Dark energy models with anisotropic fluid in Bianchi Type- VI 0 space-time with time dependent deceleration parameter

Details Dark energy models with anisotropic fluid in Bianchi Type- VI 0 space-time with time dependent deceleration parameter Dark energy models with anisotropic fluid in Bianchi Type- VI 0 space-time with time dependent deceleration parameter

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012ap%26ss.337..401p&link_type=abstract

Astrophysics and Space Science, Volume 337, Issue 1, pp.401-413

Astronomy and Astrophysics

Astrophysics

4

Scientific paper

We present two dark energy (DE) models with an anisotropic fluid in Bianchi type- VI 0 space-time by considering time dependent deceleration parameter (DP). The equation of state (EoS) for dark energy ω is found to be time dependent and its existing range for derived models is in good agreement with the recent observations. Under the suitable condition, the anisotropic models approach to isotropic scenario. We also find that during the evolution of the universe, the EoS parameter for DE changes from ω>-1 to ω=-1 in first model whereas from ω>-1 to ω<-1 in second model which is consistent with recent observations. The cosmological constant Λ is found to be a positive decreasing function of time and it approaches a small positive value at late time (i.e. the present epoch) which is corroborated by results from recent type Ia supernovae observations. The cosmic jerk parameter in our derived models is also found to be in good agreement with the recent data of astrophysical observations. The physical and geometric aspects of both the models are also discussed in detail.

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