Revisiting black holes and their thermodynamics in Einstein-Kalb-Ramond gravity
Pith reviewed 2026-05-21 18:56 UTC · model grok-4.3
The pith
Einstein-Kalb-Ramond gravity admits two families of exact static black hole solutions in any dimension.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
We obtain two distinct classes of exact static black hole solutions with general topological horizons in diverse dimensions, both with and without a cosmological constant, corresponding to different coupling sectors dictated by the field equations. We analyze their thermodynamic properties and, using the Wald formalism, compute the Noether mass and entropy, establishing the first law and clarifying the role of the Noether mass. Finally, we discuss the implications of this definition of mass for observational constraints in EKR gravity.
What carries the argument
The two classes of exact static black hole solutions that follow from distinct coupling sectors in the Einstein-Kalb-Ramond field equations.
Load-bearing premise
The field equations of EKR gravity permit exact static solutions with the chosen ansatz for the metric and Kalb-Ramond field, and the Wald formalism can be applied without additional surface terms or corrections arising from the nonminimal coupling.
What would settle it
A calculation or observation showing that the Noether mass fails to satisfy the first law for either class of solutions, or that no such exact solutions exist under the static ansatz, would falsify the central results.
read the original abstract
Einstein-Kalb-Ramond (EKR) gravity is an alternative theory in which a rank-two antisymmetric tensor field, the Kalb-Ramond field, is nonminimally coupled to gravity, potentially generating Lorentz-violating backgrounds. In this work, we revisit black hole solutions and thermodynamics in EKR gravity, addressing subtleties overlooked in previous studies. We obtain two distinct classes of exact static black hole solutions with general topological horizons in diverse dimensions, both with and without a cosmological constant, corresponding to different coupling sectors dictated by the field equations. We analyze their thermodynamic properties and, using the Wald formalism, compute the Noether mass and entropy, establishing the first law and clarifying the role of the Noether mass. Finally, we discuss the implications of this definition of mass for observational constraints in EKR gravity.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The manuscript derives two distinct classes of exact static black hole solutions with general topological horizons in diverse dimensions in Einstein-Kalb-Ramond gravity, both with and without a cosmological constant, each corresponding to different sectors of the Kalb-Ramond coupling as dictated by the field equations. It then applies the Wald Noether-charge formalism to obtain the mass and entropy, verifies the first law of thermodynamics, and discusses implications of the Noether mass for observational constraints.
Significance. The explicit construction of exact solutions across dimensions and topologies is a clear strength and supplies concrete spacetimes for testing Lorentz-violating effects in modified gravity. If the thermodynamic analysis holds, the work usefully clarifies the definition of mass and its observational consequences. The overall significance is reduced, however, until the applicability of the standard Wald procedure is verified in the presence of the nonminimal coupling.
major comments (1)
- [Thermodynamics and Wald formalism] The thermodynamics section states that the standard Wald formalism directly yields the first law for the derived solutions. Because the EKR action contains a nonminimal Kalb-Ramond coupling, the general variation produces additional contributions to the symplectic current that are absent in Einstein gravity. The manuscript does not explicitly evaluate these extra boundary terms on the horizon for the chosen static metric and KR-field ansatz, nor demonstrate that they vanish identically. This verification is load-bearing for the claimed entropy formula and first-law relation.
minor comments (2)
- The abstract and introduction refer to 'different coupling sectors dictated by the field equations'; a brief table or explicit listing of the two sectors (including the corresponding values or relations for the coupling constant) would improve readability.
- Notation for the Kalb-Ramond field strength and its coupling constant should be checked for consistency between the action, the field equations, and the solution ansatz.
Simulated Author's Rebuttal
We thank the referee for their careful reading of the manuscript and for identifying a point that requires explicit clarification. We address the major comment on the Wald formalism below.
read point-by-point responses
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Referee: The thermodynamics section states that the standard Wald formalism directly yields the first law for the derived solutions. Because the EKR action contains a nonminimal Kalb-Ramond coupling, the general variation produces additional contributions to the symplectic current that are absent in Einstein gravity. The manuscript does not explicitly evaluate these extra boundary terms on the horizon for the chosen static metric and KR-field ansatz, nor demonstrate that they vanish identically. This verification is load-bearing for the claimed entropy formula and first-law relation.
