Viscous Dark Energy Models with Variable G and Lambda

Details Viscous Dark Energy Models with Variable G and Lambda Viscous Dark Energy Models with Variable G and Lambda

2007-11-14

arxiv.org/abs/0711.2292v1

Chin.Phys.Lett.25:3834-3838,2008

Physics

High Energy Physics

High Energy Physics - Theory

6 Latex pages

Scientific paper

10.1088/0256-307X/25/10/086

We consider a cosmological model with bulk viscosity ($\eta$) and variable cosmological $(\Lambda\propto \rho^{-\alpha}, \alpha=\rm const.$) and gravitational ($G$) constants. The model exhibits many interesting cosmological features. Inflation proceeds du to the presence of bulk viscosity and dark energy without requiring the equation of state $p=-\rho$. During the inflationary era the energy density ($\rho$) does not remain constant, as in the de-Sitter type. Moreover, the cosmological and gravitational constants increase exponentially with time, whereas the energy density and viscosity decrease exponentially with time. The rate of mass creation during inflation is found to be very huge suggesting that all matter in the universe was created during inflation.

Affiliated with

Also associated with

No associations

Rating

Viscous Dark Energy Models with Variable G and Lambda 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 Viscous Dark Energy Models with Variable G and Lambda, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Viscous Dark Energy Models with Variable G and Lambda will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-214338