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Semiclassical approach for the evaporating black hole revisited

机译:再探讨蒸发黑洞的半经典方法

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摘要

A recent calculation shows that the observed energy density in the Unruh state at the future event horizon as seen by a freely falling observer is finite if the observer is released from rest at any positive distance outside the horizon; however, it is getting larger and larger so that it is negatively divergent at the horizon in the limit that the observer starts falling from rest at the horizon, which corresponds to the infinite boost with respect to the freely falling observer at a finite distance from the horizon. In order to resolve some conflicts between the recent calculation and the conventional ones in the well-known literatures, the calculation of the free-fall energy density is revisited and some differences are pointed out.
机译:最近的计算表明,如果观察者在视平线之外任何正距离处从静止状态释放,则自由下落的观察者在Unruh状态下观察到的能量密度是有限的。但是,它变得越来越大,以至于它在地平线上出现负向散的极限,即观察者从地平线上的静止状态开始下降,这对应于相对于自由下落的观察者在距物体有限距离处的无限增强。地平线。为了解决最近的计算与已知文献中的常规计算之间的一些冲突,重新讨论了自由落体能量密度的计算并指出了一些差异。

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