2017/11/23 by Ernesto Contreras, Angel Rincon, Benjamin Koch +1
Physics and Astronomy · #gr-qc
paper · pdf · doi:10.1142/s0218271818500323
published as International Journal of Modern Physics D Vol. 27, No. 3 · v2: author name corrected. Accepted in Int. J Mod.Phys. D
arxiv created 2017/11/23 · arxiv updated 2019/04/05
In this work, we present a regular black hole solution, in the context of scale-dependent General Relativity, satisfying the weak energy condition. The source of this solution is an anisotropic effective energy-momentum tensor which appears when the scale dependence of the theory is turned-on. In this sense, the solution can be considered as a semiclassical extension of the Schwarzschild one.