On a Raychaudhuri equation for hot gravitating fluids
  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. 
Chandrasekher Mukku, Swadesh M. Mahajan, Bindu A. Bambah