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On a Raychaudhuri equation for hot gravitating fluids

Chandrasekher Mukku·Swadesh M. Mahajan·Bindu A. Bambah
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Abstract

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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Chandrasekher Mukku, Swadesh M. Mahajan, Bindu A. Bambah. 2006-10-30. On a Raychaudhuri equation for hot gravitating fluids. https://doi.org/10.1007/s12043-007-0115-4

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