Energy Associated with a Charged Regular Black Hole
arXiv:gr-qc/0103110
Abstract
We show that using an adequate coordinate transformation the charged regular black hole solution given by Ayon-Beato and Garcia can be put in the Kerr-Schild form. Then we use this metric in Kerr-Schild Cartesian coordinates with a result given by Virbhadra and obtain the energy distribution associated with this.
LaTex, 1 figures