Black Holes Without Singularities
Aleksandar Bogojevic (Institute of Physics), Dejan Stojkovic (Case, Western Reserve University)

TL;DR
This paper introduces a singularity-free black hole model in two-dimensional dilaton gravity, achieved through a completely integrable deformation of the CGHS model, which behaves like the original at large distances.
Contribution
It presents a novel integrable deformation of the CGHS model resulting in a black hole solution without singularities, extending the understanding of black hole models in lower dimensions.
Findings
The deformed model describes a singularity-free black hole.
At large distances, the solution asymptotically matches the CGHS black hole.
The model maintains integrability and physical consistency.
Abstract
We study the properties of a completely integrable deformation of the CGHS dilaton gravity model in two dimensions. The solution is shown to represent a singularity free black hole that at large distances asymptoticaly joins to the CGHS solution.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Relativity and Gravitational Theory · Cosmology and Gravitation Theories
