole with an electric source, J. Cosmol. Astropart. Phys.06 (2018) 025
2018
-
[14]
Born, Modified Field Equations with a Finite Radius of the Electron, Nature132, 282 (1933)
M. Born, Modified Field Equations with a Finite Radius of the Electron, Nature132, 282 (1933)
1933
-
[15]
Born and L
M. Born and L. Infeld, Foundations of the new field theory, Proc. R. Soc. Lond. A144, 425 (1934)
1934
-
[16]
Born and L
M. Born and L. Infeld, On the quantization of the new field equations I, Proc. R. Soc. Lond. A147, 522 (1934)
1934
-
[17]
Pellicer and R
R. Pellicer and R. J. Torrence, Nonlinear Electrodynamics and General Relativity, J. Math. Phys.10, 1718 (1969)
1969
-
[18]
K. A. Bronnikov, V . N. Melnikov, G. N. Shikin, and K. P. Sta- niukovich, Scalar, electromagnetic, and gravitational fields in- teraction: Particlelike solutions, Ann. Phys.118, 84 (1979)
1979
-
[19]
Ay ´on-Beato and E
E. Ay ´on-Beato and E. Garc ´ıa, Regular Black Hole in General Relativity Coupled to Nonlinear Electrodynamics, Phys. Rev. Lett.80, 5056 (1998)
1998
-
[20]
Ay ´on-Beato and E
E. Ay ´on-Beato and E. Garc ´ıa, Non-Singular Charged Black Hole Solution for Non-Linear Source, Gen. Relativ. Gravit.31, 629 (1999)
1999
-
[21]
Ay ´on-Beato and E
E. Ay ´on-Beato and E. Garc´ıa, New regular black hole solution from nonlinear electrodynamics, Phys. Lett. B464, 25 (1999)
1999
-
[22]
Regular Black Hole in General Relativity Coupled to Nonlinear Electrodynamics
K. A. Bronnikov, Comment on “Regular Black Hole in General Relativity Coupled to Nonlinear Electrodynamics”, Phys. Rev. Lett.85, 4641 (2000)
2000
-
[23]
K. A. Bronnikov, Regular magnetic black holes and monopoles from nonlinear electrodynamics, Phys. Rev. D63, 044005 (2001)
2001
-
[24]
Burinskii and S
A. Burinskii and S. R. Hildebrandt, New type of regular black holes and particlelike solutions from nonlinear electrodynam- ics, Phys. Rev. D65, 104017 (2002)
2002
-
[25]
Dymnikova, Regular electrically charged vacuum structures with de Sitter centre in nonlinear electrodynamics coupled to general relativity, Class
I. Dymnikova, Regular electrically charged vacuum structures with de Sitter centre in nonlinear electrodynamics coupled to general relativity, Class. Quantum Gravity21, 4417 (2004)
2004
-
[26]
Balart and E
L. Balart and E. C. Vagenas, Regular black holes with a nonlin- ear electrodynamics source, Phys. Rev. D90, 124045 (2014)
2014
-
[27]
Fan and X
Z.-Y . Fan and X. Wang, Construction of regular black holes in general relativity, Phys. Rev. D94, 124027 (2016)
2016
-
[28]
Construction of regular black holes in general relativity
K. A. Bronnikov, Comment on “Construction of regular black holes in general relativity”, Phys. Rev. D96, 128501 (2017)
2017
-
[29]
Construction of regular black holes in general relativity
B. Toshmatov, Z. Stuchl ´ık, and B. Ahmedov, Comment on “Construction of regular black holes in general relativity”, Phys. Rev. D98, 028501 (2018)
2018
-
[30]
K. A. Bronnikov, Regular Black Holes Sourced by Nonlinear Electrodynamics, in C. Bambi (ed.) Regular Black Holes: To- wards a New Paradigm of Gravitational Collapse (Springer Sin- gapore, 2023)
2023
-
[31]
Murk and I
S. Murk and I. Soranidis, Light rings and causality for nonsin- gular ultracompact objects sourced by nonlinear electrodynam- ics, Phys. Rev. D110, 044064 (2024)
2024
-
[32]
P. A. Cano and ´A. Murcia, Resolution of Reissner–Nordstr ¨om singularities by higher-derivative corrections, Classical Quan- tum Gravity38, 075014 (2021)
2021
- [33]
-
[34]
Bueno, P
P. Bueno, P. A. Cano, and R. A. Hennigar, Regular black holes from pure gravity, hys. Lett. B861, 139 (2025)
2025
-
[35]
Bueno, P
