Quasinormal modes and thermodynamics of linearly charged BTZ black holes in massive gravity in (anti) de Sitter space-time

The European Physical Journal C

P. Prasia¹  V. C. Kuriakose¹ 

[1] Department of Physics, Cochin University of Science and Technology, 682022, Kochi, India;

关键词: Black Hole;    Massive Parameter;    Black Hole Solution;    Massive Gravity;    Quasinormal Mode;   

DOI  :  10.1140/epjc/s10052-016-4591-x

来源: Springer

【 摘 要 】

In this work we study the Quasi-Normal Modes (QNMs) under massless scalar perturbations and the thermodynamics of linearly charged BTZ black holes in massive gravity in the (Anti)de Sitter ((A)dS) space-time. It is found that the behavior of QNMs changes with the massive parameter of the graviton and also with the charge of the black hole. The thermodynamics of such black holes in the (A)dS space-time is also analyzed in detail. The behavior of specific heat with temperature for such black holes gives an indication of a phase transition that depends on the massive parameter of the graviton and also on the charge of the black hole.

【 授权许可】

CC BY