Abstract
Applying Parikh’s semi-classical quantum tunneling method, the tunneling radiation characteristic of the charged particle from the event horizon of the Reissner–Nordström–anti de Sitter black hole is researched. The result shows the derived spectrum is not purely thermal one, but is consistent with the underlying unitary theory, which gives a might explanation to the information loss paradox and is the correct amendment to the Hawking radiation.
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Chen, DY., Jiang, QQ. & Yang, SZ. Tunneling Radiation Characteristic of the Charged Particle from the Reissner–Nordström–anti de Sitter Black Hole. Int J Theor Phys 46, 3275–3280 (2007). https://doi.org/10.1007/s10773-007-9446-7
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DOI: https://doi.org/10.1007/s10773-007-9446-7