$\Gamma\cross[0, \infty)arrow[0, \infty)$ , with $h(|v_{\tau}|)(\cdot):=h(\cdot, |\mathrm{t} ..... Find $v\in V_{*,\sigma}^{1,2}$ (0) such that for all $\phi$ .... By definition, $V$ depends on $\tilde{v}$ , which depends on the choice of $\epsilon$.
数理解析研究所講究録 1353 巻 2004 年 21-34
21
Steady flows of incompressible Newtonian fluids with threshold slip boundary conditions C. Le Roux’ Department of Mathematics, Faculty of Natural and Agricultural Sciences,
University of Pretoria, Pretoria 0002, South Africa
慶應義塾大学・理工学部
谷
温之
$(\mathrm{A}.
\mathrm{T}\mathrm{a}\mathrm{n}\mathrm{i})^{\dagger}$
Department of Mathematics, Faculty of Science and Technology,
Keio University, 3-14-1 Hiyoshi, Kohoku-ku, Yokohama 223-8522, Japan
Abstract We give some wellposedness results for the time-independent Navier-Stokes equations with threshold slip boundary conditions in bounded domains. The boundary condition is a generalization of Navier’s slip condition and a frictionlike condition: for wall slip to occur the magnitude of the tangential traction must exceed a prescribed threshold, independent of the normal stress, and where slip occurs the tangential traction is equal to a prescribed, possibly nonlinear, function of the slip velocity. In addition, a Dirichlet condition is imposed on a component of the boundary if the domain is rotationally symmetric.
1Introduction We consider the Navier-Stokes equations for steady flows of incompressible fluids, $-\nu\triangle v+v\cdot/v$
$+$
$\mathit{7}p=f$
$\mathrm{d}\mathrm{i}\mathrm{v}v=0$
in in
$\Omega$
,
$\Omega$
,
(1.1) (1.2)
with the impermeability boundary condition $v_{\mathrm{n}}=0$
on
$\Gamma$
(1.3)
and the slip boundary condition $|(Tn)_{\tau}|\leq g\Rightarrow v_{\tau}=(v_{w})_{\tau}$
,
$|(Tn)_{\tau}|>g\triangleright v,$
,
$\neq(v_{w})_{\tau}$
$(Tn)_{\tau}=-(g+h(|(v-v_{w})_{\tau}|)) \frac{(v-v_{w})_{\tau}}{|(v-v_{w})_{\tau}|}\}$
on
$\Gamma$
(1.4) $*$
christiaan .lerouxQup . jp .keio .
$\uparrow \mathrm{t}\mathrm{a}\mathrm{n}\mathrm{i}\mathrm{Q}\mathrm{m}\mathrm{a}\mathrm{t}\mathrm{h}$
$\mathrm{a}\mathrm{c}$
. . za $\mathrm{a}\mathrm{c}$
22 Here is the flow region, a bounded domain in , is the kinetic viscosity, o is the velocity, is the modified pressure, and $f$ is the external body force per unit mass. Thus and , where is the viscosity coefficient, is the density and is the pressure. Furthermore, is the outward unit normal on the boundary of , , $v_{n}:=v\cdot n$ , ($7_{\mathcal{T}}:=v-vnn$ is the tangential component of the velocity, $T:=-\tilde{p}I+2\mu D(v)$ is the Cauchy stress tensor with , $(Tn)_{\tau}=Tn-(n\cdot Tn)n$ $=2\mu(D(v)n)_{\tau}$ is the tangential traction, is the tangential velocity of the wall surface at , : , with and : on . Condition (1.4) means that the fluid slips at a point on the boundary if and only if the magnitude of the tangential traction exceeds the slip threshold at that point, in which case the tangential traction is a (not necessarily invertible) function of the slip velocity. consists of two disjoint parts, and , such that I $|>0,$ We assume that where ), and denotes the surface measure (curve measure, if $\mathbb{R}^{3}$
$\mathbb{R}^{2}$
$\Omega$
$\nu$
$\mathrm{r}$
$v$
$p$
$p=\tilde{p}/\rho$
$\nu=\mu \mathit{1}\rho$
$\mu$
$\rho$
$n$
$\tilde{p}$
$\Omega$
$\partial\Omega$
$\Gamma\subset\partial\Omega$
$D(v):= \frac{1}{2}[\nabla v+(\nabla v)^{T}]$
$\Gamma$
$v_{w}$
$h$
$\Gamma\cross[0, \infty)arrow[0, \infty)$
$h(|v_{\tau}|)(\cdot):=h(\cdot, |\mathrm{t} \tau(\cdot)|)$
$\Gammaarrow(0, \infty)$
$g$
$\Gamma$
$g$
an
$\Gamma$
$|$
$\Omega\subset \mathbb{R}^{2}$
$|\ulcorner|$
1. 2.
