Thermodynamic stability of black holes in five-dimensional Yang-Mills massive gravity

被引:1
|
作者
Hendi, S. H. [1 ,2 ,3 ]
Nemati, A. [1 ,2 ]
机构
[1] Shiraz Univ, Sch Sci, Dept Phys, Shiraz, Iran
[2] Shiraz Univ, Sch Sci, Biruni Observ, Shiraz, Iran
[3] Canadian Quantum Res Ctr, 204-3002 32 Ave, Vernon, BC V1T 2L7, Canada
关键词
QUASI-NORMAL-MODES; PHASE-TRANSITION; MAXWELL;
D O I
10.1016/j.physletb.2023.138059
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper, we consider the Einstein-massive gravity coupled to the Yang-Mills gauge field in five dimensions. Concentrating on the static solutions with planar horizon geometry, we explore the thermodynamic behavior in the extended phase space and examine the validity of the first law of thermodynamics besides local thermal stability by the Hessian matrix. We observe that although the topology of boundary is planar, there exists the van der Waals like phase transition for this kind of solution. We find the critical quantities and discuss how the massive and Yang-Mills parameters affect them. Furthermore, some signatures of the first order phase transition such as the swallow-tail behavior of the Gibbs free energy and divergencies of the specific heat are given in detail.& COPY; 2023 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons .org /licenses /by /4 .0/). Funded by SCOAP3.
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页数:6
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