A Non-Singular Black Hole
Aleksandar Bogojevic (Institute of Physics, Belgrade), Dejan Stojkovic, (Case Western Reserve University)
TL;DR
This paper introduces a new, integrable two-dimensional black hole model that avoids singularities and smoothly connects to the classical CGHS solution at large distances.
Contribution
It presents a novel, non-singular black hole solution within an integrable deformation of the CGHS dilaton gravity model.
Findings
The black hole solution is free of singularities.
At large distances, it asymptotically matches the CGHS solution.
The model is completely integrable.
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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