The convective instability of a Maxwell-Cattaneo fluid in the presence of a vertical magnetic field
I.A. Eltayeb, D.W. Hughes, M.R.E. Proctor

TL;DR
This paper investigates the convective instability of a Maxwell-Cattaneo fluid under a vertical magnetic field, revealing new instability modes and complex behaviors influenced by magnetic Prandtl number and Maxwell-Cattaneo effects.
Contribution
It extends previous work to include non-zero magnetic Prandtl number, deriving new asymptotic results and identifying novel instability modes in Maxwell-Cattaneo fluids with magnetic fields.
Findings
Identification of a new instability mode independent of inertial and induction effects.
Non-monotonic critical Rayleigh number dependence on Prandtl number for certain parameters.
Transition between oscillatory modes with different horizontal scales at large magnetic Prandtl number.
Abstract
We study the instability of a B\'enard layer subject to a vertical uniform magnetic field, in which the fluid obeys the Maxwell-Cattaneo (MC) heat flux-temperature relation. We extend the work of Bissell (Proc. R. Soc. A, 472: 20160649, 2016) to non-zero values of the magnetic Prandtl number . With non-zero , the order of the dispersion relation is increased, leading to considerably richer behaviour. An asymptotic analysis at large values of the Chandrasekhar number confirms that the MC effect becomes important when is , where is the Maxwell-Cattaneo number. In this regime, we derive a scaled system that is independent of . When is large, the results are consistent with those derived from the governing equations in the limit of Prandtl number with finite; here we identify a new mode of instability, which is due…
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