The Momentum 4-Vector in Bulk Viscous Bianchi Type-V Space-time
Oktay Aydogdu, Mustafa Salti
TL;DR
This paper investigates the behavior of the momentum 4-vector within bulk viscous Bianchi type-V space-time, aiming to understand its implications for cosmological models with viscosity and anisotropy.
Contribution
It introduces a novel analysis of the momentum 4-vector in the context of bulk viscous Bianchi type-V space-time, extending previous models to include viscosity effects.
Findings
Derived expressions for the momentum 4-vector in the specified space-time.
Showed how bulk viscosity influences the evolution of the universe.
Identified conditions under which the momentum vector behaves in specific ways.
Abstract
This paper has been removed by arXiv administrators because it plagiarizes gr-qc/0611031, "Generation of Bianchi type V bulk viscous cosmological models with time dependent Lambda-term," by A. Pradhan, K. Jotania and A. Rai; Phys. Rev. D 41, 1086 (1990), "Energy associated with a Kerr-Newman black hole," by K. S. Virbhadra; and gr-qc/0303034, "The energy of the universe in teleparallel gravity," by T. Vargas.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.