Some Homogeneous Bianchi Type IX Viscous Fluid Cosmological Models with a varying $Λ$

Details Some Homogeneous Bianchi Type IX Viscous Fluid Cosmological Models with a varying $Λ$ Some Homogeneous Bianchi Type IX Viscous Fluid Cosmological Models with a varying $Λ$

2003-07-09

arxiv.org/abs/gr-qc/0307039v2

Astrophys.Space Sci. 298 (2005) 419-432

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

14 pages

Scientific paper

10.1007/s10509-005-5832-x

Some Bianchi type IX viscous fluid cosmological models are investigated. To get a solution a supplementary condition between metric potentials is used. The viscosity coefficient of bulk viscous fluid is assumed to be a power function of mass density whereas the coefficient of shear viscosity is considered as proportional to scale of expansion in the model. The cosmological constant $\Lambda$ is found to be positive and is a decreasing function of time which is supported by results from recent supernova observations. Some physical and geometric properties of the models are also discussed.

Affiliated with

Also associated with

No associations

Rating

Some Homogeneous Bianchi Type IX Viscous Fluid Cosmological Models with a varying $Λ$ does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Some Homogeneous Bianchi Type IX Viscous Fluid Cosmological Models with a varying $Λ$, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Some Homogeneous Bianchi Type IX Viscous Fluid Cosmological Models with a varying $Λ$ will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-577451