2004
DOI: 10.1007/s10955-004-5710-x
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Poiseuille Flow in a Heated Granular Gas

Abstract: The planar Poiseuille flow induced by a constant external field (e.g., gravity) has been the subject of recent interest in the case of molecular gases. One of the predictions from kinetic theory (confirmed by computer simulations) has been that the temperature profile exhibits a bimodal shape with a local minimum in the middle of the slab surrounded by two symmetric maxima, in contrast to the unimodal shape expected from the Navier-Stokes (NS) equations. However, from a practical point of view, the interest of… Show more

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Cited by 16 publications
(17 citation statements)
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“…It is clear that T increases monotonically with decreasing e n which implies that the degree of temperature bimodality becomes more pronounced with increasing dissipation/inelasticity. This finding is in apparent contradiction with Tij & Santos (2004) who predicted that T decreases with decreasing e n from the elastic limit up to a value of e n ∼ 0.4 and increases subsequently for e n < 0.4 (see § 3.2.4). …”
Section: The Phase Diagram: Rarefaction Versus Dissipationcontrasting
confidence: 71%
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“…It is clear that T increases monotonically with decreasing e n which implies that the degree of temperature bimodality becomes more pronounced with increasing dissipation/inelasticity. This finding is in apparent contradiction with Tij & Santos (2004) who predicted that T decreases with decreasing e n from the elastic limit up to a value of e n ∼ 0.4 and increases subsequently for e n < 0.4 (see § 3.2.4). …”
Section: The Phase Diagram: Rarefaction Versus Dissipationcontrasting
confidence: 71%
“…Let us make a quantitative comparison of our simulation with the analysis of Tij & Santos (2004) who solved the inelastic Boltzmann equation (with a BGK-type collision model) subjected to a constant gravitational force and a stochastic (white noise) thermostat. The role of the stochastic thermostat was to heat the granular gas such that it compensates the loss of energy due to collisional cooling, yielding a 'uniform' state about which a Chapman-Enskog-type expansion was carried out by treating the body force as a small parameter (which is proportional to the centreline Knudsen number Kn 0 ).…”
Section: Comparison Of Excess Temperature With Theorymentioning
confidence: 99%
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“…F ∼ 1) on the MFR. For granular gases driven by a gravitational force, a large value of F is possible because of the large disc size and mass, and the small thermal velocity (Tij & Santos 2004). Figure 9 shows that the normalized MFR reduces with increasing external acceleration.…”
Section: For Various Values Of L/σ and The Global Knudsen Numbermentioning
confidence: 99%
“…Next, we consider the steady base states that may be generated from energy input in our geometry. Independently of the nature of the boundary conditions, and if there is no pressure drop source or gravitational field in the horizontal directions (which may generate Poiseuille flows; see for example the recent works by Tij & Santos 2004;Santos & Tij 2006;Alam & Chikkadi 2010), the spatial dependence of these steady base states will occur only in the coordinate y, perpendicular to both walls (we call it vertical direction). Moreover, the flow velocity is expected to be parallel to the walls, i.e., u(y) = u x (y)e x .…”
Section: Boltzmann Kinetic Theory and General Balance Equationsmentioning
confidence: 99%