pith:NSA53V5Q
Effects of Thermal Boundary Conditions on Natural Convection and Entropy Generation in Non-Newtonian Power-Law Fluids
Thermal boundary conditions control the intensity of convection and the amount of entropy generated in non-Newtonian power-law fluids.
arxiv:2605.13633 v1 · 2026-05-13 · physics.flu-dyn · cs.CE · physics.comp-ph
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Claims
Thermal boundary conditions are found to play an important role in controlling the intensity and spatial distribution of flow, heat transfer, and irreversibility. In both geometries, uniform heating produces stronger and more distributed convective structures, while non-uniform sinusoidal heating localizes thermal forcing and consistently reduces total entropy generation.
The assumption that the flow remains steady and strictly two-dimensional for the full range of Rayleigh numbers and power-law indices examined, which is invoked when the governing equations are solved without time dependence or three-dimensional terms.
Simulations demonstrate that sinusoidal thermal boundary conditions reduce entropy generation in power-law fluid natural convection relative to uniform heating, with shear-thinning fluids producing stronger buoyancy-driven flow and higher Nusselt numbers.
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| First computed | 2026-05-18T02:44:17.721741Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
6c81ddd7b02b027db558bb8678c8f8544650484ab603d2552307d343b2ca4470
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/NSA53V5QFMBH3NKYXODHRSHYKR \
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Canonical record JSON
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