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We conduct a mathematical investigation into the dynamical stability and instability of the Rayleigh–Bénard (abbr. RB) problem for incompressible non-Newtonian fluids exhibiting power law type behavior, with (Formula presented.). We establish a critical threshold, denoted as (Formula presented.), and endeavor to demonstrate that the RB problem exhibits exponential stability through the energy method when the Rayleigh number R (which is influenced by the non-Newtonian component) falls within the interval (Formula presented.). Additionally, we formulate an instability criterion, (Formula presented.), under which the RB problem is deemed unstable, we aim to prove this instability by employing a modified variational method. Our results show that non-Newtonian part has the stabilizing effect for thermal instability. © 2024 Informa UK Limited, trading as Taylor & Francis Group.
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Applicable Analysis
ISSN: 0003-6811
Year: 2024
1 . 1 0 0
JCR@2023
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ESI Highly Cited Papers on the List: 0 Unfold All
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30 Days PV: 2
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