Gaussian black holes in Rastall gravity

Author:

Spallucci Euro12ORCID,Smailagic Anais2

Affiliation:

1. Department of Physics, University of Trieste, Strada Costiera 11, 34151 Trieste, Italy

2. I.N.F.N. Sezione di Trieste, Strada Costiera 11, 34151 Trieste, Italy

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.

Publisher

World Scientific Pub Co Pte Lt

Subject

Space and Planetary Science,Astronomy and Astrophysics,Mathematical Physics

Cited by 22 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Quantum Gravity Evolution of the Kalb–Ramond like black hole;Chinese Journal of Physics;2023-12

2. Imprints of rastall gravity on particle dynamics;Physica Scripta;2023-10-27

3. Some thermodynamics aspects in Regular Gaussian Black Hole;International Journal of Geometric Methods in Modern Physics;2023-09-22

4. Nonlinear Charged Black Hole Solution in Rastall Gravity;Universe;2022-09-28

5. Optical properties of an axially symmetric black hole in the Rastall gravity;The European Physical Journal Plus;2022-05

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