2018/04/30 by Yan-Gang Miao, Zhen-Ming Xu · 29 citations
Mathematics · Physics and Astronomy · #Astrophysical Phenomena and Observations #Black Holes and Theoretical Physics #Black hole (networking) #Black hole thermodynamics #Charged black hole #Classical mechanics #Cosmology and Gravitation Theories #Curvature #Entropy (arrow of time) #Equation of state #Geometry #Gravitation #Gravitational collapse #Hawking radiation #Mathematics #Physics #Schwarzschild radius #Thermodynamics #White hole #gr-qc #hep-th
paper · pdf · doi:10.1007/s11433-018-9254-9
published in Science China Physics Mechanics and Astronomy 62(1) (Springer Science+Business Media) · v1: 11 pages, no figures; v2: minor revisions; v3: 12 pages, minor revisions, final version to appear in Science China Physics, Mechanics & Astronomy
arxiv created 2018/05/26 · arxiv updated 2018/08/07 · openalex publication_date 2018/08/08 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
The microscopic structure of black holes remains a challenging subject. In this paper, based on the well-accepted fact that black holes can be mapped to thermodynamic systems, we make a preliminary exploration of the microscopic structure of the thermodynamically stable Schwarzschild anti-de-Sitter (SAdS) black hole. In accordance with the number density and thermodynamic scalar curvature, we give the interaction potential among the molecules of thermodynamically stable SAdS black holes and analyze its effectiveness. Moreover, we derive the thermo-correction to the equation of state for such black holes that arises from interactions among black-hole molecules using virial coefficients.