Energy Distribution in a Schwarzschild-like Spacetime
Th. Grammenos, I. Radinschi
TL;DR
This paper calculates energy and momentum distribution in a Schwarzschild-like spacetime influenced by gauge fields using M{\
Contribution
It introduces a novel application of M{\
Findings
Energy distribution is explicitly computed for the spacetime.
The method applies to effective gravity coupled with gauge fields.
Results enhance understanding of energy localization in such spacetimes.
Abstract
In this paper, utilizing M{\o}ller's energy-momentum complex, we explicitly evaluate the energy and momentum density associated with a metric describing a four-dimensional, Schwarzschild-like, spacetime derived from an effective gravity coupled with a U(1) gauge field in the context of a D3-brane dynamics in the classical regime, i.e., between the asymptotic and the Planck regime.
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