Microscopic structures and thermal stability of black holes conformally coupled to scalar fields in five dimensions
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Publication:2423318
DOI10.1016/j.nuclphysb.2019.03.015zbMath1415.83020arXiv1711.01757OpenAlexW2895047692MaRDI QIDQ2423318
Publication date: 21 June 2019
Published in: Nuclear Physics. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1711.01757
Relativistic cosmology (83F05) Black holes (83C57) Methods of quantum field theory in general relativity and gravitational theory (83C47) Kaluza-Klein and other higher-dimensional theories (83E15) Statistical thermodynamics (82B30)
Related Items (13)
Dynamic properties of thermodynamic phase transition for five-dimensional neutral Gauss-Bonnet AdS black hole on free energy landscape ⋮ Thermodynamic geometry of black holes enclosed by a cavity in extended phase space ⋮ The correspondence between thermodynamic curvature and isoperimetric theorem from ultraspinning black hole ⋮ Repulsive interactions in the microstructure of regular Hayward black hole in anti-de Sitter spacetime ⋮ Microscopic explanation for black hole phase transitions via Ruppeiner geometry: two competing factors -- the temperature and repulsive interaction among BH molecules ⋮ Intriguing microstructures of five-dimensional neutral Gauss-Bonnet AdS black hole ⋮ Probing phase structure of black holes with Lyapunov exponents ⋮ The microstructure and Ruppeiner geometry of charged anti-de Sitter black holes in Gauss–Bonnet gravity: from the critical point to the triple point ⋮ Microstructure of five-dimensional neutral Gauss-Bonnet black hole in anti-De Sitter spacetime via \(P-V\) criticality ⋮ Photon orbits and phase transition for non-linear charged anti-de Sitter black holes ⋮ Coexistent physics and microstructure of the regular Bardeen black hole in anti-de Sitter spacetime ⋮ Joule-Thomson expansion for hairy black holes ⋮ Phase transition and entropic force in Reissner-Nordström-de Sitter spacetime
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