Speaker
Ms
Heba Abdulrahman
(North-West University)
Description
Recently a generalized Chaplygin gas has been proposed as a unifying solution to the dark energy and dark matter problems. In this work, we will study the density perturbations of a universe filled with radiation, baryonic matter and the Chaplygin gas fluid and analyse the implications on large-scale structure. We will then compare our model results with power spectrum of the observable universe.
Level for award<br> (Hons, MSc, <br> PhD, N/A)?
PhD
Apply to be<br> considered for a student <br> award (Yes / No)?
yes
Primary author
Ms
Heba Abdulrahman
(North-West University)
Co-author
Prof.
Amare Abebe
(North-West University)
