Analytic explanation of the strong spin-dependent amplification in Hawking radiation from rotating black holes

DOI10.1007/JHEP08(2010)016zbMath1291.83135arXiv1008.4586OpenAlexW1978104581MaRDI QIDQ2248199

Dejan Stojkovic, De-Chang Dai

Publication date: 30 June 2014

Published in: Journal of High Energy Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1008.4586

zbMATH Keywords

black holesclassical theories of gravity

Mathematics Subject Classification ID

Black holes (83C57) Quantization of the gravitational field (83C45) Methods of quantum field theory in general relativity and gravitational theory (83C47)

Related Items (1)

Angular profile of particle emission from a higher-dimensional black hole: analytic results

Uses Software

• BlackMax

Cites Work

• Black hole superradiance from Kerr/CFT
• Condition for the superradiance modes in higher-dimensional rotating black holes with multiple angular momentum parameters
• Black hole physics. Basic concepts and new developments
• MOTION OF A GYROSCOPE ACCORDING TO EINSTEIN'S THEORY OF GRAVITATION
• Coherence in Spontaneous Radiation Processes
• Manual of BlackMax. A black-hole event generator with rotation, recoil, split branes, and brane tension. Version 2.02

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