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Adopting Parikh's mode of quantum radiation as tunneling, the tunneling effect of Reissner_Nordstrm de Sitter black hole is studied. Under implementation of energy conservation, the result shows that the emission of the particle on the event horizon and the cosmic horizon is related with the change of Bekenstein_Hawking entropy and that the spectrum is not precisely thermal.
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Keywords:
- Reissner-Nordstrm de Sitter black hole /
- energy conservation /
- quantum radiation as tunneling
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