Statistical Physics of Planar Carroll Systems
Pith reviewed 2026-06-26 06:46 UTC · model grok-4.3
The pith
Central extensions of the Carroll algebra in the plane enable consistent statistical physics for Carrollian systems with angular momentum.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
Thanks to the central extensions of the Carroll algebra in the plane, and by considering systems with angular momentum, there exists a well defined notion of planar Carrollian statistical physics. For particles on a uniformly rotating disc the partition function is computed via Souriau's geometric thermodynamics, with one central charge determining the rotation direction. Entropy scales logarithmically with the disc area, pressure follows the two-dimensional ideal gas law, and an effective Hamiltonian is derived from symmetry considerations.
What carries the argument
Central extensions of the Carroll algebra in two dimensions together with Souriau's geometric thermodynamics applied to angular-momentum-carrying particles on a uniformly rotating disc.
If this is right
- Rotation is inevitable for thermal equilibrium of planar Carroll systems.
- One of the central charges fixes the direction of rotation.
- Entropy scales logarithmically with the disc area.
- Pressure obeys the two-dimensional ideal gas law.
- An effective Hamiltonian follows directly from the symmetry algebra.
Where Pith is reading between the lines
- Dimensionality appears decisive for convergence of the Carroll limit, suggesting similar behavior may hold in other low-dimensional Carrollian models.
- The logarithmic entropy-area relation invites comparison with area-law phenomena in information or gravitational contexts where Carroll symmetry emerges.
- Symmetry-based methods used here could be applied to derive thermodynamics for Carrollian systems on other manifolds without explicit Hamiltonians.
Load-bearing premise
The central extensions of the Carroll algebra in two dimensions, together with the inclusion of angular momentum, suffice to make the Carroll limit of Poincaré statistical physics converge.
What would settle it
Explicit computation of the partition function for a planar Carroll system on a rotating disc that diverges even after including the central extensions and angular momentum.
read the original abstract
In this article, we define and study the statistical physics of planar Carrollian systems. While it has been shown recently that, for general dimensions, the Carroll limit of Poincar\'e statistical physics typically does not converge, we show that thanks to the central extensions of the Carroll algebra in the plane, and by considering systems with angular momentum, there exists a well defined notion of planar Carrollian statistical physics. Using Souriau's geometric thermodynamics, we compute the partition function for particles on a uniformly rotating disc, and show that rotation is inevitable for thermal equilibrium of planar Carroll systems, with one of the central charges determining the direction of rotation. We derive thermodynamic quantities in particular entropy, which scales logarithmically with the disc area, and pressure, which follows the two-dimensional ideal gas law. Though all results are obtained from symmetry considerations, we also derive the corresponding effective Hamiltonian.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The manuscript defines and studies the statistical physics of planar Carrollian systems. It argues that while the Carroll limit of Poincaré statistical physics fails to converge in general dimensions, the central extensions of the Carroll algebra in two dimensions, combined with the inclusion of angular momentum, allow a well-defined notion of planar Carrollian statistical physics. Using Souriau's geometric thermodynamics, the partition function is computed for particles on a uniformly rotating disc; the authors show that rotation is required for thermal equilibrium, with one central charge fixing the sense of rotation. Thermodynamic quantities are derived, including an entropy that scales logarithmically with disc area and a pressure obeying the two-dimensional ideal-gas law. An effective Hamiltonian is also obtained from symmetry considerations.
Significance. If the convergence of the Carroll limit is rigorously established, the work supplies the first consistent framework for Carrollian statistical mechanics in the plane and yields concrete, symmetry-derived predictions (logarithmic entropy, ideal-gas pressure) that are falsifiable. The reliance on geometric thermodynamics and the derivation of an effective Hamiltonian from first principles are methodological strengths that could extend to Carrollian analogs in condensed-matter or gravitational settings.
major comments (2)
- [Abstract and opening paragraph] Abstract and §1 (opening paragraph): the central claim that the two-dimensional central extensions plus angular momentum suffice to make the Carroll limit converge is load-bearing, yet the visible text supplies neither an explicit partition-function expression nor an error estimate or convergence proof for the limit; without these the thermodynamic results cannot be verified.
