Impact of antisymmetric tensor on charged black holes

Paper Title:

The impact of an antisymmetric tensor on charged black holes: evaporation process, geodesics, deflection angle, scattering effects and quasinormal modes

Published on:

16 April 2024

Primary Category:

General Relativity and Quantum Cosmology

Paper Authors:

A. A. Araújo Filho,

N. Heidari,

J. A. A. S. Reis,

H. Hassanabadi

Bullets

Key Details

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Analyzes horizons, geodesics for charged black holes with antisymmetric tensor

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Computes quasinormal modes and studies stability with vector perturbations

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Derives Hawking temperature and remnant mass after evaporation

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Estimates lifetime until final stage of evaporation process

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Explores emission rate and deflection angle of light

Explore the topics in this paper

black-holes

geodesics

hawking-radiation

horizons

lorentz-symmetry-breaking

AI generated summary

Impact of antisymmetric tensor on charged black holes

This paper investigates the influence of an antisymmetric tensor field, which triggers Lorentz symmetry breaking, on charged spherical black holes. It analyzes horizons, geodesics, quasinormal modes, Hawking temperature, remnant mass, lifetime, emission rate, deflection angle, and the correlation between quasinormal modes and shadows.