Spin effects on particle creation and evaporation in $f(R,T)$ gravity

Fuente: arXiv
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Autori principali: Filho, A. A. Araújo, Heidari, N., Lobo, Francisco S. N.
Natura: Preprint
Pubblicazione: 2025
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author Filho, A. A. Araújo
Heidari, N.
Lobo, Francisco S. N.
author_facet Filho, A. A. Araújo
Heidari, N.
Lobo, Francisco S. N.
contents In this work, we study how the spin of particle modes influences particle creation, greybody factors, absorption, and evaporation of a black hole within the framework of modified electrodynamics in $f(R,T)$ gravity, recently proposed in Ref. [1]. All spin sectors -- scalar, vector, tensor, and spinorial -- are analyzed to obtain the corresponding features. For particle creation, we consider massless bosonic and fermionic perturbations to determine the respective particle densities. Analytical expressions for the greybody factors are derived, with suitable approximations for the tensor and spinorial cases. The absorption cross section is computed numerically, and using the Stefan-Boltzmann law, we estimate the black hole evaporation lifetime. The associated energy and particle emission rates are also discussed, along with the correspondence between quasinormal modes and greybody factors.
format Preprint
id arxiv_https___arxiv_org_abs_2510_25973
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Spin effects on particle creation and evaporation in $f(R,T)$ gravity
Filho, A. A. Araújo
Heidari, N.
Lobo, Francisco S. N.
General Relativity and Quantum Cosmology
High Energy Physics - Theory
In this work, we study how the spin of particle modes influences particle creation, greybody factors, absorption, and evaporation of a black hole within the framework of modified electrodynamics in $f(R,T)$ gravity, recently proposed in Ref. [1]. All spin sectors -- scalar, vector, tensor, and spinorial -- are analyzed to obtain the corresponding features. For particle creation, we consider massless bosonic and fermionic perturbations to determine the respective particle densities. Analytical expressions for the greybody factors are derived, with suitable approximations for the tensor and spinorial cases. The absorption cross section is computed numerically, and using the Stefan-Boltzmann law, we estimate the black hole evaporation lifetime. The associated energy and particle emission rates are also discussed, along with the correspondence between quasinormal modes and greybody factors.
title Spin effects on particle creation and evaporation in $f(R,T)$ gravity
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2510.25973