28–30 Jan 2015
Asia/Calcutta timezone

Geometry of the universe described by wet dark fluid in f(R, T) theory of gravity

29 Jan 2015, 16:15
15m
Lecture Hall-2 (SINP Auditorium)

Lecture Hall-2

SINP Auditorium

Contributory Talks Dark Energy-II

Speaker

Dr Gauranga Charan Samanta (Birla Institute of Technology and Science, Pilani, K k Birla, Goa Campus)

Description

The Bianchi type-III cosmological model in gravity is investigated with the equation of state for wet dark fluid i.e. $P_{WDF}=\omega (\rho_{WDF}-\rho^*)$. Using Volumetric and power law expansion we obtained the exact solution of the field equations. The various astrophysical phenomena namely the look back time, proper distance, luminosity distance, Angular diameter, jerk parameter and cosmic snap with red shift and state-finder parameters are also discussed.

Author

Dr Gauranga Charan Samanta (Birla Institute of Technology and Science, Pilani, K k Birla, Goa Campus)

Presentation materials