Energy Distribution for Non-commutative Radiating Schwarzschild Black Holes

TL;DR

This paper calculates the energy distribution of a non-commutative radiating Schwarzschild black hole using Einstein and Moller prescriptions, revealing dependence on mass, non-commutative parameter, and radius, with Einstein's method showing more robustness.

Contribution

It provides the first detailed comparison of energy-momentum distributions for non-commutative radiating Schwarzschild black holes using two different prescriptions.

Findings

Energy expressions depend on mass, $ heta$ parameter, and radius.

Einstein prescription yields more consistent energy results.

Results highlight differences between Einstein and Moller prescriptions.

Abstract

The aim of this article is the calculation of the energy-momentum for a non-commutative radiating Schwarzschild black hole in order to obtain the expressions for energy. We make the calculations with the Einstein and M\oller prescriptions. We show that the expressions for energy in both the prescriptions depend on the mass $M$, $\theta$ parameter and radial coordinate. We make some comparisons between the results. Our results show that the Einstein prescription is a more powerful concept than the M\oller prescription.