RUS  ENG
Full version
JOURNALS // Teoreticheskaya i Matematicheskaya Fizika // Archive

TMF, 2023 Volume 217, Number 1, Pages 3–18 (Mi tmf10407)

This article is cited in 1 paper

Noether charge, thermodynamics and phase transition of a black hole in the Schwarzschild–anti-de Sitter–Beltrami spacetime

T. Angsachon, K. Ruenearom

Division of Physics, Faculty of Science and Technology, Thammasat University, Bangkok, Thailand

Abstract: We investigate the thermodynamic properties and Hawking–Page phase transition of a black hole in the Schwarzschild–anti-de Sitter–Beltrami (SAdSB) spacetime. We discuss the Beltrami, or inertial, coordinates of the anti-de Sitter (AdS) spacetime. A transformation between noninertial and inertial coordinates of the AdS spacetime is formulated in order to construct a solution of a spherical gravitating mass and other physical quantities. The Killing vector is determined and used to calculate the event horizon radius of this black hole. The SAdSB black hole entropy and temperature are determined by the Noether charge method; the temperature is shown to be bounded by the AdS radius. Similarly, the Smarr relation and the first law of black hole thermodynamics for the SAdSB spacetime are formulated. The Gibbs free energy and heat capacity of this black hole are calculated and the phase transition between small and large black holes is considered. A first-order phase transition between the thermal AdS spacetime and the large-black-hole phase is also investigated and the Hawking–Page temperature is computed and compared with that of the Schwarzschild-anti-de Sitter black hole.

Keywords: black hole thermodynamics, anti-de Sitter–Beltrami spacetime, Iyer–Wald entropy, phase transition.

Received: 19.11.2022
Revised: 03.07.2023

DOI: 10.4213/tmf10407


 English version:
Theoretical and Mathematical Physics, 2023, 217:1, 1423–1436

Bibliographic databases:


© Steklov Math. Inst. of RAS, 2024