Dyonic Black Holes in Lorentz-Violating Gravity with a Background Kalb--Ramond Field
Pith reviewed 2026-05-20 09:14 UTC · model grok-4.3
The pith
A nonminimal coupling between the Kalb-Ramond and electromagnetic fields produces an exact dyonic black hole solution in Lorentz-violating gravity.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
By introducing a nonminimal coupling between the Kalb--Ramond field and the electromagnetic field, an exact four-dimensional static, spherically symmetric dyonic black hole solution is constructed in Lorentz-violating gravity with a background Kalb--Ramond field. The curvature invariants confirm a genuine singularity at r=0. Geodesic analysis of null and timelike particles yields the photon-sphere radius, shadow radius, and innermost stable circular orbit, all modified by the Lorentz-violating parameter and the dyonic charges. In the extended phase space the thermodynamic quantities satisfy the first law and the Smarr relation, and the system exhibits a first-order phase transition between小黑
What carries the argument
The nonminimal coupling term between the Kalb-Ramond field and the electromagnetic field, which permits the exact closed-form dyonic metric while preserving the static spherically symmetric ansatz.
If this is right
- The shadow radius is modified by the Lorentz-violating parameter and the dyonic charges.
- The domain of stable circular motion for timelike particles depends on the Lorentz-violating parameter and the dyonic charges.
- The first law of black hole thermodynamics and the Smarr relation hold in the extended phase space.
- A first-order phase transition occurs between small and large black holes and is influenced by the Lorentz-violating parameter and the dyonic charges.
Where Pith is reading between the lines
- The explicit dependence of shadow size on the Lorentz-violating parameter offers a potential route to constrain such violations using future very-long-baseline interferometry observations.
- The same nonminimal coupling strategy could be tested in other background-field models to generate additional exact solutions.
- The parameter-dependent phase transition may link to questions of black-hole stability during early-universe evolution when similar fields are present.
Load-bearing premise
The nonminimal coupling between the Kalb-Ramond field and the electromagnetic field is assumed to permit an exact closed-form solution for the dyonic metric while preserving the static spherically symmetric ansatz.
What would settle it
Substituting the proposed metric, electromagnetic potential, and Kalb-Ramond background into the modified field equations and verifying whether they hold identically for the chosen nonminimal coupling.
read the original abstract
By introducing a nonminimal coupling between the Kalb--Ramond field and the electromagnetic field, we construct an exact four-dimensional static, spherically symmetric dyonic black hole solution in Lorentz-violating gravity with a background Kalb--Ramond field. The curvature invariants show that the spacetime retains a genuine curvature singularity at $r=0$. We then analyze the geodesic motion of null and timelike particles and obtain the photon-sphere radius, the shadow radius, and the innermost stable circular orbit, demonstrating that both the Lorentz-violating parameter and the dyonic charges can appreciably modify the shadow size and the domain of stable circular motion. In the extended phase space, we derive the thermodynamic quantities and verify the first law of black hole thermodynamics together with the Smarr relation. The system also exhibits a first-order phase transition between small and large black holes, and its phase structure is strongly influenced by the Lorentz-violating parameter and the dyonic charges.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The manuscript introduces a nonminimal coupling between the Kalb-Ramond field and the electromagnetic field to construct an exact four-dimensional static spherically symmetric dyonic black hole solution in Lorentz-violating gravity with a background Kalb-Ramond field. It verifies that curvature invariants exhibit a genuine singularity at r=0, computes geodesic quantities including the photon-sphere radius, shadow radius, and ISCO for null and timelike particles, and derives thermodynamic quantities in extended phase space to confirm the first law, Smarr relation, and a first-order phase transition between small and large black holes whose structure depends on the Lorentz-violating parameter and dyonic charges.
Significance. If the exact solution is shown to satisfy the full set of modified field equations, the work supplies a concrete example of how Lorentz violation combined with a Kalb-Ramond background and dyonic charges alters observable features such as shadow size and the domain of stable orbits, as well as the thermodynamic phase structure. The explicit verification of the first law and Smarr relation in the presence of the new parameters strengthens the thermodynamic analysis.
major comments (2)
- [§2] §2 (action and field equations): The nonminimal coupling term between the Kalb-Ramond field and the electromagnetic field is introduced to permit an exact dyonic solution, yet the manuscript does not display the component-by-component substitution of the assumed metric, dyonic vector potential, and background Kalb-Ramond vev into the modified Einstein equations. Without this explicit check, it remains unclear whether the coupling cancels all angular or radial source terms that would otherwise violate the static spherically symmetric ansatz when both electric and magnetic charges are nonzero.
