(1) International Institute of Information Technology, Hyderabad, 500 032, India;(2) Institute of Fusion Studies, University of Texas, Austin, Texas 78712, USA;(3) School of Physics, University of Hyderabad, Hyderabad, 500 046, India
Abstract:
We generalise the Raychaudhuri equation for the evolution of a self gravitating fluid to include an Abelian and non-Abelian
hybrid magneto fluid at a finite temperature. The aim is to utilise this equation for investigating the dynamics of astrophysical
high temperature Abelian and non-Abelian plasmas.