Thermodynamics of accelerating and rotating black holes

Abstract

Thermodynamics of a large family of black holes from electrovacuum solutions of Einstein's equations is studied. This family includes rotating and non-accelerating black holes with NUT charge, and rotating and accelerating black holes. The surface gravity, Hawking temperature and the area laws for these black holes are presented. The first law of thermodynamics is also given. An interesting outcome of our analysis is the restriction obtained on the magnitude of acceleration for these black holes.

References in corpus (6)

• Accelerating Kerr-Newman black holes in (anti-)de Sitter space-time
• Tunneling of Dirac particles from accelerating and rotating black holes
• Charged fermions tunneling from accelerating and rotating black holes
• Radiation generated by accelerating and rotating charged black holes in (anti-)de Sitter space
• The Disjointed Thermodynamics of Rotating Black Holes With a NUT Twist
• Quantum corrections to the entropy of charged rotating black holes

Cited by in corpus (11)

• Thermodynamics of Regular Accelerating Black Holes
• Chaotic motion of particles in the accelerating and rotating black holes spacetime
• Thermodynamical hairs of the four-dimensional Taub-Newman-Unti-Tamburino spacetimes
• Tunneling of Dirac particles from accelerating and rotating black holes
• Charged fermions tunneling from accelerating and rotating black holes
• Thermal Stability, P-V Criticality and Heat Engine of Charged Rotating Accelerating Black Holes
• Fermions Tunneling from Plebanski-Demianski Black Holes
• Entropy Bound of Horizons for Accelerating, Rotating and Charged Plebanski-Demianski Black Hole
• Hawking radiation of scalars from charged accelerating and rotating black holes with NUT parameter
• The quasilocal energy and thermodynamic first law in accelerating AdS black holes
• The non-Kerr black hole with acceleration