- [§3] §3 (metric and curvature invariants): The curvature invariants are stated to confirm a genuine singularity at r=0, but the explicit expressions for the metric functions (including the dependence on the Lorentz-violating parameter and the two charges) are not accompanied by the algebraic steps that solve the modified field equations. This verification is load-bearing for the central claim of an exact closed-form solution.
minor comments (2)
- [Abstract] The abstract and introduction refer to the nonminimal coupling without specifying its precise tensorial form (e.g., the contraction involving B_{μν}F^{μν}); adding the explicit Lagrangian term would improve readability.
- Figure captions for the shadow and phase-transition plots should explicitly state the fixed values of the Lorentz-violating parameter and the two charges used in each panel.
Simulated Author's Rebuttal
We thank the referee for the careful reading of our manuscript and the constructive comments. We address each major comment below and indicate the revisions we plan to implement.
read point-by-point responses
-
Referee: [§2] §2 (action and field equations): The nonminimal coupling term between the Kalb-Ramond field and the electromagnetic field is introduced to permit an exact dyonic solution, yet the manuscript does not display the component-by-component substitution of the assumed metric, dyonic vector potential, and background Kalb-Ramond vev into the modified Einstein equations. Without this explicit check, it remains unclear whether the coupling cancels all angular or radial source terms that would otherwise violate the static spherically symmetric ansatz when both electric and magnetic charges are nonzero.
Authors: We agree that an explicit component-by-component verification would improve clarity. In the revised manuscript we will add an appendix that substitutes the static spherically symmetric metric, the dyonic electromagnetic potential, and the background Kalb-Ramond vacuum expectation value into the modified Einstein equations, showing term-by-term cancellation of all non-spherically-symmetric source terms due to the nonminimal coupling. revision: yes
-
Referee: [§3] §3 (metric and curvature invariants): The curvature invariants are stated to confirm a genuine singularity at r=0, but the explicit expressions for the metric functions (including the dependence on the Lorentz-violating parameter and the two charges) are not accompanied by the algebraic steps that solve the modified field equations. This verification is load-bearing for the central claim of an exact closed-form solution.
Authors: We acknowledge that the algebraic steps leading to the closed-form metric functions should be shown explicitly. We will insert these intermediate steps into §3 (or a dedicated subsection) of the revised manuscript so that the dependence on the Lorentz-violating parameter and the dyonic charges is derived transparently from the field equations. revision: yes
Circularity Check
No significant circularity: exact solution constructed via ansatz and modified field equations
full rationale
The paper introduces a nonminimal coupling in the gravitational action specifically to admit an exact static spherically symmetric dyonic solution with a fixed background Kalb-Ramond field. The metric, electromagnetic potential, and KR field are posited as ansatzes, the modified Einstein and matter field equations are solved for the metric functions, and the resulting spacetime is then used to compute geodesics, shadow radius, and thermodynamic quantities. The first law and Smarr relation are verified as consistency checks on the obtained solution rather than as independent predictions. No parameter is fitted to data and then relabeled as a prediction, no uniqueness theorem is imported from self-citation to forbid alternatives, and no ansatz is smuggled through prior work. The derivation chain is self-contained against the chosen action and ansatz.
Axiom & Free-Parameter Ledger
free parameters (2)
- Lorentz-violating parameter
- Nonminimal coupling constant
axioms (2)
- domain assumption The metric ansatz is static and spherically symmetric in four dimensions
- domain assumption Extended phase space thermodynamics applies with cosmological constant as pressure
invented entities (1)
-
Background Kalb-Ramond field
no independent evidence
Lean theorems connected to this paper
-
IndisputableMonolith/Foundation/RealityFromDistinction.leanreality_from_one_distinction unclear?
unclearRelation between the paper passage and the cited Recognition theorem.
By introducing a nonminimal coupling between the Kalb–Ramond field and the electromagnetic field, we construct an exact four-dimensional static, spherically symmetric dyonic black hole solution
-
IndisputableMonolith/Cost/FunctionalEquation.leanwashburn_uniqueness_aczel unclear?
unclearRelation between the paper passage and the cited Recognition theorem.
