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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… Click to show full 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.
Keywords:
van der;
der waals;
kerr newman;
black hole;
rotating van;
newman black
Journal Title: General Relativity and Gravitation
Year Published: 2020
Link to full text (if available)
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Journal Title: General Relativity and Gravitation
Year Published: 2020
Link to full text (if available)
Share on Social Media: Sign Up to like & get
recommendations!