Magnetofluid Dynamics in curved spacetime

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.

9 pages

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Cited by in corpus (7)

• Beltrami state in black-hole accretion disk: A magnetofluid approach
• Novel mechanism for vorticity generation in black-hole accretion disks
• On Beltrami states near black hole event horizon
• Generalized Magnetofluid Connections in Pair Plasmas
• Magnetic Connections in Curved Spacetime
• Diamagnetic field states in cosmological plasmas
• Black hole in a superconducting plasma