J 2025

Charged black holes in KR gravity: Weak deflection angle, shadow cast, quasinormal modes and neutrino annihilation

PANTIG, Reggie C; Ali OVGUN and Ángel Erasmo RINCÓN RIVERO

Basic information

Original name

Charged black holes in KR gravity: Weak deflection angle, shadow cast, quasinormal modes and neutrino annihilation

Authors

PANTIG, Reggie C; Ali OVGUN and Ángel Erasmo RINCÓN RIVERO

Edition

Physics of the Dark Universe, 2025, 2212-6864

Other information

Language

English

Type of outcome

Article in a journal

Field of Study

10308 Astronomy

Country of publisher

Netherlands

Confidentiality degree

is not subject to a state or trade secret

References:

Impact factor

Impact factor: 6.400 in 2024

Organization unit

Institute of physics in Opava

UT WoS

001546580500001

EID Scopus

2-s2.0-105012539387

Keywords in English

Black holes;Lorentz symmetry breaking;Kalb-Ramond;Weak deflection angle;Neutrino annihilation;Quasinormal modes

Tags

Tags

International impact, Reviewed
Changed: 21/1/2026 14:25, Mgr. Pavlína Jalůvková

Abstract

In the original language

In this paper, we investigate the phenomenology of electrically charged black holes in a Lorentz-violating gravitational framework mediated by a background Kalb-Ramond (KR) antisymmetric tensor field. Employing the Gauss-Bonnet theorem (GBT) in a non-asymptotically flat geometry, we derive analytic expressions for the weak deflection angle of light and massive particles, revealing persistent corrections due to the Lorentz-violating parameter 8. Scalar and Dirac perturbations are also studied using both the Wentzel-Kramers-Brillouin (WKB) approximation and the P & ouml;schl-Teller approximation approach to verify the stability of the solution against these types of perturbations. Shadow analysis further uncovers a nontrivial deformation of the photon sphere and critical impact parameter, with KR-induced effects modifying the charge contribution in a manner incompatible with standard Einstein-Maxwell theory. Constraints derived from the Event Horizon Telescope (EHT) data for Sgr A* and M87* validate the model and provide stringent bounds on 8, establishing the KR framework as an observationally testable extension of General Relativity (GR).