No drama in two-dimensional black hole evaporation

Jonathan Barenboim, Andrei V. Frolov, Gabor Kunstatter
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Abstract

We numerically calculate the spacetime describing the formation and evaporation of a regular black hole in 2D dilaton gravity. The apparent horizons evaporate smoothly in finite time to form a compact trapped region. We nevertheless see rich dynamics: an antitrapped region forms alongside the black hole and additional compact trapped and antitrapped regions are formed by backreaction effects as the mass radiates away. The spacetime is asymptotically flat at future null infinity and is free of singularities and Cauchy horizons. These results suggest that the evaporation of regular 2D black holes is unitary.

Abstract Image

二维黑洞蒸发没有戏剧性
我们对描述二维稀拉顿引力中规则黑洞形成和蒸发的时空进行了数值计算。表观水平面在有限时间内平滑蒸发,形成一个紧凑的被困区域。然而,我们看到了丰富的动力学过程:黑洞旁边形成了一个反捕获区,随着质量的辐射消失,反作用力效应又形成了额外的紧凑捕获区和反捕获区。时空在未来空无穷大处近似平坦,不存在奇点和考奇地平线。这些结果表明,规则二维黑洞的蒸发是单一的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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CiteScore
8.60
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