论文标题
黑色贝壳的鹰辐射
Hawking Radiation of Black Shells
论文作者
论文摘要
黑色外壳由一个巨大的薄球形外壳组成，该球形壳向其重力半径收缩，从远离壳的外部观察者的角度来看，与Hooft的砖墙相吻合。该物体是由J.R. Arenas和W.Israel构想的，以有效地对黑洞的重力塌陷动力学和热力学进行建模[5,6,21,1]。我们在本文中表明，当我们考虑在近地平线限制中的klein-gordon方程时，黑洞呈现出相同的黑洞排放率。我们将使用Parikh-Wilczek隧道方法获得黑色壳的排放率[2]。
A black shell consists of a massive thin spherical shell contracting toward its gravitational radius, coinciding with 't Hooft's brick wall, from the point of view of an external observer far from the shell. This object was conceived by J.R.Arenas and W.Israel in order to effectively model the gravitational collapse dynamics and the thermodynamics of a black hole [5,6,21,1]. We show in this article that a black shell presents the same emission rate of a black hole when we consider Klein-Gordon equation in the near horizon limit. We will use Parikh-Wilczek tunneling approach to obtain the black shell emission rate [2].
