Exploring Lorentz-violating effects of Kalb-Ramond field on charged black hole thermodynamics and photon dynamics

This study explores the influence of the Kalb-Ramond (KR) field, characterized by Lorentz-violating effects, on the structure, thermodynamics, and observational phenomena of Reissner-Nordstr"om-like black holes. By introducing a modified Einstein-Hilbert action incorporating the KR field's nonminimal coupling with the \ifmmode \bar{\imath}\else \={\i}\fi{}Ricci tensor, we derive a spherically symmetric black hole solution. The Lorentz-violating parameter $L$ alters the black hole's horizon structure, curvature invariants, and thermodynamic properties, such as Hawking temperature and entropy, with exponential quantum corrections offering deeper insights into high-energy phenomena. Photon dynamics in both vacuum and plasma environments reveal refractive effects due to the KR field, with weak gravitational lensing analyzed using the Gauss-Bonnet theorem and perturbative methods, including higher-order deflection corrections. Observational signatures like modified photon spheres, lensing angles, and shadows are discussed, providing potential avenues for experimental validation.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2025-03-14
DOI
https://doi.org/10.1103/physrevd.111.064049
Citations
40
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
46.19

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article

Exploring Lorentz-violating effects of Kalb-Ramond field on charged black hole thermodynamics and photon dynamics

İzzet Sakallı, Erdem Sucu
40 citations
Physical review. D/Physical review. D.
Cosmology and Gravitation Theories
46.19
article

Exploring Lorentz-violating effects of Kalb-Ramond field on charged black hole thermodynamics and photon dynamics

İzzet Sakallı, Erdem Sucu
article en
40 citations

Abstract

This study explores the influence of the Kalb-Ramond (KR) field, characterized by Lorentz-violating effects, on the structure, thermodynamics, and observational phenomena of Reissner-Nordstr"om-like black holes. By introducing a modified Einstein-Hilbert action incorporating the KR field's nonminimal coupling with the \ifmmode \bar{\imath}\else \={\i}\fi{}Ricci tensor, we derive a spherically symmetric black hole solution. The Lorentz-violating parameter $L$ alters the black hole's horizon structure, curvature invariants, and thermodynamic properties, such as Hawking temperature and entropy, with exponential quantum corrections offering deeper insights into high-energy phenomena. Photon dynamics in both vacuum and plasma environments reveal refractive effects due to the KR field, with weak gravitational lensing analyzed using the Gauss-Bonnet theorem and perturbative methods, including higher-order deflection corrections. Observational signatures like modified photon spheres, lensing angles, and shadows are discussed, providing potential avenues for experimental validation.

Physical review. D/Physical review. D.Vol. 111(6)
Eastern Mediterranean University (CY)
Sponsoring Consortium for Open Access Publishing in Particle Physics, Türkiye Bilimsel ve Teknolojik Araştırma Kurumu
Affordable and clean energy
Openalex Percentile: Top 0%
Cosmology and Gravitation Theories
46.19
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