论文标题
黑洞熵距离猜想和黑洞蒸发
The Black Hole Entropy Distance Conjecture and Black Hole Evaporation
论文作者
论文摘要
我们将最近提议的黑洞熵距离猜想延伸到De Sitter空间中带电的黑洞的情况。通过系统地研究带有多个视野的黑洞几何形状空间的距离，我们发现距离通常与熵的对数有关。从无限距离的猜想中，这可以预测无限熵极限的无质量塔的出现。此外，我们研究了这些黑洞的蒸发，并将其与几何距离联系起来。我们发现，蒸发最后阶段的相应距离是有限的。我们得出的结论是，蒸发不会导致黑洞微晶体的轻塔出现。
We extend the recently proposed Black Hole Entropy Distance Conjecture to the case of charged black holes in de Sitter space. By systematically studying distances in the space of black hole geometries with multiple horizons, we find that the distance is generically related to the logarithm of the entropy. From the infinite distance conjecture this predicts the appearance of a massless tower of modes in the limit of infinite entropy. Further, we study the evaporation of these black holes and relate it to the geometric distance. We find that the corresponding distance to the final stage of evaporation is finite. We conclude that evaporation does not lead to the appearance of a light tower of black hole microstates.
