The Hawking Radiation of the Charged Massive Particle via Tunneling from a Plane Symmetry Black Hole

Abstract:

In Anti-de Sitter space-time, we develop the Parikh-Wilczek’s semi-classical quantum tunneling method to investigate the Hawking radiation of the charged massive particle via tunneling from a plane symmetry black hole. The result shows that, when taking self-gravitation interaction into account, the tunneling rate of the charged massive particle is related to the change of Bekenstein-Hawking entropy, and that the exact emission spectrum is not strictly pure thermal, but is consistent with the underlying unitary theory.

• Periodical: Applied Mechanics and Materials (Volumes 170-173)
• Pages: 2940-2943
• DOI: https://doi.org/10.4028/www.scientific.net/AMM.170-173.2940
• Online since: May 2012
• Authors: Qing Quan Jiang
• Keywords: Bekenstein-Hawking Entropy, Quantum Tunneling, Self-Gravitation Interaction

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