Abstract
A grand unified field is constructed from Maxwell’s field tensor and an appropriately modified flow field, both nonminimally 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 nonminimal coupling through Ricci scalar to gravity is investigated to derive a double Beltrami equation in curved space-time.
- Received 27 October 2014
DOI:https://doi.org/10.1103/PhysRevD.91.064055
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