- [Section on Souriau geometric thermodynamics] Section on Souriau geometric thermodynamics (presumably §3–4): the statement that one central charge determines the direction of rotation requires an explicit relation between the sign of the central charge, the equilibrium condition, and the measure on the coadjoint orbit; the current symmetry argument alone does not demonstrate uniqueness or stability of the rotating equilibrium.
minor comments (2)
- The effective Hamiltonian is stated to be derived from symmetry; placing its explicit form in an appendix or main-text equation would allow direct comparison with the geometric-thermodynamics partition function.
- Notation for the two central charges should be introduced once and used consistently; the current text occasionally refers to “one of the central charges” without a numbered label.
Simulated Author's Rebuttal
We thank the referee for their careful reading and constructive comments on our manuscript. We address the two major comments point by point below, clarifying the role of the central extensions and geometric thermodynamics while indicating revisions that will strengthen the explicitness of the arguments.
read point-by-point responses
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Referee: [Abstract and opening paragraph] Abstract and §1 (opening paragraph): the central claim that the two-dimensional central extensions plus angular momentum suffice to make the Carroll limit converge is load-bearing, yet the visible text supplies neither an explicit partition-function expression nor an error estimate or convergence proof for the limit; without these the thermodynamic results cannot be verified.
Authors: We agree that the convergence claim is central and benefits from greater explicitness. The partition function is computed explicitly via Souriau's geometric thermodynamics on the coadjoint orbits of the centrally extended Carroll algebra (including angular momentum) in Sections 3–4; the central extensions regularize the phase-space integrals that diverge in the Carroll limit without them. The resulting thermodynamic quantities (logarithmic entropy, ideal-gas pressure) are direct consequences. To make this fully verifiable from the opening sections, we will insert the explicit partition-function expression together with a short convergence argument and error estimate in the revised manuscript. revision: yes
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Referee: [Section on Souriau geometric thermodynamics] Section on Souriau geometric thermodynamics (presumably §3–4): the statement that one central charge determines the direction of rotation requires an explicit relation between the sign of the central charge, the equilibrium condition, and the measure on the coadjoint orbit; the current symmetry argument alone does not demonstrate uniqueness or stability of the rotating equilibrium.
Authors: We thank the referee for this precise observation. The geometric construction already ties the sign of one central charge to the orientation of the coadjoint orbit and hence to the sense of rotation that yields a normalizable equilibrium measure; the second central charge is fixed by the requirement of a well-defined thermal state. Nevertheless, the referee is correct that an explicit formula linking the central-charge sign, the equilibrium condition, and the orbit measure would strengthen the uniqueness and stability statements. We will add this relation, together with a brief stability remark, in the revised version of Sections 3–4. revision: yes
Circularity Check
No significant circularity
full rationale
The derivation begins from the external fact of central extensions in the 2D Carroll algebra plus angular momentum, which the abstract states suffice for convergence of the Carroll limit (contrasted with the non-convergent general-dimensional case shown elsewhere). It then invokes the independent Souriau geometric-thermodynamics framework to obtain the partition function on a rotating disc, from which entropy (logarithmic in area) and pressure (2D ideal-gas law) follow by direct symmetry algebra without any fitted parameters renamed as predictions, self-definitional loops, or load-bearing self-citations. All steps remain self-contained against external mathematical and thermodynamic benchmarks.
Axiom & Free-Parameter Ledger
axioms (2)
- domain assumption Central extensions of the Carroll algebra in the plane allow the Carroll limit of Poincaré statistical physics to converge when angular momentum is included.
- domain assumption Souriau's geometric thermodynamics can be applied to Carrollian systems on a rotating disc.
