The deformed two-dimensional black hole
高能物理 - 理论
2009-10-31 v2 广义相对论与量子宇宙学
摘要
A deformation of the wave equation on a two-dimensional black hole is considered as a toy-model for possible gravitational or stringy nonlocal effects. The deformed wave-equation allows for an initial-value problem despite being nonlocal. The classical singularity present in the classical geometry is resolved by the deformation, so that propagation of a wave-packet can be continued through the classically singular region, ultimately reaching another asymptotically ``flat'' region.
引用
@article{arxiv.hep-th/9902189,
title = {The deformed two-dimensional black hole},
author = {J. Teschner},
journal= {arXiv preprint arXiv:hep-th/9902189},
year = {2009}
}
备注
12 pager, Latex with eepic macros, minor changes