The Kerr–Newman black hole as a rotating Van der Waals gas

F. D. Villalba; A. F. Vargas; E. Contreras; Pedro Bargueño

doi:10.1007/s10714-020-02739-2

The Kerr–Newman black hole as a rotating Van der Waals gas

F. D. Villalba, A. F. Vargas, E. Contreras, Pedro Bargueño

Física

Producción científica: Contribución a una revista › Artículo › revisión exhaustiva

3 Citas (Scopus)

Resumen

In this work we employ the horizon approach for the thermodynamics of black holes, together with holographic equipartition, to show that the Kerr–Newman black hole can be considered as a rotating Van der Waals gas. Our results are interpreted in light of a simple mechanical and geometrical model, which is amenable to emerge from the space-time atom perspective.

Idioma original	Inglés
Número de artículo	87
Publicación	General Relativity and Gravitation
Volumen	52
N.º	9
DOI	https://doi.org/10.1007/s10714-020-02739-2
Estado	Publicada - 1 sep. 2020

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AU - Contreras, E.

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AB - In this work we employ the horizon approach for the thermodynamics of black holes, together with holographic equipartition, to show that the Kerr–Newman black hole can be considered as a rotating Van der Waals gas. Our results are interpreted in light of a simple mechanical and geometrical model, which is amenable to emerge from the space-time atom perspective.

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The Kerr–Newman black hole as a rotating Van der Waals gas

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