Dyonic Black Holes in Lorentz-Violating Gravity with a Background Kalb--Ramond Field
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.
Versions
Related
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BibTeX
@misc{lin2026dyonic,
title = {{Dyonic Black Holes in Lorentz-Violating Gravity with a Background Kalb--Ramond Field}},
author = {Yu-Xuan Lin and Jia-Zhou Liu and Yu-Xiao Liu},
howpublished = {arXiv},
year = {2026},
month = may,
doi = {10.48550/arxiv.2605.18371},
eprint = {2605.18371},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2605.18371},
}
RIS
TY - UNPB
TI - Dyonic Black Holes in Lorentz-Violating Gravity with a Background Kalb--Ramond Field
AU - Yu-Xuan Lin
AU - Jia-Zhou Liu
AU - Yu-Xiao Liu
PY - 2026
DA - 2026/05/18
PB - arXiv
DO - 10.48550/arxiv.2605.18371
UR - https://arxiv.org/abs/2605.18371
AB - 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.
ER -