Authors: We appreciate the referee drawing attention to this subtlety in the nonminimal theory. For the static topological black-hole ansatz used in the paper, the Kalb-Ramond field has support only in the (t,r) plane. When the symplectic current is constructed from the full EKR action and evaluated on the Killing horizon, the additional terms generated by the nonminimal coupling are proportional to contractions that vanish identically because the horizon normal is orthogonal to the KR field strength and the Lie derivative along the Killing vector is zero. We have added an explicit appendix (or subsection) that carries out this boundary-term calculation for both classes of solutions, confirming that no extra contributions survive. The standard Wald expressions for mass and entropy therefore remain valid, and the first law continues to hold as stated. revision: yes
Circularity Check
No significant circularity; derivation remains independent of its inputs
full rationale
The paper obtains exact static black hole solutions by direct substitution of a static metric ansatz and Kalb-Ramond field configuration into the EKR field equations, producing two parameterized families. Thermodynamic quantities follow from applying the standard Wald Noether-charge procedure to the resulting Killing vector on these solutions. No equation reduces a claimed prediction to a fitted parameter by construction, no uniqueness theorem is imported from self-citation to forbid alternatives, and no ansatz is smuggled via prior work. The derivation chain is therefore self-contained against external benchmarks and receives the default non-circularity finding.
Axiom & Free-Parameter Ledger
free parameters (1)
- Kalb-Ramond coupling strength
axioms (2)
- domain assumption The EKR field equations admit static solutions with general topological horizons.
- domain assumption The Wald formalism applies directly to compute Noether mass and entropy without extra corrections from Lorentz violation.
Lean theorems connected to this paper
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IndisputableMonolith/Cost/FunctionalEquation.leanwashburn_uniqueness_aczel unclear?
unclearRelation between the paper passage and the cited Recognition theorem.
We employ the Wald formalism to compute the Noether mass and entropy, thereby establishing the corresponding first law of black hole thermodynamics.
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IndisputableMonolith/Foundation/RealityFromDistinction.leanreality_from_one_distinction unclear?
unclearRelation between the paper passage and the cited Recognition theorem.
the Lagrangian density of EKR gravity takes the form L=R−2Λ +γ1BμλBνλRμν +γ2BμνBμνR−1/12 HμνλHμνλ −V(BμνBμν)
What do these tags mean?
- matches
- The paper's claim is directly supported by a theorem in the formal canon.
- supports
- The theorem supports part of the paper's argument, but the paper may add assumptions or extra steps.
- extends
- The paper goes beyond the formal theorem; the theorem is a base layer rather than the whole result.
- uses
- The paper appears to rely on the theorem as machinery.
- contradicts
- The paper's claim conflicts with a theorem or certificate in the canon.
- unclear
- Pith found a possible connection, but the passage is too broad, indirect, or ambiguous to say the theorem truly supports the claim.
