ModMax-black hole surrounded by cloud of strings in Bumblebee gravity

TL;DR

This paper explores the optical, thermodynamic, and scattering characteristics of a ModMax black hole in Einstein-bumblebee gravity, analyzing how various parameters influence radiation and scattering phenomena.

Contribution

It provides a comprehensive analysis of how Lorentz violation, string clouds, and ModMax parameters affect black hole thermodynamics and scattering properties.

Findings

Thermodynamic quantities depend on system parameters.

Greybody factors vary with black hole parameters.

Optical and scattering features are influenced by Lorentz violation and string cloud parameters.

Abstract

In this article, we investigate the optical, thermodynamic, and scattering properties of a ModMax black hole surrounded by a cloud of strings within the framework of Einstein-bumblebee gravity. We then analyze in detail the thermodynamic properties of this black hole, including the Hawking temperature, entropy, and other relevant thermodynamic quantities, and examine the outcomes. Furthermore, we study the greybody factors (GFs) associated with the emission of various perturbative fields propagating in this black hole background. In particular, we consider spin-0 scalar fields, spin-1 electromagnetic fields, and spin-2 graviton fields, and evaluate the corresponding absorption probabilities and energy emission rates. Our analysis demonstrates how the optical features, thermodynamics and GFs depend on the underlying parameters of the system, such as the Lorentz symmetry violation parameter, the cloud of strings parameter, the ModMax parameter, the electric charge, and the black hole mass, thereby providing a comprehensive understanding of the physical effects of these parameters on the radiation and scattering processes around the black hole.