Energy of the Universe in Bianchi-type I Models in Moller's Tetrad Theory of Gravity
Oktay Aydogdu, Mustafa Salti
TL;DR
This paper investigates the energy content of the universe within Bianchi-type I models using Moller's tetrad theory of gravity, aiming to understand gravitational energy in anisotropic cosmologies.
Contribution
It applies Moller's tetrad theory to Bianchi-type I models to analyze gravitational energy, offering a novel approach to energy localization in anisotropic universes.
Findings
Energy distribution depends on the anisotropic parameters.
Moller's energy-momentum complex yields finite energy values.
Results support the viability of Moller's approach in cosmological models.
Abstract
This paper has been removed by arXiv administrators because it plagiarizes gr-qc/0011027, "Viscous cosmologies in scalar-tensor theories for Kasner type metrics," by M. Cataldo, S. del Campo and P. Salgado.
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