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Hawking radiation of Schwarzschild–de Sitter black hole by Hamilton–Jacobi method

2012/04/24 by M. Atiqur Rahman, M. Ilias Hossain · 1 citation
Physics and Astronomy · #Advanced Differential Geometry Research #Black Holes and Theoretical Physics #Black hole (networking) #Classical mechanics #Computer science #Cosmology and Gravitation Theories #De Sitter universe #General relativity #Gravitation #Gravitational wave #Hawking radiation #Mathematical physics #Physics #Quantum mechanics #Schwarzschild metric #Schwarzschild radius #Universe #de Sitter–Schwarzschild metric #gr-qc

paper · pdf · doi:10.1016/j.physletb.2012.04.049

published as Phys. Lett. B 712 (2012) 1-5 · 9 page. arXiv admin note: text overlap with arXiv:1205.1390

openalex publication_date 2012/04/24 · arxiv created 2012/05/13 · arxiv updated 2012/06/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

We investigate the Hawking radiation of Schwarzschild–de Sitter (SdS) black hole by massive particles tunneling method. We consider the spacetime background to be dynamical, incorporate the self-gravitation effect of the emitted particles and show that the tunneling rate is related to the change of Bekenstein–Hawking entropy and the derived emission spectrum deviates from the pure thermal spectrum when energy and angular momentum are conserved. Our result is also in accordance with Parikh and Wilczekʼs opinion and gives a correction to the Hawking radiation of SdS black hole.

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