Reference graph
Works this paper leans on
-
[1]
Une nouvelle limite non-relativiste du groupe de Poincar´e
J.-M. L ´evy-Leblond, “Une nouvelle limite non-relativiste du groupe de Poincar´e”, Annales de l’I.H.P. Physique th´eorique3, p. 1 (1965),http://www.numdam.org/item/AIHPA_1965__3_1_1_0
1965
-
[2]
Possible kinematics
H. Bacry, J. Levy-Leblond, “Possible kinematics”, J. Math. Phys.9, p. 1605, (1968)
1968
-
[3]
On an analogue of the Galilei group
N. D. Sen Gupta, “On an analogue of the Galilei group”, Nuovo Cim. A44, p. 512, (1966)
1966
-
[4]
Carroll versus Newton and Galilei: two dual non-Einsteinian concepts of time
C. Duval, G. W. Gibbons, P. A. Horvathy, P. M. Zhang, “Carroll versus Newton and Galilei: two dual non-Einsteinian concepts of time”, Class. Quant. Grav.31, p. 085016, (2014), arXiv: 1402.0657
Pith/arXiv arXiv 2014
-
[5]
E. Bergshoeff, J. Gomis, G. Longhi, “Dynamics of Carroll Particles”, Class. Quant. Grav.31, p. 205009, (2014), arXiv: 1405.2264
Pith/arXiv arXiv 2014
-
[6]
Gravitational waves in general relativity. 7. Waves from axisymmetric isolated systems
H. Bondi, M. G. J. van der Burg, A. W. K. Metzner, “Gravitational waves in general relativity. 7. Waves from axisymmetric isolated systems”, Proc. Roy. Soc. Lond. A269, p. 21, (1962)
1962
-
[7]
Asymptotic Symmetries in Gravitational Theory
R. Sachs, “Asymptotic Symmetries in Gravitational Theory”, Phys. Rev.128, p. 2851, (1962)
1962
-
[8]
Conformal Carroll groups and BMS symmetry
C. Duval, G. W. Gibbons, P. A. Horvathy, “Conformal Carroll groups and BMS symmetry”, Class. Quant. Grav.31, p. 092001, (2014), arXiv: 1402.5894
Pith/arXiv arXiv 2014
-
[9]
C. Duval, G. W. Gibbons, P. A. Horvathy, “Conformal Carroll groups”, J. Phys. A47, p. 335204, (2014), arXiv: 1403.4213
Pith/arXiv arXiv 2014
-
[10]
Flat holography and Carrollian fluids
L. Ciambelli, C. Marteau, A. C. Petkou, P. M. Petropoulos, K. Siampos, “Flat holography and Carrollian fluids”, JHEP07, p. 165, (2018), arXiv: 1802.06809
Pith/arXiv arXiv 2018
-
[11]
Two-dimensional fluids and their holographic duals
A. Campoleoni, L. Ciambelli, C. Marteau, P. M. Petropoulos, K. Siampos, “Two-dimensional fluids and their holographic duals”, Nucl. Phys. B946, p. 114692, (2019), arXiv: 1812.04019
Pith/arXiv arXiv 2019
-
[12]
Carrollian Perspective on Celestial Holography
L. Donnay, A. Fiorucci, Y. Herfray, R. Ruzziconi, “Carrollian Perspective on Celestial Holography”, Phys. Rev. Lett.129, p. 071602, (2022)
2022
-
[13]
Bridging Carrollian and celestial holography
L. Donnay, A. Fiorucci, Y. Herfray, R. Ruzziconi, “Bridging Carrollian and celestial holography”, Phys. Rev. D107, p. 126027, (2023), arXiv: 2212.12553
arXiv 2023
-
[14]
Carrollian approach to 1 + 3D flat holography
A. Saha, “Carrollian approach to 1 + 3D flat holography”, JHEP06, p. 051, (2023), arXiv: 2304.02696
arXiv 2023
-
[15]
Scattering Amplitudes: Celestial and Carrollian
A. Bagchi, S. Banerjee, R. Basu, S. Dutta, “Scattering Amplitudes: Celestial and Carrollian”, Phys. Rev. Lett.128, p. 241601, (2022). 13
2022
-
[16]
Carrollian superconformal theories and super BMS
A. Bagchi, D. Grumiller, P. Nandi, “Carrollian superconformal theories and super BMS”, JHEP05, p. 044, (2022), arXiv: 2202.01172
arXiv 2022
-
[17]
AdS Witten diagrams to Carrollian correlators
A. Bagchi, P. Dhivakar, S. Dutta, “AdS Witten diagrams to Carrollian correlators”, JHEP04, p. 135, (2023), arXiv: 2303.07388
arXiv 2023
-
[18]
Near-horizon Carroll symmetry and black hole Love numbers
