Hawking radiation in a d-dimensional static spherically symmetric black hole surrounded by quintessence
Hawking radiation in a d-dimensional static spherically symmetric black hole surrounded by quintessence
复制标题
DOI：
10.1103/physrevd.77.124011
复制
发表时间：
2008-01
影响因子：
5
通讯作者：
Songbai Chen;Bin Wang;R. Su
中科院分区：
文献类型：
--
作者：
Songbai Chen;Bin Wang;R. Su
本文给出了d维黑洞周围具有典型物质的爱因斯坦方程的一个解，其渐近结构由典型物质的状态决定。我们研究了这个黑洞的热力学，发现黑洞的质量取决于状态方程的精髓，而第一定律是普遍的。在这个黑洞背景下研究霍金辐射，我们观察到霍金辐射在低能区占主导地位。对于黑洞周围的精粹物质的状态方程所引起的不同的渐近结构，我们得知精粹物质的状态参量对Hawking辐射的影响是不同的。
We present a solution of Einstein equations with quintessential matter surrounding a d-dimensional black hole, whose asymptotic structures are determined by the state of the quintessential matter. We examine the thermodynamics of this black hole and find that the mass of the black hole depends on the equation of state of the quintessence, while the first law is universal. Investigating the Hawking radiation in this black hole background, we observe that the Hawking radiation dominates on the brane in the low-energy regime. For different asymptotic structures caused by the equation of state of the quintessential matter surrounding the black hole, we learn that the influences by the state parameter of the quintessence on Hawking radiation are different.