Tilted Bianchi Type V Bulk Viscous Cosmological Models in General Relativity
Anirudh Pradhan, Abha Rai
TL;DR
This paper explores conformally flat tilted Bianchi type V cosmological models with bulk viscous fluids and heat flow, analyzing their physical and geometric properties within general relativity.
Contribution
It introduces new solutions for tilted Bianchi type V models with bulk viscosity as a power function of density, including heat flow effects.
Findings
Models exhibit specific geometric structures.
Bulk viscosity influences cosmic evolution.
Heat flow impacts physical properties.
Abstract
Conformally flat tilted Bianchi type V cosmological models in presence of a bulk viscous fluid and heat flow are investigated. The coefficient of bulk viscosity is assumed to be a power function of mass density. Some physical and geometric aspects of the models are also discussed.
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.