the exact solution for the metric function is F(r) = 1/(1−ℓ) − 2M/r + Q²/((1−ℓ)² r²) + p²/((1−2ℓ) r²)
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]
N.D. Birrell and P.C.W. Davies,Quantum Fields in Curved Space, Cambridge Monographs on Mathematical Physics, Cambridge University Press, Cambridge (1982)
work page 1982
-
[2]
Maldacena,The large-n limit of superconformal field theories and supergravity,Int
J. Maldacena,The large-n limit of superconformal field theories and supergravity,Int. J. Theor. Phys.38(1999) 1113
work page 1999
-
[3]
O. Aharony, S.S. Gubser, J. Maldacena, H. Ooguri and Y. Oz,Large n field theories, string theory and gravity,Phys. Rep.323(2000) 183
work page 2000
- [4]
-
[5]
J. Alfaro, H.A. Morales-Técotl and L.F. Urrutia,Quantum gravity corrections to neutrino propagation,Phys. Rev. Lett.84(2000) 2318
work page 2000
-
[6]
J. Alfaro, H.A. Morales-Técotl and L.F. Urrutia,Loop quantum gravity and light propagation, Phys. Rev. D65(2002) 103509
work page 2002
-
[7]
C. Rovelli and L. Smolin,Loop space representation of quantum general relativity,Nucl. Phys. B331(1990) 80
work page 1990
-
[8]
V.A. Kostelecký and S. Samuel,Spontaneous breaking of lorentz symmetry in string theory, Phys. Rev. D39(1989) 683
work page 1989
-
[9]
D. Colladay and V.A. Kostelecký,CPTviolation and the standard model,Phys. Rev. D55 (1997) 6760
work page 1997
-
[10]
D. Colladay and V.A. Kostelecký,Lorentz-violating extension of the standard model,Phys. Rev. D58(1998) 116002
work page 1998
-
[11]
Kostelecký,Gravity, lorentz violation, and the standard model,Phys
V.A. Kostelecký,Gravity, lorentz violation, and the standard model,Phys. Rev. D69(2004) 105009
work page 2004
-
[12]
V.A. Kostelecký and N. Russell,Data tables for lorentz andcptviolation,Rev. Mod. Phys.83 (2011) 11
work page 2011
-
[13]
Tasson,What do we know about lorentz invariance?,Rep
J.D. Tasson,What do we know about lorentz invariance?,Rep. Prog. Phys.77(2014) 062901
work page 2014
-
[14]
Liberati,Tests of lorentz invariance: a 2013 update,Class
S. Liberati,Tests of lorentz invariance: a 2013 update,Class. Quantum Grav.30(2013) 133001
work page 2013
-
[15]
Q.G. Bailey and V.A. Kostelecký,Signals for lorentz violation in post-newtonian gravity,Phys. Rev. D74(2006) 045001. – 25 –
work page 2006
-
[16]
V.A. Kostelecký and J.D. Tasson,Prospects for large relativity violations in matter-gravity couplings,Phys. Rev. Lett.102(2009) 010402
work page 2009
-
[17]
V.A. Kostelecký and J.D. Tasson,Matter-gravity couplings and lorentz violation,Phys. Rev. D 83(2011) 016013
work page 2011
-
[18]
V.A. Kostelecký and M. Mewes,Electrodynamics with lorentz-violating operators of arbitrary dimension,Phys. Rev. D80(2009) 015020
work page 2009
-
[19]
A. Hees, Q. Bailey, A. Bourgoin, H. Pihan-Le Bars, C. Guerlin and C. Le Poncin-Lafitte,Tests of lorentz symmetry in the gravitational sector,Universe2(2016) 30
work page 2016
-
[20]
L. Shao,Tests of local lorentz invariance violation of gravity in the standard model extension with pulsars,Phys. Rev. Lett.112(2014) 111103
work page 2014
-
[21]
R. Bluhm and V.A. Kostelecký,Spontaneous lorentz violation, nambu-goldstone modes, and gravity,Phys. Rev. D71(2005) 065008
work page 2005
-
[22]
Nambu-Goldstone Modes in Gravitational Theories with Spontaneous Lorentz Breaking
R. Bluhm,Nambu-goldstone modes in gravitational theories with spontaneous lorentz breaking, Int. J. Mod. Phys. D16(2008) 2357 [hep-th/0607127]
work page internal anchor Pith review Pith/arXiv arXiv 2008
-
[23]
O. Bertolami and J. Páramos,Vacuum solutions of a gravity model with vector-induced spontaneous lorentz symmetry breaking,Phys. Rev. D72(2005) 044001
work page 2005
- [24]
-
[25]
R.V. Maluf and J.C.S. Neves,Black holes with a cosmological constant in bumblebee gravity, Phys. Rev. D103(2021) 044002