P. Bueno, P. A. Cano, and R. A. Hennigar, (Generalized) quasi- topological gravities at all orders Classical Quantum Gravity 37, 015002 (2019)
2019
-
[36]
Bueno, P
P. Bueno, P. A. Cano, R. A. Hennigar, M. Lu, and J. Moreno, Generalized quasi-topological gravities: the whole shebang, Classical Quantum Gravity40, 015004 (2022). 22
2022
-
[37]
Moreno and ´A
J. Moreno and ´A. J. Murcia, Classification of generalized qua- sitopological gravities, Phys. Rev. D108, 044016 (2023)
2023
- [38]
-
[39]
Bueno, P
P. Bueno, P. A. Cano, R. A. Hennigar, and ´A. J. Murcia Regular black holes from thin-shell collapse, Phys. Rev. D111, 104009 (2025)
2025
-
[40]
Bueno, P
P. Bueno, P. A. Cano, R. A. Hennigar, and ´A. J. Murcia Dy- namical Formation of Regular Black Holes, Phys. Rev. Lett. 134, 181401 (2025)
2025
-
[41]
Bueno, P
P. Bueno, P. A. Cano, R. A. Hennigar, ´A. J. Murcia, and A. Vincente-Cano, Regular black holes from Oppenheimer-Snyder collapse, Phys. Rev. D112, 064039 (2025)
2025
-
[42]
P. G. S. Fernandes, Singularity resolution and inflation from an infinite tower of regularized curvature corrections, Phys. Rev. D112, 084028 (2025)
2025
-
[43]
J. Borissova and R. Carballo-Rubio, Regular black holes from pure gravity in four dimensions, arXiv: 2602.16773 [gr-qc] (2026)
-
[44]
K. Giesel and H. Liu, From Principles to Effective Models: A Constructive Framework for Effective Covariant Actions with a Unique Vacuum Solution, arXiv: 2512.24960 (2025)
-
[45]
K.Giesel, H. Liu, P. Singh, and S. A. Weigl, Regular black holes and their relationship to polymerized models and mimetic grav- ity, Phys. Rev. D111, 064064 (2025)
2025
-
[46]
Arrechea, S
J. Arrechea, S. Liberati, H. Neshat, and V . Vellucci, From de Sitter to anti–de Sitter singularity regularization: Theory and phenomenology, Phys. Rev. D112, 124029 (2025)
2025
-
[47]
Bambi (ed.),Regular Black Holes: Towards a New Paradigm of Gravitational Collapse(Springer Singapore, 2023)
C. Bambi (ed.),Regular Black Holes: Towards a New Paradigm of Gravitational Collapse(Springer Singapore, 2023)
2023
-
[48]
H. A. Buchdahl, General Relativistic Fluid Spheres, Phys. Rev. 116, 1027 (1959)
1959
-
[49]
Arrechea, C
J. Arrechea, C. Barcel ´o, R. Carballo-Rubio, and L. J. Garay, Semiclassical relativistic stars, Sci. Rep.12, 15958 (2022)
2022
-
[50]
Arrechea, C
J. Arrechea, C. Barcel ´o, R. Carballo-Rubio, and L. J. Garay, Ultracompact horizonless objects in order-reduced semiclassi- cal gravity, Phys. Rev. D109, 104056 (2024)
2024
-
[51]
I. A. Reyes and G. M. Tomaselli, Quantum field theory on com- pact stars near the Buchdahl limit, Phys. Rev. D108, 065006 (2023)
2023
- [52]
-
[53]
R. A. Hennigar, D. Kubiz ˇn´ak, S. Murk, and I. Soranidis, Ther- modynamics of regular black holes in anti-de Sitter space, J. High Energ. Phys. 2025, 121 (2025)
2025
-
[54]
Frolov, Notes on nonsingular models of black holes, Phys
V . Frolov, Notes on nonsingular models of black holes, Phys. Rev. D94, 104056 (2016)
2016
-
[55]
Cadoni, M
M. Cadoni, M. Oi, and A. P. Sanna, Effective models of nonsin- gular quantum black holes, Phys. Rev. D106, 024030 (2022)
2022
-
[56]
Cadoni, M
M. Cadoni, M. De Laurentis, I. De Martino, R. D. Monica, M. Oi and A. P. Sanna, Are nonsingular black holes with super- Planckian hair ruled out by S2 star data?, Phys. Rev. D107, 044038 (2023)
2023
- [57]
-
[58]
Barcel ´o, V
C. Barcel ´o, V . Boyanov, R. Carballo-Rubio and L. J. Garay, Black hole inner horizon evaporation in semiclassical gravity, Class. Quantum Grav.38125003 (2021)
2021
-
[59]
Barcel ´o, V
C. Barcel ´o, V . Boyanov, R. Carballo-Rubio and L. J. Garay, Classical mass inflation versus semiclassical inner horizon in- flation, Phys. Rev. D106, 124006 (2022)
2022
-
[60]
