arXiv · gr-qc/9804070
A Non-Singular Black Hole
Abstract
We present a completely integrable deformation of the CGHS dilaton gravity model in two dimensions. The solution is a singularity free black hole that at large distances asymptoticaly joins to the CGHS solution.
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Aleksandar Bogojevic, Dejan Stojkovic. 1998-04-26. A Non-Singular Black Hole. https://doi.org/10.1103/physrevd.61.084011
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