work page 2021
-
[26]
C. Ding, C. Liu, R. Casana and A. Cavalcante,Exact kerr-like solution and its shadow in a gravity model with spontaneous lorentz symmetry breaking,Eur. Phys. J. C80(2020) 178
work page 2020
-
[27]
C. Ding and X. Chen,Slowly rotating einstein-bumblebee black hole solution and its greybody factor in a lorentz violation model,Chin. Phys. C45(2021) 025106
work page 2021
-
[28]
İ. Güllü and A. Övgün,Schwarzschild-like black hole with a topological defect in bumblebee gravity,Ann. Phys.436(2022) 168721
work page 2022
- [29]
-
[30]
C. Ding, Y. Shi, J. Chen, Y. Zhou and C. Liu,High dimensional ads-like black hole and phase transition in einstein-bumblebee gravity,Chin. Phys. C47(2023) 045102
work page 2023
- [31]
-
[32]
S. Li, L. Liang and L. Ma,Dyonic rn-like and taub-nut-like black holes in einstein-bumblebee gravity,JCAP2026(2026) 005
work page 2026
- [33]
-
[34]
X.-M. Kuang and A. Övgün,Strong gravitational lensing and shadow constraint from m87* of slowly rotating kerr-like black hole,Ann. Phys.447(2022) 169147 [2205.11003]. – 26 –
-
[35]
Quasi-normal modes of bumblebee wormhole
R. Oliveira, D.M. Dantas, V. Santos and C.A.S. Almeida,Quasinormal modes of bumblebee wormhole,Class. Quant. Grav.36(2019) 105013 [1812.01798]
work page internal anchor Pith review Pith/arXiv arXiv 2019
- [36]
-
[37]
D.A. Gomes, R.V. Maluf and C.A.S. Almeida,Thermodynamics of schwarzschild-like black holes in modified gravity models,Ann. Phys.418(2020) 168198 [1811.08503]
-
[38]
S. Kanzi and İ. Sakallı,Gup modified hawking radiation in bumblebee gravity,Nucl. Phys. B 946(2019) 114703 [1905.00477]
-
[39]
R. Oliveira, D.M. Dantas and C.A.S. Almeida,Quasinormal frequencies for a black hole in a bumblebee gravity,EPL135(2021) 10003 [2105.07956]
-
[40]
S. Kanzi and İ. Sakallı,Greybody radiation and quasinormal modes of kerr-like black hole in bumblebee gravity model,Eur. Phys. J. C81(2021) 501 [2102.06303]
-
[41]
A. Övgün, K. Jusufi and İ. Sakallı,Gravitational lensing under the effect of weyl and bumblebee gravities: Applications of gauss–bonnet theorem,Ann. Phys.399(2018) 193 [1805.09431]
work page internal anchor Pith review Pith/arXiv arXiv 2018
-
[42]
İ. Sakallı and E. Yörük,Modified hawking radiation of schwarzschild-like black hole in bumblebee gravity model,Phys. Scr.98(2023) 125307
work page 2023
- [43]
- [44]
-
[45]
M. Kalb and P. Ramond,Classical direct interstring action,Phys. Rev. D9(1974) 2273
work page 1974
- [46]
-
[47]
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(2023)
work page 2023
-
[48]
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(2020) 335
work page 2020
-
[49]
Y. Sekhmani, A. Al-Badawi, M. Fathi, A. Vachher, S.G. Ghosh, M. Shahzadi et al.,Rotating and traversable wormhole solutions in kalb–ramond gravity,Eur. Phys. J. C86(2026) 160 [2508.06793]
-
[50]
Z.-Q. Duan, Y.-Z. Chen, Q. Yu, K. Yang and J.-Y. Zhao,Electrically charged black holes in gravity with a background kalb-ramond field,Phys. Lett. B856(2024) 138915
work page 2024
-
[51]
Y. Sekhmani, A. Al-Badawi, M. Fathi, A. Vachher and S.G. Ghosh,Black hole solutions surrounded by an anisotropic fluid in a kalb–ramond two–form background,2603.07052
-
[52]
W. Liu, D. Wu and J. Wang,Shadow of slowly rotating kalb–ramond black holes,JCAP05 (2025) 017. – 27 –
work page 2025
- [53]
- [54]
-
[55]
E.L.B. Junior, J.T.S.S. Junior, F.S.N. Lobo, M.E. Rodrigues, D. Rubiera-Garcia, L.F.D. da Silva et al.,Spontaneous lorentz symmetry-breaking constraints in kalb–ramond gravity,Eur. Phys. J. C84(2024) 1257 [2405.03291]
-
[56]
S. Jumaniyozov, S.U. Khan, J. Rayimbaev, A. Abdujabbarov, S. Urinbaev and S. Murodov, Circular motion and qpos near black holes in kalb–ramond gravity,Eur. Phys. J. C84(2024) 964
work page 2024
-
[57]
