Restricted Phased Space Thermodynamics for Black Holes in Higher Dimensions and Higher Curvature Gravities.

Euler homogeneity T − S phase transitions black hole thermodynamics higher curvature gravity higher dimensional gravity restricted phase space formalism

Journal

Entropy (Basel, Switzerland)
ISSN: 1099-4300
Titre abrégé: Entropy (Basel)
Pays: Switzerland
ID NLM: 101243874

Informations de publication

Date de publication:
16 Aug 2022
Historique:
received: 25 07 2022
revised: 10 08 2022
accepted: 12 08 2022
entrez: 26 8 2022
pubmed: 27 8 2022
medline: 27 8 2022
Statut: epublish

Résumé

The recently proposed restricted phase space thermodynamics is shown to be applicable to a large class of higher dimensional higher curvature gravity models coupled to Maxwell field, which are known as black hole scan models and are labeled by the spacetime dimension

Identifiants

pubmed: 36010795
pii: e24081131
doi: 10.3390/e24081131
pmc: PMC9407627
pii:
doi:

Types de publication

Journal Article

Langues

eng

Subventions

Organisme : National Natural Science Foundation of China
ID : 11575088

Références

Phys Rev D Part Fields. 1993 Oct 15;48(8):R3427-R3431
pubmed: 10016675
Phys Rev D Part Fields. 1994 Jul 15;50(2):846-864
pubmed: 10017782
Phys Rev Lett. 2021 Aug 27;127(9):091301
pubmed: 34506158
Phys Rev D Part Fields. 1986 Apr 15;33(8):2092-2099
pubmed: 9956880

Auteurs

Xiangqing Kong (X)

School of Physics, Nankai University, Tianjin 300071, China.

Tao Wang (T)

School of Physics, Nankai University, Tianjin 300071, China.

Zeyuan Gao (Z)

School of Physics, Nankai University, Tianjin 300071, China.

Liu Zhao (L)

School of Physics, Nankai University, Tianjin 300071, China.

Classifications MeSH