Microscopic explanation for black hole phase transitions via Ruppeiner geometry: two competing factors -- the temperature and repulsive interaction among BH molecules

DOI10.1016/j.nuclphysb.2019.114752zbMath1435.83079arXiv1812.11765OpenAlexW2972180630WikidataQ126011130 ScholiaQ126011130MaRDI QIDQ2186357

Yanyan Li

Publication date: 9 June 2020

Published in: Nuclear Physics. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1812.11765

Mathematics Subject Classification ID

Black holes (83C57) Quantization of the gravitational field (83C45) Phase transitions (general) in equilibrium statistical mechanics (82B26) Electromagnetic fields in general relativity and gravitational theory (83C50) Statistical thermodynamics (82B30)

Related Items (5)

Dynamic properties of thermodynamic phase transition for five-dimensional neutral Gauss-Bonnet AdS black hole on free energy landscape ⋮ 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 ⋮ Insight into the microstructure of FRW universe from a \(P\)-\(V\) phase transition ⋮ Microstructure of five-dimensional neutral Gauss-Bonnet black hole in anti-De Sitter spacetime via \(P-V\) criticality

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