Journal
CLASSICAL AND QUANTUM GRAVITY
Volume 40, Issue 14, Pages -Publisher
IOP Publishing Ltd
DOI: 10.1088/1361-6382/acde3c
Keywords
nonsingular black holes; conformal symmetry; de Sitter core
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The form of the metric for static, nonsingular black holes with a de Sitter core, representing a deformation of the Schwarzschild solution, is derived by assuming a flow between two conformal points described by the gravitational sources at small and great distances. The resulting black-hole metric is found to be a specific case of the Fan & Wang metric, which has been recently constrained using data from the S2 star orbits around the galactic center SgrA*.
We derive the form of the metric for static, nonsingular black holes with a de Sitter core, representing a deformation of the Schwarzschild solution, by assuming that the gravitational sources describe a flow between two conformal points, at small and great distances. The resulting black-hole metric turns out to be a particular case of the Fan & Wang metric, whose parameters have been recently constrained by using the data of the S2 star orbits around the galactic center SgrA*.
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