科研之友
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摘要
Following Hamilton-Jacobi method, we have investigated the Hawking radiation of Kerr-Newman-NUT black hole. We have considered the spacetime background dynamical and incorporate the self-gravitation effect of the emitted particles when energy conservation and angular momentum conservation are taken into account. We have found that the emission rate at the event horizon is equal to the difference of Bekenstein-Hawking entropy before and after emission.
- 出版日期2012-12