$\Sigma$
$\overline{\Gamma}\cap\overline{\Sigma}=\emptyset$
$|\Sigma|>0$
if
, i.e. dist $\Omega$
$(\mathrm{F}, \Sigma)>0,$
if
$|\Sigma|>0;$
is rotationally symmetric.
For brevity, we will refer to these geometric assumptions as condition (C). If $|\Sigma|>0,$ we impose the Dirichlet condition $v=v_{*}$
on
$\Sigma$
,
(1.5)
Thus, is an impermeable solid surface along where is such that porous may slip, and is a which the fluid or artificial boundary where the flow is , (x, ) $=0$ if and only if $v=0,$ then condition (1.4) prescribed. If for every is equivalent to $\int_{\Sigma}v_{*}\cdot n=0.$
$v_{*}$
$\Gamma$
$\mathrm{C}$
$xx$
$\in\Gamma$
$h$
$v$
$|(\mathrm{J}n)_{\tau}|\leq g+h(|(v-v_{w})_{\tau}|)$
,
$(Tn)_{\tau}\cdot(v-v_{w})_{\tau}=-(g +h(|(\mathrm{t}-\mathrm{Z}^{\mathrm{t}}w)\tau|))$
$|(v-v_{w})_{\tau}|\}$
on
$\Gamma \mathrm{r}$
(1.6)
Slip boundary conditions of this kind have been used to model flows of polymer melts during extrusion, flows of yield stress fluids, and flows of Newtonian fluids with a moving contact line. It can be viewed as generalization of the following three slip boundary conditions: $\circ$
The slip condition of Navier [1], $(Tn)_{\tau}=-kv_{\tau}$
on , $\Gamma$
(1.7)
where $k:\Gammaarrow(0, \infty)$ is given, is the special case of (1.4) in which $g(oe)=0,$ (x, ) $=k(x)u$ for all and $u\geq 0$ (if we ignore the assumption $g(x)>0)$ , and can be described by a single rigid body motion. Navier’s slip condition has been applied in a wide variety of fluid problems. The wellposedness of a number of boundary-value problems (e.g. [2, 3]), initial-boundaryvalue problems (e.g. $[4]-[7]$ ), free surface problems (e.g. $[8]-[10]$ ) and control problems (e.g. [11]-[13]) for the Navier-Stokes equations with Navier’s slip $h$
$x$
$u$
$v_{w}$
$\in\Gamma$
23 condition has been established. In particular, Tani et al. general Navier slip condition $\theta(Tn)_{\tau}=-$ $(1-\theta)v_{\tau}$
$[4]-[6]$
consider the
on ,
(1.8)
$\Gamma$
where : $\Gamma\cross[0, T)arrow[0,1]$ is a prescribed function of position and time. Thus, the extremes of nO-slip $(\theta=0)$ and free slip (&=1) are possible in condition (1.8). $\theta$
Nonlinear Navier-type slip conditions of the form
$\mathrm{o}$
$(v-v_{w})_{\tau}=-7 \mathrm{J}(|(\mathrm{i} n)_{\tau}|)\frac{(Tn)_{\tau}}{|(Tn)_{\tau}|}$
on
(1.9)
$\Gamma$
or $(Tn)_{\tau}=-h(|( \mathrm{t}) -v_{w})_{\tau}|)\frac{(v-v_{w})_{\tau}}{|(v-v_{w})_{\tau}|}$
on
(1.10)
$\Gamma_{:}$
where , $h:\Gamma\cross[0, \infty)arrow[0, \infty)$ are given functions, are often used to model the wall slip of non-Newtonian fluids. See [14] for more detail and some related references. $\overline{h}$
The threshold slip condition
$\circ$
$|(Tn)\mathrm{J}$
$|$
$\leq g,$
on
,
$(\mathrm{J} n)_{\tau}|=!/$ $\Rightarrow|(v-v_{w})_{\tau}|(Tn)_{\tau}=-g(v-v_{w})_{\tau}\}$ $(Tn)\tau|