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Taking into consideration the radiation particle reaction with the total energy of spacetime conservation, Hawking radiation from black hole is re-investigated using the Damour-Ruffini method. It is found that the tunneling probability relates to Bekenstein-Hawking entropy, and the radiation spectrum is not exactly thermal. The result is consistent with the works of other researchers, and satisfies the unitary theory of quantum mechanics.
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Keywords:
- Damour-Ruffini method /
- Hawking radiation /
- energy conservation
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