A black hole in two-dimensional space-time
高能物理 - 理论
2007-05-23 v1 广义相对论与量子宇宙学
摘要
An imploding shell of radiation is shown to create a 2-D black hole within the framework of the ``R=T'' theory. The radius of the horizon is given by 1/(2M), where M is the mass of the black hole. The topology of the central singularity is that of a corner. The radiation emitted very far from the black hole is thermal with temperature M/(2\pi). The back-reaction problem is solved to one-loop order.
引用
@article{arxiv.hep-th/9705135,
title = {A black hole in two-dimensional space-time},
author = {F. Vendrell},
journal= {arXiv preprint arXiv:hep-th/9705135},
year = {2007}
}
备注
12 pages, Revtex, 2 figures