The non-Kerr black hole with acceleration

Abstract

The no-hair theorem can be tested in the strong gravity regime by using the top-bottom approach and the bottom-top approach. The non-Kerr spacetime of the later approach is an ideal framework to do the tests in the region very close to the black holes. In this work, we propose a non-Kerr black hole metric (and its charged extension) that is accelerating as well. These new objects are studied for their basic properties and thermodynamics.

References in corpus (4)

• A Metric for Rapidly Spinning Black Holes Suitable for Strong-Field Tests of the No-Hair Theorem
• Tunneling of Dirac particles from accelerating and rotating black holes
• Radiation generated by accelerating and rotating charged black holes in (anti-)de Sitter space
• Quantum corrections to the entropy of Einstein-Maxwell dilaton-axion black holes