Bianchi type VI cosmological models: A Scale-Covariant study
Mohd. Zeyauddin, Bijan Saha

TL;DR
This paper analyzes an anisotropic Bianchi type VI universe within a Scale Covariant theory of gravitation, revealing a big bang singularity and consistency with current cosmological observations.
Contribution
It introduces a Bianchi type VI cosmological model in Scale Covariant gravity and thoroughly studies its physical parameters and singularity behavior.
Findings
Presence of a finite initial singularity at t=0
Model aligns with observed universe characteristics
Physical parameters are comprehensively analyzed
Abstract
A model for an anisotropic Bianchi type VI universe in a Scale Covariant theory of gravitation (Canuto et al. 1977) is analyzed. A finite singularity is found in the model at the initial time . All the physical parameters are studied and thoroughly discussed. The model behaves like a big bang singular model of the universe. This universe model is found to be consistent with the observations on the present day universe.
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.
