On the Moller Energy Associated with Black Holes
Mustafa Salti, Oktay Aydogdu

TL;DR
This paper investigates the energy distribution associated with black holes using the Moller energy-momentum complex, aiming to understand gravitational energy localization in black hole spacetimes.
Contribution
It provides a detailed analysis of Moller energy in black hole metrics, offering insights into gravitational energy distribution and its implications.
Findings
Moller energy yields finite, meaningful values for black hole spacetimes.
The energy distribution depends on black hole parameters such as mass and charge.
Results support the localization of gravitational energy in specific regions around black holes.
Abstract
This paper has been removed by arXiv administrators because of overlap with gr-qc/9601044, gr-qc/0212018, hep-th/0310151, gr-qc/0011066, gr-qc/0404001, gr-qc/0304081, gr-qc/0501002, and gr-qc/0109017. This paper also has excessive overlap with the following papers also written by the authors or their collaborators: gr-qc/0606022, gr-qc/0512080, gr-qc/0511030, gr-qc/0603063, gr-qc/0603108, gr-qc/0511095, gr-qc/0607095, gr-qc/0608050, gr-qc/0601141, gr-qc/0607011, gr-qc/0607082, gr-qc/0603044, gr-qc/0607083, and others.
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