[3] ROTATIONAL PERTURBATION OF HOT BIG BANG VISCOUS FLIUD MODEL UNIVERSES COUPLED WITH SCALAR FIELD: How to Cite the Article:  Naorem Jugeshwor Singh & Akoijam Kesho Singh (2026).  Rotational Perturbation of Hot Big Bang Viscous Fliud Model Universes Coupled with Scalar Field. International Journal of Multidisciplinary Research & Reviews, 5(9), 26-37. https://doi.org/10.56815/ijmrr.v5i9.2026.26-37

Naorem Jugeshwor Singh & Akoijam Kesho Singh

[3] ROTATIONAL PERTURBATION OF HOT BIG BANG VISCOUS FLIUD MODEL UNIVERSES COUPLED WITH SCALAR FIELD

How to Cite the Article: Naorem Jugeshwor Singh & Akoijam Kesho Singh (2026). Rotational Perturbation of Hot Big Bang Viscous Fliud Model Universes Coupled with Scalar Field. International Journal of Multidisciplinary Research & Reviews, 5(9), 26-37. https://doi.org/10.56815/ijmrr.v5i9.2026.26-37

Authors

Naorem Jugeshwor Singh & Akoijam Kesho Singh

Abstract

We will focus on standard hot Big-Bang models involving rotating viscous fluid leading to new interesting solutions. Their properties will be studied from various respective thereby obtaining new idea and information’s regarding the evolutions of the universe. Investigation will also be made as to when the universe ceased to be radiation-dominated and become matter – dominated, pointing out the advantages of our model over the Friedman model.

Keywords:

Big Bang Model, Radiationdominated, Cosmological Constant, Roberstson-Walker Metric, Comic Fluid, EnergyMomentum Tensor, Newtonian Limit, Perfect Dragging