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.
机构:
Victoria Univ Wellington, Sch Math Stat & Operat Res, Wellington, New ZealandVictoria Univ Wellington, Sch Math Stat & Operat Res, Wellington, New Zealand