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Magnetofluid Dynamics in curved spacetime (1410.7732v2)
Published 27 Oct 2014 in gr-qc and physics.plasm-ph
Abstract: A grand unified field $\mathcal{M}{\mu\nu}$ is constructed from Maxwell's Field tensor and appropriately modified flow field, both non-minimally coupled to gravity, to analyze the dynamics of hot charged fluids in curved background space-time. With a suitable $3+1$ decomposition, this new formalism of the hot fluid is then applied to investigate the vortical dynamics of the system. Finally, the equilibrium state for plasma with non-linear coupling through Ricci scalar $R$ to gravity is investigated to derive a double Beltrami equation in curved space-time.
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