论文标题
从五维最小的超级大洞中解决信息损失悖论
Resolving the information loss paradox from the five-dimensional minimal supergravity black hole
论文作者
论文摘要
在本文中，我们使用半经典的汉密尔顿 - 雅各比方程研究了带电旋转黑洞的霍金式隧道辐射。通过使用两种分离的方式，我们获得了黑洞的校正熵。结果平等为我们提供了可能解决信息损失悖论的特殊条件。然后，我们专注于相变，结果表明，如果在熵中纳入热波动的效果，则黑洞是不稳定的，而根据黑洞特异性热的签名改变行为，则存在相变。我们发现，在存在热波动的情况下，五维最小超级重力的黑色孔的表现就像Horava-Lifshitz重力中的黑洞一样，因此可以使用二阶相变。
In this paper, we study the Hawking tunneling radiation of the charged rotating black hole in five-dimensional minimal supergravity theory by using the semiclassical Hamilton-Jacobi equation. By using two separated ways we obtain the corrected entropy of the black hole. Equality of results gives us a special condition that may solve the information loss paradox. Then, we focus on the phase transitions, and the results show that if the effects of thermal fluctuations are incorporated in the entropy, the black hole is unstable, while there are phase transitions according to the sign-changing behavior of the black hole specific heat. We find that, in presence of thermal fluctuations, the black holes of five-dimensional minimal supergravity behave like the black holes in Horava-Lifshitz gravity hence the second-order phase transition is possible.
