Radiation generated by accelerating and rotating charged black holes in (anti-)de Sitter space

Abstract

Asymptotic behaviour of gravitational and electromagnetic fields of exact type D solutions from the large Plebanski-Demianski family of black hole spacetimes is analyzed. The amplitude and directional structure of radiation is evaluated in cases when the cosmological constant is non-vanishing, so that the conformal infinities have either de Sitter-like or anti-de Sitter-like character. In particular, explicit relations between the parameters that characterize the sources (that is their mass, electric and magnetic charges, NUT parameter, rotational parameter, and acceleration) and properties of the radiation generated by them are presented. The results further elucidate the physical interpretation of these solutions and may help to understand radiative characteristics of more general spacetimes than those that are asymptotically flat.

24 pages, 18 figures. To appear in Classical and Quantum Gravity

References in corpus (3)

• Accelerating Kerr-Newman black holes in (anti-)de Sitter space-time
• Radiation from accelerated black holes in an anti-de Sitter universe
• Gravitational and electromagnetic fields near a de Sitter-like infinity

Cited by in corpus (6)

• Tunneling of Dirac particles from accelerating and rotating black holes
• Charged fermions tunneling from accelerating and rotating black holes
• Dynamics and Fundamental Frequencies of Test Particles Orbiting Kerr-Newman-NUT-Kiselev Blacks Hole in Rastall Gravity
• Hawking radiation of scalar particles from accelerating and rotating black holes
• Deformed conformal symmetry of Kerr-Newman-NUT-AdS black holes
• The non-Kerr black hole with acceleration