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


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.

Año de publicación:

2020

Keywords:

  • Horizon thermodynamics
  • Equation of state
  • Kerr black hole

Fuente:

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scopusscopus

Tipo de documento:

Article

Estado:

Acceso restringido

Áreas de conocimiento:

  • Agujero negro
  • Física

Áreas temáticas:

  • Física