Singularity-free gravitational collapse: From regular black holes to horizonless objects,
R. Carballo-Rubio, F. Di Filippo, S. Liberati and M. Visser, Singularity-free gravitational collapse: From regular black holes to horizonless objects, arXiv:2302.00028 [gr-qc] (2023)
-
[61]
Simovic and I
F. Simovic and I. Soranidis, Euclidean and Hamiltonian ther- modynamics for regular black holes, Phys. Rev. D109, 044029 (2024)
2024
-
[62]
Soranidis, Euclidean methods and phase transitions for the strongest deformations compatible with Schwarzschild asymp- totics, Phys
I. Soranidis, Euclidean methods and phase transitions for the strongest deformations compatible with Schwarzschild asymp- totics, Phys. Rev. D109, 044041 (2024)
2024
-
[63]
RovelliQuantum Gravity(Cambridge University Press, 2010)
C. RovelliQuantum Gravity(Cambridge University Press, 2010)
2010
-
[64]
Rovelli and F
C. Rovelli and F. Vidotto,Covariant Loop Quantum Gravity: An Elementary Introduction to Quantum Gravity and Spinfoam Theory(Cambridge University Press, 2015)
2015
-
[65]
Thiemann,Modern Canonical Quantum General Relativity (Cambridge University Press, 2010)
T. Thiemann,Modern Canonical Quantum General Relativity (Cambridge University Press, 2010)
2010
-
[66]
Hancock,Lectures on the Theory of Elliptic Functions(J
H. Hancock,Lectures on the Theory of Elliptic Functions(J. Wiley and Sons Ltd., New York, 1910)
1910
-
[67]
Vazquez-Leal, M
H. Vazquez-Leal, M. A. Sandoval-Hernandez, and U. Filobello- Nino, The novel family of transcendental Leal-functions with applications to science and engineering, Heliyon6(2020), no e05418
2020
-
[68]
Fujita, X
T. Fujita, X. Gao, and J. Yokoyama, Spatially covariant theo- ries of gravity: disformal transformation, cosmological pertur- bations and the Einstein frame, J. Cosmol. Astropart. Phys.02, 014 (2016)
2016
-
[69]
Gao and Y .-M
X. Gao and Y .-M. Hu, Higher derivative scalar-tensor theory and spatially covariant gravity: The correspondence, Phys. Rev. D102, 084006 (2020)
2020
-
[70]
Ashtekar, T
A. Ashtekar, T. Pawlowski, and P. Singh, Quantum Nature of the Big Bang, Phys. Rev. Lett.96, 141301 (2006)
2006
-
[71]
Ashtekar, T
A. Ashtekar, T. Pawlowski, and P. Singh, Quantum nature of the big bang: Improved dynamics, Phys. Rev. D74, 084003 (2006)
2006
-
[72]
Giesel and H
K. Giesel and H. Liu, to appear
-
[73]
Takahashi and T
K. Takahashi and T. Kobayashi, Extended mimetic gravity: Hamiltonian analysis and gradient instabilities, J. Cosmol. As- tropart. Phys.11, 038 (2017)
2017
-
[74]
Langlois, M
D. Langlois, M. Mancarella, K. Noui and F. Vernizzi, Mimetic gravity as DHOST theories, J. Cosmol. Astropart. Phys.02, 036 (2019)
2019
-
[75]
Han and H
M. Han and H. Liu, Covariantµ¯-scheme effective dynam- ics, mimetic gravity, and nonsingular black holes: Applications to spherically symmetric quantum gravity, Phys. Rev. D109, 084033 (2024)
2024
-
[76]
A. H. Chamseddine and V . Mukhanov, Resolving Cosmological Singularities, JCAP03(2017), 009
2017
-
[77]
Langlois, H
D. Langlois, H. Liu, K. Noui and E. Wilson-Ewing, Effective loop quantum cosmology as a higher-derivative scalar-tensor theory, Class. Quant. Grav.34(2017) no.22, 225004
2017
-
[78]
Ben Achour, F
J. Ben Achour, F. Lamy, H. Liu and K. Noui, Non-singular black holes and the Limiting Curvature Mechanism: A Hamil- tonian perspective, JCAP05(2018), 072
2018
-
[79]
Han and H
M. Han and H. Liu, Improved effective dynamics of loop- quantum-gravity black hole and Nariai limit, Classical Quan- tum Gravity39, 035011 (2022)
2022
-
[80]
Ben Achour, F
J. Ben Achour, F. Lamy, H. Liu, and K. Noui, Polymer Schwarzschild black hole: An effective metric, Europhysics let- ters123, 20006 (2018)
2018
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.