R. F. Penna, “Near-horizon Carroll symmetry and black hole Love numbers”, arXiv: 1812.05643
-
[19]
Carrollian Physics at the Black Hole Horizon
L. Donnay, C. Marteau, “Carrollian Physics at the Black Hole Horizon”, Class. Quant. Grav.36, p. 165002, (2019), arXiv: 1903.09654
arXiv 2019
-
[20]
Anyonic spin-Hall effect on the black hole horizon
L. Marsot, P.-M. Zhang, P. Horvathy, “Anyonic spin-Hall effect on the black hole horizon”, Phys. Rev. D106, p. L121503, (2022), arXiv: 2207.06302
arXiv 2022
-
[21]
Non-linear black hole dynamics and Carrollian fluids
J. Redondo-Yuste, L. Lehner, “Non-linear black hole dynamics and Carrollian fluids”, JHEP02, p. 240, (2023), arXiv: 2212.06175
arXiv 2023
-
[22]
Carrollian hydrodynamics from symmetries
L. Freidel, P. Jai-akson, “Carrollian hydrodynamics from symmetries”, Class. Quant. Grav.40, p. 055009, (2023), arXiv: 2209.03328
arXiv 2023
-
[23]
Carrollian hydrodynamics and symplectic structure on stretched horizons
L. Freidel, P. Jai-akson, “Carrollian hydrodynamics and symplectic structure on stretched horizons”, JHEP05, p. 135, (2024), arXiv: 2211.06415
arXiv 2024
-
[24]
Geometry of Carrollian stretched horizons
L. Freidel, P. Jai-akson, “Geometry of Carrollian stretched horizons”, Class. Quant. Grav.42, p. 065010, (2025), arXiv: 2406.06709
arXiv 2025
-
[25]
Carroll symmetry of plane gravitational waves
C. Duval, G. W. Gibbons, P. A. Horvathy, P. M. Zhang, “Carroll symmetry of plane gravitational waves”, Class. Quant. Grav.34, p. 175003, (2017), arXiv: 1702.08284
Pith/arXiv arXiv 2017
-
[26]
The Memory Effect for Plane Gravitational Waves
P. M. Zhang, C. Duval, G. W. Gibbons, P. A. Horvathy, “The Memory Effect for Plane Gravitational Waves”, Phys. Lett. B772, p. 743, (2017), arXiv: 1704.05997
Pith/arXiv arXiv 2017
-
[27]
Soft gravitons and the memory effect for plane gravitational waves
P. M. Zhang, C. Duval, G. W. Gibbons, P. A. Horvathy, “Soft gravitons and the memory effect for plane gravitational waves”, Phys. Rev. D96, p. 064013, (2017), arXiv: 1705.01378
Pith/arXiv arXiv 2017
-
[28]
Strings near black holes are Carrollian
A. Bagchi, A. Banerjee, J. Hartong, E. Have, K. S. Kolekar, M. Mandlik, “Strings near black holes are Carrollian”, Phys. Rev. D110, p. 086009, (2024), arXiv: 2312.14240
arXiv 2024
-
[29]
Unification of Decoupling Limits in String and M Theory
C. D. A. Blair, J. Lahnsteiner, N. A. Obers, Z. Yan, “Unification of Decoupling Limits in String and M Theory”, Phys. Rev. Lett.132, p. 161603, (2024), arXiv: 2311.10564
arXiv 2024
-
[30]
Worldsheet formalism for decoupling limits in string theory
J. Gomis, Z. Yan, “Worldsheet formalism for decoupling limits in string theory”, JHEP07, p. 102, (2024), arXiv: 2311.10565
Pith/arXiv arXiv 2024
-
[31]
Strings near black holes are Carrollian. Part II
A. Bagchi, A. Banerjee, J. Hartong, E. Have, K. S. Kolekar, “Strings near black holes are Carrollian. Part II”, JHEP11, p. 024, (2024), arXiv: 2407.12911
arXiv 2024
-
[32]
Strings near BTZ black holes: a Carrollian chronicle
A. Banerjee, A. Bhattacharya, S. R. Iyer, A. Mishra, P. Pandit, “Strings near BTZ black holes: a Carrollian chronicle”, JHEP02, p. 152, (2026), arXiv: 2510.16104
Pith/arXiv arXiv 2026
-
[33]
Magic fermions: Carroll and flat bands
A. Bagchi, A. Banerjee, R. Basu, M. Islam, S. Mondal, “Magic fermions: Carroll and flat bands”, JHEP03, p. 227, (2023), arXiv: 2211.11640
arXiv 2023
-
[34]
Fractons, dipole symmetries and curved spacetime
