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

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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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Acknowledgements

P. B. dedicates this work to Anaís, Lucía, Inés and Ana for continuous support. P. B. is funded by the Beatriz Galindo contract BEAGAL 18/00207 (Spain). F. V. acknowledges funding by the Department of Physics of Universidad de los Andes. A.V is supported by a Melbourne Research Scholarship and the N.D. Goldsworthy Scholarship

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Authors and Affiliations

  1. Departamento de Física, Universidad de los Andes, Apartado Aéreo 4976, Bogotá, Distrito Capital, Colombia

    F. D. Villalba

  2. School of Physics, University of Melbourne, Parkville, VIC, 3010, Australia

    A. F. Vargas

  3. Departamento de Física, Colegio de Ciencias e Ingeriería, Universidad San Francisco de Quito, Quito, Ecuador

    E. Contreras

  4. Departamento de Física Aplicada, Universidad de Alicante, Campus de San Vicente del Raspeig, E-03690, Alicante, Spain

    Pedro Bargueño

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  1. F. D. Villalba
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  2. A. F. Vargas
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  3. E. Contreras
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  4. Pedro Bargueño
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Correspondence to Pedro Bargueño.

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Villalba, F.D., Vargas, A.F., Contreras, E. et al. The Kerr–Newman black hole as a rotating Van der Waals gas. Gen Relativ Gravit 52, 87 (2020). https://doi.org/10.1007/s10714-020-02739-2

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