Ruppeiner geometry, PV criticality and interacting microstructures of black holes in dRGT massive gravity

Author:

Safir T. K.12,Rizwan C. L. Ahmed3,Vaid Deepak1

Affiliation:

1. Department of Physics, National Institute of Technology Karnataka, Surathkal 575025, India

2. Department of Physics, T. K. M. College of Arts and Science, Kollam, Kerala 691005, India

3. PG Department of Physics, Government College Kasaragod, Kerala, 671123, India

Abstract

We probe the microstructure of the dRGT massive black hole in an anti-de Sitter background. The calculations are performed in an extended phase space with pressure and volume taken as fluctuation variables. We analyze the microstructure by exploiting the Ruppeiner geometry, where the thermodynamic curvature scalar is constructed via adiabatic compressibility. The nature of the curvature scalar along the coexistence line of small black hole (SBH) and large black hole (LBH) is investigated. In the microscopic interaction, we observe that the SBH phase behaves as an anyonic gas and the LBH phase is analogous to a boson gas. Further, we study the effect of graviton mass on the underlying microstructure of the black hole.

Publisher

World Scientific Pub Co Pte Ltd

Subject

Astronomy and Astrophysics,Nuclear and High Energy Physics,Atomic and Molecular Physics, and Optics

Cited by 2 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Dynamic phase transition of black holes in massive gravity;Annals of Physics;2023-11

2. Topological nature of black hole solutions in dRGT massive gravity;International Journal of Modern Physics A;2023-09-10

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