Stability of horizon with pressure and volume of d-dimensional charged AdS black holes with cloud of strings and quintessence

TL;DR

This paper investigates the thermodynamic stability of charged AdS black holes in various dimensions, considering effects of quintessence, cloud of strings, and different assumptions about particle energy, using scalar field scattering and particle absorption methods.

Contribution

It introduces a comparative analysis of black hole stability under two energy assumptions and explores the influence of dimension, quintessence, and strings on thermodynamics.

Findings

Black hole stability varies with dimension and surrounding fields.

Different energy assumptions lead to distinct thermodynamic behaviors.

Thermodynamic properties are affected by quintessence and cloud of strings.

Abstract

In this paper, the thermodynamics and the stability of horizon of the charged AdS black hole surrounded by quintessence and cloud of strings in d-dimensional spacetime are studied via the scalar field scattering and the charged particle absorption. The cosmological constant is interpreted as a thermodynamics variable. During the study, we consider the case where the energy of the particle(scalar field) is related to the internal energy of the black hole. Furthermore, we also consider another assumption, which is proposed in [Phys. Rev. D 100, no.10, 104022 (2019)]. This assumption considers that the energy of the particle(scalar field) is related to the internal energy of the black hole. In addition, we compare and discuss the results obtained under these two assumptions. At the same time, we also considered the effect of the dimension. The thermodynamics of black holes in different dimensions has also been studied and compared.