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Energy and Momentum in Expansive Nondecelerative Universe

Miroslav Sukenik·Jozef Sima
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Abstract

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.

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Miroslav Sukenik, Jozef Sima. 2001-01-08. Energy and Momentum in Expansive Nondecelerative Universe. https://arxiv.org/abs/gr-qc/0101026

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