We generalize 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 utilize this equation for investigating the
dynamics of astrophysical high temperature Abelian and non-Abelian plasmas.Comment: 13 pages, Invited contribution to Pramana special issue dedicated to
A.K. Raychaudhuri, "The Raychaudhuri equation and its role in Modern
Cosmology". Pramana style files include