Energy and Momentum in Expansive Nondecelerative Universe

2001/01/08 by Miroslav Súkeník, Miroslav Sukenik, Sukenik, Miroslav +3
Computer Science · Physics and Astronomy · #Computational Physics and Python Applications #Cosmology and Gravitation Theories #Relativity and Gravitational Theory #gr-qc

paper · pdf · doi:10.48550/arxiv.gr-qc/0101026

8 pages, LaTeX

arxiv created 2001/01/08 · arxiv updated 2009/11/30

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.

Related

• Model of Expansive Nondecelerativa Universe and unified approach to fundamental physical interactions
• An alternative method for calculating the energy of gravitational waves
• A Mode of Unifying Gravitation and Strong Interactions Proposed by the Model of Expansive Nondecelerative Universe
• Compatibility of the expansive nondecelerative universe model with the Newton gravitational theory and the general theory of relativity
• Localization of gravitational field energy and a procedure proposed for its experimental verification