Energy Contents of Some Well-Known Solutions in Teleparallel Gravity
M. Sharif, Abdul Jawad
TL;DR
This paper investigates the energy content of well-known black hole solutions within teleparallel gravity using the Hamiltonian approach, demonstrating consistency with general relativity prescriptions and analyzing energy-momentum flux.
Contribution
It applies the Hamiltonian method to compute energy in teleparallel gravity, showing results align with GR and exploring energy-momentum flux for black hole solutions.
Findings
Energy results match several GR prescriptions
Hamiltonian approach is effective in teleparallel gravity
Energy-momentum flux is evaluated for solutions
Abstract
In the context of teleparallel equivalent to General Relativity, we study energy and its relevant quantities for some well-known black hole solutions. For this purpose, we use the Hamiltonian approach which gives reasonable and interesting results. We find that our results of energy exactly coincide with several prescriptions in General Relativity. This supports the claim that different energy-momentum prescriptions can give identical results for a given spacetime. We also evaluate energy-momentum flux of these solutions.
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