Based on particles in a dynamical geometry, extending the Parikh ＇s method of quantum tunneling, radiation, we deeply investigate the quantum tunneling radiation of Kerr-NUT bhck hole. When self-gravitating action, e...Based on particles in a dynamical geometry, extending the Parikh ＇s method of quantum tunneling, radiation, we deeply investigate the quantum tunneling radiation of Kerr-NUT bhck hole. When self-gravitating action, energy conservation, and angular momentum conservation are taken into account, the emission rate of the particle on the event horizon is related to the change of Bekenstein-Hawking entropy and the emission spectrum is not precisely thermal, but is consistent with an underlying unitary theory.展开更多
Using Damour-Ruffini method,we investigate Hawking radiation from NUT-Taub-like(NT-like) black hole.Considering the total energy conservation and the back reaction of the particle to the spacetime,we get the radiation...Using Damour-Ruffini method,we investigate Hawking radiation from NUT-Taub-like(NT-like) black hole.Considering the total energy conservation and the back reaction of the particle to the spacetime,we get the radiation spectrum on the black hole event horizon,which is related to the change of Bekenstein-Hawking entropy.Meanwhile,we find that the radiation is not exactly thermal,and can take out information from the black hole,which can be used to explain the information loss paradox.The result that we get satisfies the unitary theory of quantum mechanics and is consistent with the work finished before.展开更多
基金The project supported by National Natural Science Foundation of China under Grant No. 10347008 and Science Foundation for Fundamental Research of Sichuan Province under Grand No. 05JY029-092. We would like to thank Prof. Zhang Jing-Yi and Dr. Ren Jun for their beneficial discussions.
文摘Based on particles in a dynamical geometry, extending the Parikh ＇s method of quantum tunneling, radiation, we deeply investigate the quantum tunneling radiation of Kerr-NUT bhck hole. When self-gravitating action, energy conservation, and angular momentum conservation are taken into account, the emission rate of the particle on the event horizon is related to the change of Bekenstein-Hawking entropy and the emission spectrum is not precisely thermal, but is consistent with an underlying unitary theory.
文摘Using Damour-Ruffini method,we investigate Hawking radiation from NUT-Taub-like(NT-like) black hole.Considering the total energy conservation and the back reaction of the particle to the spacetime,we get the radiation spectrum on the black hole event horizon,which is related to the change of Bekenstein-Hawking entropy.Meanwhile,we find that the radiation is not exactly thermal,and can take out information from the black hole,which can be used to explain the information loss paradox.The result that we get satisfies the unitary theory of quantum mechanics and is consistent with the work finished before.
