Thermodynamics phase transition and Hawking radiation of the Schwarzschild black hole with quintessence-like matter and a deficit solid angle

DOI10.1007/s10714-018-2367-3zbMath1392.83055OpenAlexW2800614725WikidataQ129929381 ScholiaQ129929381MaRDI QIDQ725370

Kamiko Kouemeni Jean Rodrigue, Bouetou Bouetou Thomas, Mahamat Saleh, Timoléon Créprin Kofané

Publication date: 1 August 2018

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10714-018-2367-3

zbMATH Keywords

thermodynamicsphase transitionblack holequintessence-like matterdeficit solid angle

Mathematics Subject Classification ID

Black holes (83C57) Methods of quantum field theory in general relativity and gravitational theory (83C47) Classical and relativistic thermodynamics (80A10)

Related Items (5)

Quasinormal modes of nonlinearly charged black holes surrounded by a cloud of strings in Rastall gravity ⋮ Thermodynamic phase transition and global stability of the regular Hayward black hole surrounded by quintessence ⋮ Hawking radiation from cubic and quartic black holes via tunneling of GUP corrected scalar and fermion particles ⋮ The Reissner–Nordström black hole surrounded by quintessence and a cloud of strings: Thermodynamics and quasinormal modes ⋮ The Letelier spacetime with quintessence: Solution, thermodynamics and Hawking radiation

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