Accelerating Plane Symmetric Cosmological Model with Bulk Viscous and Cosmic Strings in Lyra's Geometry
M Krishna, SobhanBabu Kappala, R Santhikumar

TL;DR
This paper develops an exact cosmological model within Lyra's geometry incorporating bulk viscous fluid and cosmic strings, analyzing its physical and geometrical properties with a constant deceleration parameter.
Contribution
It presents a novel exact solution for a plane symmetric cosmological model in Lyra's geometry with bulk viscosity and cosmic strings, exploring their combined effects.
Findings
Decelerating parameter remains constant.
Bulk viscous pressure proportional to energy density.
Model's physical and geometrical properties analyzed.
Abstract
The present study deals with Lyra's geometry in plane symmetric metric discussed in the presence of bulk viscous fluid and one dimensional strings are assumed to be loaded with particles and the particle energy density. The variation of Hubble's parameter gives a constant value of decelerating parameter. The exact solution has been found for the plane symmetric model in Lyra's geometry in the framework of bulk viscosity and string cosmology. Also, the bulk viscous pressure is assumed to be proportional to the energy density. The physical and geometrical properties of the model 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.
Taxonomy
TopicsCosmology and Gravitation Theories · Solar and Space Plasma Dynamics · Galaxies: Formation, Evolution, Phenomena
