Gaussian black holes in Rastall gravity
Euro SpallucciDepartment of Physics, University of Trieste, Strada Costiera 11, 34151 Trieste, ItalyAnais SmailagicI.N.F.N. Sezione di Trieste, Strada Costiera 11, 34151 Trieste, Italy
2017en
ABI
Abstract
In this short note we present the solution of Rastall gravity equations sourced by a Gaussian matter distribution. We find that the black hole metric shares all the common features of other regular, General Relativity BH solutions discussed in the literature: there is no curvature singularity and the Hawking radiation leaves a remnant at zero temperature in the form of a massive ordinary particle.
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Cited by 20 references