论文标题
黑洞和页面曲线的完全蒸发
Complete evaporation of black holes and Page curves
论文作者
论文摘要
Schwarzschild黑洞的完全蒸发的问题是，对于消失的黑洞质量M的温度爆炸了$ t = 1/8πm$。我们考虑使用reissner-nordstrom Black Black Hole，并注意到，如果质量$ M $ $ M $并充电Q <m，则可以使Q> M-C M^3，C> M^3，C> M^3，C> M^3，而不是blight blight，则可能是完整的M BLACK SEDUENS，它可能会散发出黑色的温度。我们描述了状态方程表面上的曲线，以便沿着它们的运动提供完整的蒸发。辐射熵遵循页面曲线，并在蒸发结束时消失。 讨论了旋转Kerr，Schwarzschild-De-Sitter和Reissner-Nordstrom-（Anti）-De-Sitter黑洞的类似结果。
The problem of complete evaporation of Schwarzschild black holes raised by Hawking is that one has an explosion of the temperature $T=1/8πM$ for vanishing black hole mass M. We consider the Reissner-Nordstrom black hole and note that if mass $M$ and charge Q<M satisfy the bound Q>M-C M^3, C>0 for small M then the complete evaporation of black holes without blow-up of temperature is possible. We describe curves on the surface of state equations such that the motion along them provides complete evaporation. The radiation entropy follows the Page curve and vanishes at the end of evaporation. Similar results for rotating Kerr, Schwarzschild-de-Sitter and Reissner-Nordstrom-(Anti)-de-Sitter black holes are discussed.
