On a Raychaudhuri equation for hot gravitating fluids
classification
🌀 gr-qc
keywords
equationabelianfluidgravitatingnon-abelianraychaudhuritemperatureastrophysical
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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.
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