L. Bidussi, J. Hartong, E. Have, J. Musaeus, S. Prohazka, “Fractons, dipole symmetries and curved spacetime”, SciPost Phys.12, p. 205, (2022), arXiv: 2111.03668
arXiv 2022
-
[35]
Hall effects in Carroll dynamics
L. Marsot, P. M. Zhang, M. Chernodub, P. A. Horvathy, “Hall effects in Carroll dynamics”, Phys. Rept.1028, p. 1, (2023), arXiv: 2212.02360. 14
arXiv 2023
-
[36]
Carroll/fracton particles and their correspondence
J. Figueroa-O’Farrill, A. P ´erez, S. Prohazka, “Carroll/fracton particles and their correspondence”, JHEP06, p. 207, (2023), arXiv: 2305.06730
arXiv 2023
-
[37]
Embedding Galilean and Carrollian geometries I. Gravitational waves
K. Morand, “Embedding Galilean and Carrollian geometries I. Gravitational waves”, J. Math. Phys. 61, p. 082502, (2020), arXiv: 1811.12681
arXiv 2020
-
[38]
Carroll structures, null geometry, and conformal isometries
L. Ciambelli, R. G. Leigh, C. Marteau, P. M. Petropoulos, “Carroll structures, null geometry, and conformal isometries”, Phys. Rev. D100, p. 046010, (2019)
2019
-
[39]
Geometry of Zero Signature Space-times
M. Henneaux, “Geometry of Zero Signature Space-times”, Bull. Soc. Math. Belg.31, p. 47 (1979)
1979
-
[40]
Celestial mechanics, conformal structures and gravitational waves
C. Duval, G. W. Gibbons, P. Horvathy, “Celestial mechanics, conformal structures and gravitational waves”, Phys. Rev. D43, p. 3907, (1991), arXiv: hep-th/0512188
Pith/arXiv arXiv 1991
-
[41]
On the ultrarelativistic limit of general relativity
G. Dautcourt, “On the ultrarelativistic limit of general relativity”, Acta Phys. Polon. B29, p. 1047 (1998), arXiv: gr-qc/9801093
Pith/arXiv arXiv 1998
-
[42]
Central extensions of the quasiorthogonal Lie algebras
J. A. de Azcarraga, F. J. Herranz, J. C. Perez Bueno, M. Santander, “Central extensions of the quasiorthogonal Lie algebras”, J. Phys. A31, p. 1373, (1998), arXiv: q-alg/9612021
Pith/arXiv arXiv 1998
-
[43]
Group theoretical construction of planar Noncommutative Phase Spaces
A. Ngendakumana, J. Nzotungicimpaye, L. Todjihounde, “Group theoretical construction of planar Noncommutative Phase Spaces”, J. Math. Phys.55, p. 013508, (2014), arXiv: 1308.3065
Pith/arXiv arXiv 2014
-
[44]
On Unitary ray representations of continuous groups
V. Bargmann, “On Unitary ray representations of continuous groups”, Annals of Mathematics59, p. 1, (1954)
1954
-
[45]
Galilei Group and Galilean Invariance
J.-M. L ´evy-Leblond, “Galilei Group and Galilean Invariance”, inGroup Theory and Its Applications (Loebl, ed.), vol II, p. 221, New York: Academic Press, 1971
1971
-
[46]
Moyal quantization of 2+1-dimensional Galilean systems
A. Ballesteros, M. Gadella, M. A. Del Olmo, “Moyal quantization of 2+1-dimensional Galilean systems”, Journal of Mathematical Physics33, p. 3379, (1992)
1992
-
[47]
J. Lukierski, P. C. Stichel, W. J. Zakrzewski, “Galilean invariant (2+1)-dimensional models with a Chern-Simons-like term and D = 2 noncommutative geometry”, Annals Phys.260, p. 224, (1997), arXiv: hep-th/9612017
Pith/arXiv arXiv 1997
-
[48]
The exotic Galilei group and the “Peierls substitution
C. Duval, P. A. Horv´athy, “The exotic Galilei group and the “Peierls substitution””, Physics letters. B 479, p. 284, (2000)
2000
-
[49]
Exotic Galilean symmetry in the noncommutative plane, and the Hall effect
C. Duval, P. A. Horvathy, “Exotic Galilean symmetry in the noncommutative plane, and the Hall effect”, J. Phys. A34, p. 10097, (2001), arXiv: hep-th/0106089
Pith/arXiv arXiv 2001
-
[50]
Anomalous Quantum Hall Effect: An Incompressible Quantum Fluid with Fraction- ally Charged Excitations
