Energy Contents of a Class of Regular Black Hole Solutions in Teleparallel Gravity

Abstract

In this paper, we discuss the energy-momentum problem in the realm of teleparallel gravity. The energy-momentum distribution for a class of regular black holes coupled with a non-linear electrodynamics source is investigated by using Hamiltonian approach of teleparallel theory. The generalized regular black hole contains two specific parameters $\alpha$ and $\beta$ (a sort of dipole and quadrupole of non-linear source) on which the energy distribution depends. It is interesting to mention here that our results exactly coincide with different energy-momentum prescriptions in General Relativity.

arXiv comment13 pages, accepted for publication Mod. Phys. Lett. A

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• Energy conditions in generalized teleparallel gravity models
• Matter Conditions for Regular Black Holes in $\mathbf{f}(\mathbf{T})$ Gravity
• Accretion onto Some Well-Known Regular Black Holes
• $f(T)$ gravity and energy distribution in Landau-Lifshitz prescription
• Teleparallel Energy-Momentum Distribution of Locally Rotationally Symmetric Spacetimes