Energy and Momentum in Expansive Nondecelerative Universe

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Incorporation of the Vaidya metric in the model of Expansive Nondecelerative Universe allows to precisely localize gravitational energy for weak fields and obtain the components of the Einstein energy-momentum pseudotensor for strong gravitational fields. The components are identical to those calculated by Virbhadra.
8 pages, LaTeX

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General Relativity and Quantum Cosmology

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http://salesiana.dossiersoluciones.com/handle/123456789/33766

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/gr-qc/0101026
 http://arxiv.org/abs/gr-qc/0101026

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arXiv