Magnetofluid Dynamics in curved spacetime
Chinmoy Bhattacharjee, Rupam Das, S.M.Mahajan

TL;DR
This paper develops a unified formalism for hot charged fluid dynamics in curved spacetime, incorporating non-minimal coupling to gravity, and explores vortical behavior and equilibrium states with nonlinear Ricci scalar coupling.
Contribution
It introduces a novel grand unified field tensor combining electromagnetic and flow fields with gravity, and applies it to analyze vortical dynamics and equilibrium in curved spacetime.
Findings
Derived a double Beltrami equation in curved spacetime.
Analyzed vortical dynamics of hot charged fluids.
Explored equilibrium states with Ricci scalar coupling.
Abstract
A grand unified field 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 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 to gravity is investigated to derive a double Beltrami equation in curved space-time.
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