Reference graph
Works this paper leans on
-
[1]
Modern tests of Lorentz invariance,
D. Mattingly, “Modern tests of Lorentz invariance,” Living Rev. Rel.8, 5 (2005) [arXiv:gr- qc/0502097 [gr-qc]]
-
[2]
Tests of Lorentz invariance: a 2013 update
S. Liberati, “Tests of Lorentz invariance: a 2013 update,” Class. Quant. Grav.30, 133001 (2013) [arXiv:1304.5795 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 2013
-
[3]
The Confrontation between General Relativity and Experiment
C. M. Will, “The Confrontation between General Relativity and Experiment,” Living Rev. Rel.17, 4 (2014) [arXiv:1403.7377 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 2014
-
[4]
Testing General Relativity with Present and Future Astrophysical Observations
E. Berti, E. Barausse, V. Cardoso, L. Gualtieri, P. Pani, U. Sperhake, L. C. Stein, N. Wex, K. Yagi and T. Baker,et al.“Testing General Relativity with Present and Future Astrophysical Observations,” Class. Quant. Grav.32, 243001 (2015) [arXiv:1501.07274 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 2015
-
[5]
Tests of Lorentz symmetry in the gravitational sector
A. Hees, Q. G. Bailey, A. Bourgoin, H. P. L. Bars, C. Guerlin and C. Le Poncin-Lafitte, “Tests of Lorentz symmetry in the gravitational sector,” Universe2, no.4, 30 (2016) [arXiv:1610.04682 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 2016
-
[6]
Testing fundamental physics with astrophysical transients,
J. J. Wei and X. F. Wu, “Testing fundamental physics with astrophysical transients,” Front. Phys.16, no.4, 44300 (2021) [arXiv:2102.03724 [astro-ph.HE]]
-
[7]
Probes for String-Inspired Foam, Lorentz, and CPT Violations in Astrophysics,
C. Li and B. Q. Ma, “Probes for String-Inspired Foam, Lorentz, and CPT Violations in Astrophysics,” Symmetry17, no.6, 974 (2025) [arXiv:2508.11172 [hep-ph]]
-
[8]
Spontaneous Breaking of Lorentz Symmetry in String Theory,
V. A. Kostelecky and S. Samuel, “Spontaneous Breaking of Lorentz Symmetry in String Theory,” Phys. Rev. D39, 683 (1989). 21
work page 1989
-
[9]
CPT Violation and the Standard Model
D. Colladay and V. A. Kostelecky, “CPT violation and the standard model,” Phys. Rev. D 55, 6760-6774 (1997) [arXiv:hep-ph/9703464 [hep-ph]]
work page internal anchor Pith review Pith/arXiv arXiv 1997
-
[10]
Lorentz-Violating Extension of the Standard Model
D. Colladay and V. A. Kostelecky, “Lorentz violating extension of the standard model,” Phys. Rev. D58, 116002 (1998) [arXiv:hep-ph/9809521 [hep-ph]]
work page internal anchor Pith review Pith/arXiv arXiv 1998
-
[11]
Gravity, Lorentz Violation, and the Standard Model
V. A. Kostelecky, “Gravity, Lorentz violation, and the standard model,” Phys. Rev. D69, 105009 (2004) [arXiv:hep-th/0312310 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv 2004
-
[12]
Lorentz violation with an antisymmetric tensor
B. Altschul, Q. G. Bailey and V. A. Kostelecky, “Lorentz violation with an antisymmetric tensor,” Phys. Rev. D81, 065028 (2010) [arXiv:0912.4852 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 2010
-
[13]
Classical direct interstring action,
M. Kalb and P. Ramond, “Classical direct interstring action,” Phys. Rev. D9, 2273-2284 (1974)
work page 1974
-
[14]
Modified black hole solution with a background Kalb–Ramond field,
L. A. Lessa, J. E. G. Silva, R. V. Maluf and C. A. S. Almeida, “Modified black hole solution with a background Kalb–Ramond field,” Eur. Phys. J. C80, no.4, 335 (2020) [arXiv:1911.10296 [gr-qc]]
-
[15]
Static and spherically symmetric black holes in gravity with a background Kalb-Ramond field,
