Rotational Perturbation of Hot Big Bang Viscous Fliud Model Universes Coupled with Scalar Field
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
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