R. B. Laughlin, “Anomalous Quantum Hall Effect: An Incompressible Quantum Fluid with Fraction- ally Charged Excitations”, Phys. Rev. Lett.50, p. 1395, (1983)
1983
-
[51]
Planar Carrollean dynamics, and the Carroll quantum equation
L. Marsot, “Planar Carrollean dynamics, and the Carroll quantum equation”, J. Geom. Phys.179, p. 104574, (2022), arXiv: 2110.08489
arXiv 2022
-
[52]
J. de Boer, J. Hartong, N. A. Obers, W. Sybesma, S. Vandoren, “Carroll stories”, JHEP09, p. 148, (2023), arXiv: 2307.06827
arXiv 2023
-
[53]
L. D. Landau, E. M. Lifshitz,Statistical Physics, part 1, vol 5 ofCourse of Theoretical Physics. Pergamon Press, England, 1980
1980
-
[54]
Souriau,Structure des syst `emes dynamiques
J.-M. Souriau,Structure des syst `emes dynamiques. Dunod, Paris, 1970, doi: 10.1007/978-1-4612- 0281-3. Translation to English:Structure of Dynamical Systems. A Symplectic View of Physics. (Birkh¨auser, Basel, 1997)
-
[55]
J. E. Marsden, T. Ratiu,Introduction to Mechanics and Symmetry. New York, Springer-Verlag, 1994. 15
1994
-
[56]
C.-M. Marle, “From Tools in Symplectic and Poisson Geometry to J.-M. Souriau’s Theories of Statistical Mechanics and Thermodynamics”, Entropy18, p. 370, (2016), arXiv: 1608.00103
Pith/arXiv arXiv 2016
-
[57]
Geometric Theory of Heat from Souriau Lie Groups Thermodynamics and Koszul Hessian Geometry: Applications in Information Geometry for Exponential Families
F. Barbaresco, “Geometric Theory of Heat from Souriau Lie Groups Thermodynamics and Koszul Hessian Geometry: Applications in Information Geometry for Exponential Families”, Entropy18, p. 386, (2016)
2016
-
[58]
Thermodynamics `a la Souriau on K ¨ahler Non-Compact Symmetric Spaces for Cartan Neural Networks
P. G. Fr ´e, A. S. Sorin, M. Trigiante, “Thermodynamics `a la Souriau on K ¨ahler Non-Compact Symmetric Spaces for Cartan Neural Networks”, Entropy29, p. 365, (2026), arXiv: 2512.16772
Pith/arXiv arXiv 2026
-
[59]
D. Doshi, A. Gromov, “Vortices as Fractons”, Commun. Phys.4, p. 44, (2021), arXiv: 2005.03015
arXiv 2021
-
[60]
Logarithmic correction to the Bekenstein-Hawking entropy
R. K. Kaul, P. Majumdar, “Logarithmic correction to the Bekenstein-Hawking entropy”, Phys. Rev. Lett.84, p. 5255, (2000), arXiv: gr-qc/0002040
Pith/arXiv arXiv 2000
-
[61]
Logarithmic corrections to black hole entropy from the Cardy formula
S. Carlip, “Logarithmic corrections to black hole entropy from the Cardy formula”, Class. Quant. Grav.17, p. 4175, (2000), arXiv: gr-qc/0005017
Pith/arXiv arXiv 2000
-
[62]
Thermal fluctuations and black hole entropy
G. Gour, A. J. M. Medved, “Thermal fluctuations and black hole entropy”, Class. Quant. Grav.20, p. 3307, (2003), arXiv: gr-qc/0305018
Pith/arXiv arXiv 2003
-
[63]
Log correction to the black hole area law
A. Ghosh, P. Mitra, “Log correction to the black hole area law”, Phys. Rev. D71, p. 027502, (2005)
2005
-
[64]
When conceptual worlds collide: The GUP and the BH entropy
A. J. M. Medved, E. C. Vagenas, “When conceptual worlds collide: The GUP and the BH entropy”, Phys. Rev. D70, p. 124021, (2004), arXiv: hep-th/0411022
Pith/arXiv arXiv 2004
-
[65]
A. Sen, “Logarithmic Corrections to Schwarzschild and Other Non-extremal Black Hole Entropy in Different Dimensions”, JHEP04, p. 156, (2013), arXiv: 1205.0971
Pith/arXiv arXiv 2013
-
[66]
Kinetic Theory of Carroll Hydrodynamics
V. Chabirand, A. Fiorucci, P. M. Petropoulos, M. Vilatte, “Kinetic Theory of Carroll Hydrodynamics”, arXiv: 2605.06786. 16
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