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^*

^*Corresponding author for this work

Física

Universidad de los Andes Colombia
University of Melbourne
University of Alicante

Research output: Contribution to journal › Article › peer-review

4 Scopus citations

Abstract

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.

Original language	English
Article number	87
Journal	General Relativity and Gravitation
Volume	52
Issue number	9
DOIs	https://doi.org/10.1007/s10714-020-02739-2
State	Published - 1 Sep 2020

Keywords

Equation of state
Horizon thermodynamics
Kerr black hole

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10.1007/s10714-020-02739-2

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abstract = "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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AU - Contreras, E.

AU - Bargueño, Pedro

PY - 2020/9/1

Y1 - 2020/9/1

N2 - 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.

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.

KW - Equation of state

KW - Horizon thermodynamics

KW - Kerr black hole

UR - https://www.scopus.com/pages/publications/85091410624

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DO - 10.1007/s10714-020-02739-2

M3 - Artículo

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VL - 52

JO - General Relativity and Gravitation

JF - General Relativity and Gravitation

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ER -

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

Abstract

Keywords

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