Energy and Momentum in Expansive Nondecelerative Universe
Miroslav Sukenik, Jozef Sima
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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