Cosmological constant dominated transit universe from early deceleration   to current acceleration phase in Bianchi-V space-time
  The paper presents the transition of universe from early decelerating phase to current accelerating phase with viscous fluid and time dependent cosmological constant $(\Lambda)$ as source of matter in Bianchi-V space-time. To study the transit behaviour of universe, we have assumed the scale factor as increasing function of time which generates a time dependent deceleration parameter (DP). The study reveals that the cosmological term does not change its fundamental nature for $\xi$ = constant and $\xi=\xi(t)$, where $\xi$ is the coefficient of bulk viscosity. The $\Lambda(t)$ is found to be positive and is decreasing function of time. The same is observed by recent supernovae observations. The physical behaviour of universe has been discussed in detail. 
Anil Kumar Yadav
physics.gen-ph