Y. Ma, S. Zheng, H. Li and B. Li,Schottky anomaly of the kalb–ramond-de sitter spacetime, Nucl. Phys. B1009(2024) 116732
work page 2024
-
[58]
A. Al-Badawi, S. Shaymatov and I. Sakallı,Geodesics structure and deflection angle of electrically charged black holes in gravity with a background kalb–ramond field,Eur. Phys. J. C 84(2024) 825 [2408.09228]
- [59]
- [60]
-
[61]
F. Atamurotov, D. Ortiqboev, A. Abdujabbarov and G. Mustafa,Particle dynamics and gravitational weak lensing around black hole in the kalb–ramond gravity,Eur. Phys. J. C82 (2022) 659
work page 2022
- [62]
-
[63]
S.K. Jha,Observational signature of lorentz violation in kalb-ramond field model and bumblebee model: A comprehensive comparative study,Int. J. Mod. Phys. D34(2025) 2550055 [2404.15808]
-
[64]
Black hole with global monopole charge in self-interacting Kalb-Ramond field,
M. Fathi and A. Övgün,Black hole with global monopole charge in self-interacting kalb–ramond field,Eur. Phys. J. Plus140(2025) 280 [2501.09899]
-
[65]
A.A.A. Filho, J.A.A.S. Reis and H. Hassanabadi,Exploring antisymmetric tensor effects on black hole shadows and quasinormal frequencies,JCAP05(2024) 029 [2309.15778]
-
[66]
Filho,Particle creation and evaporation in kalb-ramond gravity,JCAP04(2025) 076 [2411.06841]
A.A.A. Filho,Particle creation and evaporation in kalb-ramond gravity,JCAP04(2025) 076 [2411.06841]
-
[67]
F. Hosseinifar, A.A.A. Filho, M.Y. Zhang, H. Chen and H. Hassanabadi,Shadows, greybody factors, emission rate, topological charge, and phase transitions for a charged black hole with a kalb–ramond field background,2407.07017. – 28 –
-
[68]
R. Kumar, S.G. Ghosh and A. Wang,Gravitational deflection of light and shadow cast by rotating kalb-ramond black holes,Phys. Rev. D101(2020) 104001
work page 2020
- [69]
-
[70]
B. Altschul, Q.G. Bailey and V.A. Kostelecký,Lorentz violation with an antisymmetric tensor, Phys. Rev. D81(2010) 065028
work page 2010
-
[71]
R. Bluhm, S.-H. Fung and V.A. Kostelecký,Spontaneous lorentz and diffeomorphism violation, massive modes, and gravity,Phys. Rev. D77(2008) 065020
work page 2008
-
[72]
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(2023) 124004 [2308.06613]
-
[73]
S.M. Carroll,Spacetime and Geometry: An Introduction to General Relativity, Cambridge University Press, Cambridge, 3rd ed. (2019)
work page 2019
-
[74]
Bekenstein,Black holes and entropy,Phys
J.D. Bekenstein,Black holes and entropy,Phys. Rev. D7(1973) 2333
work page 1973
-
[75]
J.M. Bardeen, B. Carter and S.W. Hawking,The four laws of black hole mechanics,Commun. Math. Phys.31(1973) 161
work page 1973
-
[76]
Hawking,Particle creation by black holes,Commun
S.W. Hawking,Particle creation by black holes,Commun. Math. Phys.43(1975) 199
work page 1975
-
[77]
Enthalpy and the Mechanics of AdS Black Holes
D. Kastor, S. Ray and J. Traschen,Enthalpy and the mechanics of ads black holes,Class. Quantum Grav.26(2009) 195011 [0904.2765]
work page internal anchor Pith review Pith/arXiv arXiv 2009
-
[78]
Pressure and volume in the first law of black hole thermodynamics
B.P. Dolan,The cosmological constant and the black hole equation of state,Class. Quantum Grav.28(2011) 235017 [1106.6260]
work page internal anchor Pith review Pith/arXiv arXiv 2011
-
[79]
Black Hole Enthalpy and an Entropy Inequality for the Thermodynamic Volume
M. Cvetič, G.W. Gibbons, D. Kubizňák and C.N. Pope,Black hole enthalpy and an entropy inequality for the thermodynamic volume,Phys. Rev. D84(2011) 024037 [1012.2888]
work page internal anchor Pith review Pith/arXiv arXiv 2011
-
[80]
P-V criticality of charged AdS black holes
D. Kubizňák and R.B. Mann,p−vcriticality of charged ads black holes,JHEP2012(2012) 1 [1205.0559]
work page internal anchor Pith review Pith/arXiv arXiv 2012
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.