Energy-Momentum in viscous Kasner-type Universe in Bergmann-Thomson Formulations
Mustafa Salti, Ali Havare
TL;DR
This paper investigates the energy-momentum distribution in a viscous Kasner-type universe using Bergmann-Thomson formulations, aiming to understand gravitational energy in anisotropic cosmological models.
Contribution
It applies Bergmann-Thomson energy-momentum complex to viscous Kasner universes, providing new insights into gravitational energy localization in anisotropic cosmologies.
Findings
Derived expressions for energy-momentum distribution in viscous Kasner models.
Analyzed the effects of viscosity on energy localization.
Compared results with other gravitational energy definitions.
Abstract
This paper has been removed by arXiv administrators because it plagiarizes gr-qc/0303034, "The energy of the universe in teleparallel gravity," by T. Vargas; and 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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