dorsal/arxiv
View SchemaPressure determinations for incompressible fluids and magnetofluids
| Authors | Brian T. Kress, David C. Montgomery |
|---|---|
| Categories | |
| ArXiv ID | physics/0011018 |
| URL | https://arxiv.org/abs/physics/0011018 |
| DOI | 10.1017/S0022377800008825 |
Abstract
Certain unresolved ambiguities surround pressure determinations for incompressible flows, both Navier-Stokes and magnetohydrodynamic. For uniform-density fluids with standard Newtonian viscous terms, taking the divergence of the equation of motion leaves a Poisson equation for the pressure to be solved. But Poisson equations require boundary conditions. For the case of rectangular periodic boundary conditions, pressures determined in this way are unambiguous. But in the presence of "no-slip" rigid walls, the equation of motion can be used to infer both Dirichlet and Neumann boundary conditions on the pressure P, and thus amounts to an over-determination. This has occasionally been recognized as a problem, and numerical treatments of wall-bounded shear flows usually have built in some relatively ad hoc dynamical recipe for dealing with it, often one which appears to "work" satisfactorily. Here we consider a class of solenoidal velocity fields which vanish at no-slip walls, have all spatial derivatives, but are simple enough that explicit analytical solutions for P can be given. Satisfying the two boundary conditions separately gives two pressures, a "Neumann pressure" and a "Dirichlet pressure" which differ non-trivially at the initial instant, even before any dynamics are implemented. We compare the two pressures, and find that in particular, they lead to different volume forces near the walls. This suggests a reconsideration of no-slip boundary conditions, in which the vanishing of the tangential velocity at a no-slip wall is replaced by a local wall-friction term in the equation of motion.
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"abstract": "Certain unresolved ambiguities surround pressure determinations for\nincompressible flows, both Navier-Stokes and magnetohydrodynamic. For\nuniform-density fluids with standard Newtonian viscous terms, taking the\ndivergence of the equation of motion leaves a Poisson equation for the pressure\nto be solved. But Poisson equations require boundary conditions. For the case\nof rectangular periodic boundary conditions, pressures determined in this way\nare unambiguous. But in the presence of \"no-slip\" rigid walls, the equation of\nmotion can be used to infer both Dirichlet and Neumann boundary conditions on\nthe pressure P, and thus amounts to an over-determination. This has\noccasionally been recognized as a problem, and numerical treatments of\nwall-bounded shear flows usually have built in some relatively ad hoc dynamical\nrecipe for dealing with it, often one which appears to \"work\" satisfactorily.\nHere we consider a class of solenoidal velocity fields which vanish at no-slip\nwalls, have all spatial derivatives, but are simple enough that explicit\nanalytical solutions for P can be given. Satisfying the two boundary conditions\nseparately gives two pressures, a \"Neumann pressure\" and a \"Dirichlet pressure\"\nwhich differ non-trivially at the initial instant, even before any dynamics are\nimplemented. We compare the two pressures, and find that in particular, they\nlead to different volume forces near the walls. This suggests a reconsideration\nof no-slip boundary conditions, in which the vanishing of the tangential\nvelocity at a no-slip wall is replaced by a local wall-friction term in the\nequation of motion.",
"arxiv_id": "physics/0011018",
"authors": [
"Brian T. Kress",
"David C. Montgomery"
],
"categories": [
"physics.flu-dyn",
"physics.plasm-ph"
],
"doi": "10.1017/S0022377800008825",
"title": "Pressure determinations for incompressible fluids and magnetofluids",
"url": "https://arxiv.org/abs/physics/0011018"
},
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