K. Yang, Y. Z. Chen, Z. Q. Duan and J. Y. Zhao, “Static and spherically symmetric black holes in gravity with a background Kalb-Ramond field,” Phys. Rev. D108, no.12, 124004 (2023) [arXiv:2308.06613 [gr-qc]]
-
[16]
Black Hole Entropy and Viscosity Bound in Horndeski Gravity
X. H. Feng, H. S. Liu, H. L¨ u and C. N. Pope, “Black Hole Entropy and Viscosity Bound in Horndeski Gravity,” JHEP11, 176 (2015) [arXiv:1509.07142 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv 2015
-
[17]
Thermodynamics of Charged Black Holes in Einstein-Horndeski-Maxwell Theory
X. H. Feng, H. S. Liu, H. L¨ u and C. N. Pope, “Thermodynamics of Charged Black Holes in Einstein-Horndeski-Maxwell Theory,” Phys. Rev. D93, no.4, 044030 (2016) [arXiv:1512.02659 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv 2016
-
[18]
Notes on thermodynamics of Schwarzschild- like bumblebee black hole,
Y. S. An, “Notes on thermodynamics of Schwarzschild-like bumblebee black hole,” Phys. Dark Univ.45, 101520 (2024) [arXiv:2401.15430 [gr-qc]]
-
[19]
Taub-NUT-like black holes in Einstein-bumblebee gravity,
Y. Q. Chen and H. S. Liu, “Taub-NUT-like black holes in Einstein-bumblebee gravity,” Phys. Rev. D112, no.8, 084040 (2025) [arXiv:2505.23104 [gr-qc]]
-
[20]
Dyonic RN-like and Taub-NUT-like black holes in Einstein- bumblebee gravity,
S. Li, L. Liang and L. Ma, “Dyonic RN-like and Taub-NUT-like black holes in Einstein- bumblebee gravity,” [arXiv:2510.04405 [gr-qc]]
-
[21]
Black Hole Entropy is Noether Charge
R. M. Wald, “Black hole entropy is the Noether charge,” Phys. Rev. D48, no.8, R3427-R3431 (1993) [arXiv:gr-qc/9307038 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 1993
-
[22]
Some Properties of Noether Charge and a Proposal for Dynamical Black Hole Entropy
V. Iyer and R. M. Wald, “Some properties of Noether charge and a proposal for dynamical black hole entropy,” Phys. Rev. D50, 846-864 (1994) [arXiv:gr-qc/9403028 [gr-qc]]. 22
work page internal anchor Pith review Pith/arXiv arXiv 1994
-
[23]
AdS Dyonic Black Hole and its Thermodynamics
H. L¨ u, Y. Pang and C. N. Pope, “AdS Dyonic Black Hole and its Thermodynamics,” JHEP 11, 033 (2013) [arXiv:1307.6243 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv 2013
-
[24]
Dyonic AdS black holes in maximal gauged supergravity
D. D. K. Chow and G. Comp` ere, “Dyonic AdS black holes in maximal gauged supergravity,” Phys. Rev. D89, no.6, 065003 (2014) [arXiv:1311.1204 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv 2014
-
[25]
S. Q. Wu and S. Li, “Thermodynamics of Static Dyonic AdS Black Holes in theω- Deformed Kaluza-Klein Gauged Supergravity Theory,” Phys. Lett. B746, 276-280 (2015) [arXiv:1505.00117 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv 2015
-
[26]
Improved Wald formalism and first law of dyonic black strings with mixed Chern-Simons terms,
L. Ma, Y. Pang and H. Lu, “Improved Wald formalism and first law of dyonic black strings with mixed Chern-Simons terms,” JHEP10, 142 (2022) [arXiv:2202.08290 [hep-th]]
-
[27]
Thermodynamics of Taub-NUT and Plebanski solutions,
H. S. Liu, H. Lu and L. Ma, “Thermodynamics of Taub-NUT and Plebanski solutions,” JHEP 10, 174 (2022) [arXiv:2208.05494 [gr-qc]]
-
[28]
Thermodynamical First Laws of Black Holes in Quadratically-Extended Gravities
Z. Y. Fan and H. Lu, “Thermodynamical First Laws of Black Holes in Quadratically-Extended Gravities,” Phys. Rev. D91, no.6, 064009 (2015) [arXiv:1501.00006 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv 2015
-
[29]
Higher derivative contributions to black hole thermodynamics at NNLO,
L. Ma, Y. Pang and H. Lu, “Higher derivative contributions to black hole thermodynamics at NNLO,” JHEP06(2023), 087 [erratum: JHEP08(2024), 118] [arXiv:2304.08527 [hep-th]]
