On the Bergmann Energy-Momentum Complex of a Charged Regular Black Hole
I.Radinschi

TL;DR
This paper applies the Bergmann energy-momentum complex to compute the energy distribution of a charged regular black hole, finding consistent results with the Einstein prescription and deriving a general energy expression for spherically symmetric Kerr-Schild spacetimes.
Contribution
It demonstrates the use of the Bergmann complex for charged regular black holes and derives a general energy formula for Kerr-Schild class spacetimes.
Findings
Energy distribution matches Einstein prescription results.
Derived a general energy expression for spherically symmetric Kerr-Schild spacetimes.
Validated the Bergmann complex as a tool for black hole energy calculations.
Abstract
We use the Bergmann energy-momentum complex to calculate the energy of a charged regular black hole. The energy distribution is the same as we obtained in the Einstein prescription. Also, we get the expression of the energy in the Bergmann prescription for a general spherically symmetric space-time of the Kerr-Schild class.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsBlack Holes and Theoretical Physics · Algebraic and Geometric Analysis · Noncommutative and Quantum Gravity Theories
