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

TL;DR

This paper investigates how particle spin affects black hole particle creation, greybody factors, and evaporation within $f(R,T)$ gravity, analyzing various spin sectors and deriving analytical and numerical results.

Contribution

It provides the first comprehensive analysis of spin effects on black hole phenomena in $f(R,T)$ gravity, including analytical expressions for greybody factors and evaporation estimates.

Findings

Analytical greybody factors derived for scalar, vector, tensor, and spinorial fields.

Numerical computation of absorption cross sections and evaporation lifetimes.

Demonstrates the influence of particle spin on black hole emission spectra.

Abstract

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.