-
[30]
Improved Reall-Santos method for AdS black holes in general 4-derivative gravities,
P. J. Hu, L. Ma, H. L¨ u and Y. Pang, “Improved Reall-Santos method for AdS black holes in general 4-derivative gravities,” Sci. China Phys. Mech. Astron.67(2024) no.8, 280412 [arXiv:2312.11610 [hep-th]]
-
[31]
Effectiveness of Weyl gravity in probing quantum corrections to AdS black holes,
L. Ma, P. J. Hu, Y. Pang and H. Lu, “Effectiveness of Weyl gravity in probing quantum corrections to AdS black holes,” Phys. Rev. D110(2024) no.2, L021901 [arXiv:2403.12131 [hep-th]]
-
[32]
Thermodynamics of Lifshitz Black Holes
H. S. Liu and H. L¨ u, “Thermodynamics of Lifshitz Black Holes,” JHEP12, 071 (2014) [arXiv:1410.6181 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv 2014
-
[33]
Scalar Charges in Asymptotic AdS Geometries
H. S. Liu and H. L¨ u, “Scalar Charges in Asymptotic AdS Geometries,” Phys. Lett. B730, 267-270 (2014) [arXiv:1401.0010 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv 2014
-
[34]
Thermodynamics of AdS Black Holes in Einstein-Scalar Gravity
H. Lu, C. N. Pope and Q. Wen, “Thermodynamics of AdS Black Holes in Einstein-Scalar Gravity,” JHEP03, 165 (2015) [arXiv:1408.1514 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv 2015
-
[35]
First law of black hole mechanics in Einstein-Maxwell and Einstein-Yang-Mills theories
S. Gao, “The First law of black hole mechanics in Einstein-Maxwell and Einstein-Yang-Mills theories,” Phys. Rev. D68, 044016 (2003) [arXiv:gr-qc/0304094 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 2003
-
[36]
Dyonic (A)dS Black Holes in Einstein-Born-Infeld Theory in Diverse Dimensions
S. Li, H. Lu and H. Wei, “Dyonic (A)dS Black Holes in Einstein-Born-Infeld Theory in Diverse Dimensions,” JHEP07, 004 (2016) [arXiv:1606.02733 [hep-th]]. 23
work page internal anchor Pith review Pith/arXiv arXiv 2016
-
[37]
Thermodynamics of Einstein-Proca AdS Black Holes
H. S. Liu, H. L¨ u and C. N. Pope, “Thermodynamics of Einstein-Proca AdS Black Holes,” JHEP06, 109 (2014) [arXiv:1402.5153 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv 2014
-
[38]
Radial oscillations of neutron stars in Starobin- sky gravity and its Gauss-Bonnet extension,
Z. Li, Z. X. Yu, Z. Luo, S. Li and H. Yu, “Radial oscillations of neutron stars in Starobin- sky gravity and its Gauss-Bonnet extension,” Phys. Rev. D112, no.4, 044019 (2025) [arXiv:2507.18916 [gr-qc]]
-
[39]
Estimating the final spin of binary black holes merger in STU supergravity,
S. L. Li, W. D. Tan, P. Wu and H. Yu, “Estimating the final spin of binary black holes merger in STU supergravity,” Nucl. Phys. B975, 115665 (2022) [arXiv:2003.01957 [gr-qc]]
-
[40]
Spontaneous Lorentz and Diffeomorphism Violation, Massive Modes, and Gravity
R. Bluhm, S. H. Fung and V. A. Kostelecky, “Spontaneous Lorentz and Diffeomorphism Violation, Massive Modes, and Gravity,” Phys. Rev. D77, 065020 (2008) [arXiv:0712.4119 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv 2008
-
[41]
Black holes with a cosmological constant in bumblebee gravity,
R. V. Maluf and J. C. S. Neves, “Black holes with a cosmological constant in bumblebee gravity,” Phys. Rev. D103, no.4, 044002 (2021) [arXiv:2011.12841 [gr-qc]]
-
[42]
Generalised Smarr Formula and the Viscosity Bound for Einstein-Maxwell-Dilaton Black Holes
H. S. Liu, H. Lu and C. N. Pope, “Generalized Smarr formula and the viscosity bound for Einstein-Maxwell-dilaton black holes,” Phys. Rev. D92, 064014 (2015) [arXiv:1507.02294 [hep-th]]. 24
work page internal anchor Pith review Pith/arXiv arXiv 2015
discussion (0)
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