Localization of Energy and Momentum in an Asymptotically Reissner-Nordström Non-Singular Black Hole Space-Time Geometry

The space-time geometry exterior to a new four-dimensional, spherically symmetric and charged black hole solution that, through a coupling of general relativity with a non-linear electrodynamics, is non-singular everywhere, for small <i>r</i> it behaves as a de Sitter metric, and asympto...

Full description

Bibliographic Details
Main Authors: Irina Radinschi, Pradyumn Kumar Sahoo, Theophanes Grammenos, Surajit Chattopadhyay, Marius-Mihai Cazacu
Format: Article
Language:English
Published: MDPI AG 2020-05-01
Series:Universe
Subjects:
Online Access:https://www.mdpi.com/2218-1997/6/5/69