Hawking Radiations of Kerr-Newman Black Hole in de Sitter Spacetime by Hamilton-Jacobi Method

M. I. Hossain, M. Hossain
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Abstract

Incorporating Parikh and Wilczek’s opinion Hawking radiations of Kerr-Newman-de Sitter (KNdS) black hole has been investigated by Hamilton-Jacobi method. We have assumed the space time background as dynamical, energy and angular momentum as conserved incorporating the self-gravitation effect of the emitted particles. We have shown that the massive particle tunneling rate is related to the change of Bekenstein-Hawking entropy and the derived emission spectrum deviates from the pure thermal spectrum.
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用Hamilton-Jacobi方法研究de Sitter时空中Kerr-Newman黑洞的霍金辐射
结合Parikh和Wilczek的观点,用Hamilton-Jacobi方法研究了Kerr-Newman-de Sitter (KNdS)黑洞的霍金辐射。我们假设时空背景是动态的,能量和角动量是守恒的,包含了发射粒子的自引力效应。我们已经证明了大质量粒子隧穿速率与贝肯斯坦-霍金熵的变化有关,并且推导出的发射光谱偏离了纯热光谱。
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