Joule-Thomson expansion in a mimetic black hole.

Joule–Thomson expansion Mimetic black hole Mimetic gravity Modified gravity

Journal

Scientific reports
ISSN: 2045-2322
Titre abrégé: Sci Rep
Pays: England
ID NLM: 101563288

Informations de publication

Date de publication:
22 Aug 2024
Historique:
received: 12 05 2024
accepted: 14 08 2024
medline: 23 8 2024
pubmed: 23 8 2024
entrez: 22 8 2024
Statut: epublish

Résumé

This paper investigates some implications of mimetic gravity on the black hole thermodynamics. We begin with an analysis of the mimetic action and its relationship to the spacetime curvature, highlighting the field equations and their contributions to the black hole solutions. Then we explore the behavior of various thermodynamic parameters including pressure, temperature and heat capacity, revealing some intriguing features of the system near the event horizon. We analyze also the inversion temperatures, inversion curves and the Joule-Thomson coefficients to enrich our comprehension of thermodynamic phenomena in this context. By extending coordinates close to the event horizon, we study the Joule-Thomson expansion, demonstrating how strong gravitational fields create pressure gradients similar to gas cooling processes. Comparison between mimetic black hole and Schwarzschild black hole in this setup provides a deeper understanding of the unique characteristics of the mimetic gravity.

Identifiants

pubmed: 39174665
doi: 10.1038/s41598-024-70308-7
pii: 10.1038/s41598-024-70308-7
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

19475

Informations de copyright

© 2024. The Author(s).

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Auteurs

Amir Hossein Rezaei (AH)

Department of Physics, Amirkabir University of Technology (Tehran Polytechnic), Tehran, Iran.

Kourosh Nozari (K)

Department of Theoretical Physics, Faculty of Sciences, University of Mazandaran, P. O. Box 47416-95447, Babolsar, Iran. knozari@umz.ac.ir.

Classifications MeSH