2019
DOI: 10.1103/physrevfluids.4.033402
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Effect of heat-flux boundary conditions on the Rayleigh-Bénard instability in a rarefied gas

Abstract: We consider the effect of heat-flux boundary conditions, replacing the previously studied isothermal wall conditions, on the Rayleigh-Bénard instability in a rarefied gas. The problem is investigated in the limit of small Knudsen numbers, by means of a linear stability analysis of a slip flow model, and the direct simulation Monte Carlo method. In the latter, a noniterative algorithm is applied to implement the heat-flux conditions. The results delineate the instability domain in the parameters plane of the Kn… Show more

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Cited by 9 publications
(4 citation statements)
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References 25 publications
(60 reference statements)
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“…To apply the latter, the boundary temperature is treated as unknown, and a modification of the conventional computational scheme is required. This is carried out using recent contributions by the authors [40,41,43,44],…”
Section: Numerical Scheme: Dsmc Methodsmentioning
confidence: 99%
“…To apply the latter, the boundary temperature is treated as unknown, and a modification of the conventional computational scheme is required. This is carried out using recent contributions by the authors [40,41,43,44],…”
Section: Numerical Scheme: Dsmc Methodsmentioning
confidence: 99%
“…To apply the latter, the boundary temperature is treated as unknown, and a modification of the conventional numerical scheme is required. This is carried out based on recent contributions by the authors [36,[38][39][40][41], where a non-iterative algorithm for the imposition of a heat-flux condition has been suggested and tested. For completeness, the algorithm is repeated here.…”
Section: Numerical Scheme: Dsmc Methodsmentioning
confidence: 99%
“…At Kn ≪ 1, these modes should approximate the initial Knudsen-layer behaviour of the gas, inevitably missing in the NSF description. As in the NSF approximation, once the transformed G(λ, t) fields are determined, the solution is transformed back to the (x, t) plane using Eq (40).…”
Section: Specular Wallmentioning
confidence: 99%
“…They considered a modified Ra, defined by Golshtein and Elperin [34] for a hard-sphere gas, and showed that the derived neutral curves are asymptotically equivalent with a line of constant Rayleigh (Ra ≈ 1773) at r = 0.1 and Kn < 0.01 in the (Fr, Kn) plane. Recently, Ben-Ami and Manela [54] replaced the isothermal wall conditions by the heat-flux boundary conditions and applied the linear temporal stability to the problem. They demonstrated that the heat-flux boundary causes destabilizing effects, extending the convection zone limits to a lower critical Rayleigh (at the onset of convection) and higher rarefaction limits.…”
Section: Introductionmentioning
confidence: 99%