1. Introduction
Existence of an equilibrium surface for an isolated compressible liquid mass rotating about a fixed axis was first proved in [9]. Our aim is to prove the existence of equilibrium figures for a rotating compressible two-layer fluid.
The problem of the rotation of an isolated incompressible liquid mass about a fixed axis as a rigid body was considered by many famous mathematicians, among them were Newton, Maclaurin, Jacobi, Kovalevskaya, Lyapunov, Poincare and others [1,2,3], who mainly studied the movement without capillarity. The capillary fluids were first investigated by Globa-Mikhailenko [4], Boussinesq and Charrueau in the begining of 20th century. The latter gave a detailed analysis of the problem, calculated the shape of equilibrium figures, including the toroidal case, and considered some aspects of the stability [5,6]. These results were included in a big review on this subject presented in the book of Appell [7]. Stability problem for various ellipsoidal equilibrium figures is analyzed in monograph [8].
Now we state, in a complete setting, the problem on unsteady motion of two compressible barotropic fluids of finite volume separated by a closed unknown interface.
At the initial instant
, let a fluid with dynamic viscosities
,
be in a bounded domain
, and in the domain
, surrounding it, there be a fluid with dynamic viscosities
,
;
The domain is bounded by the free surface and includes the closed interface ; are given. This two-component cloud rotates about the vertical axis with an angular velocity .
For , it is necessary to find the surfaces , , as well as velocity vector field and the density of the fluids satisfying diffraction problem for the Navier – Stokes system
where
is stress tensor,
is double strain rate tensor,
is identity matrix;
,
are step functions of dynamic viscosities, equal to
,
in
and
,
in
respectively;
is fluid pressure given by a known smooth density function;
and
are initial distributions of velocity and density of the liquids,
is the outward normal vector to the union
;
are twice the mean curvatures of the surfaces
(moreover,
at points of convexity
towards
);
are surface tension coefficients on
and
, respectively;
is the rate of evolution of
in the direction
. We assume that the Cartesian coordinate system
is introduced in the space
. The central dot denotes the Cartesian scalar product.
We mean summation over repeated indices from 1 to 3 if they are denoted by Latin letters, and from 1 to 2 if they are Greek. We mark vectors and vector spaces in bold. The notation denotes the vector with the components , .
The kinematic boundary condition excludes mass transfer across fluid boundaries. It follows from our assumption that the fluid particles do not leave the boundaries during the time.
Local (in time) solvability was proved for problem (1) in the whole space with a closed interface between the fluids. The result was obtain both in the Sobolev – Slobodetskiǐ classes of functions [10] and in the Hölder ones [11]. One can get similar results for a two-component domain bounded by a free boundary if one takes into account the estimates for a model problem in a half-space [12,13].
As we have mentioned, we suppose the liquids to be barotropic which implies that the pressure p is a known increasing function of the density: . Let, in addition, , .
We assume that equilibrium figures , are nearly globular domains with the radiuses (), and the motion of fluids is close to the state of rest, i.e., the velocity is small, and the density differs little from a step function . This picture is schematically presented in Figure 1. We denote the balls by .
We are going to prove the existence of
and
, the boundaries of the figures
and
, respectively. We follow the plan of paper [9].
Figure 1.
Equilibrium Figures for a Two-Layer Compressible Fluid.
Figure 1.
Equilibrium Figures for a Two-Layer Compressible Fluid.
At rest, the bubble consisted of nested spherical two layers
and
with uniform distributions of densities
has the piecewise constant pressure:
The masses of the layers are
Steady motion of a two-layer gaseous body
uniformly rotating about the axis
with a constant angular velocity
is governed by the homogeneous stationary Navier–Stokes equations
(here the density
and velocity
depend only on
x) and the boundary conditions
where
,
are twice the mean curvatures of
,
, respectively. The last relation follows from the boundary condition
. The pressure
depends on
.
It is easily seen that velocity vector field
satisfies (4) together with pressure function gradient
where
is the
ith basis vector,
.
First, we consider the simple case when equality (7) coincides with the following one
whence
and
in
with constants
, because pressure functions can differ each other in different domains by a constant. These constants can be found from relations (2):
Let be the unit sphere in with the center in zero, . We suppose to be given by functions on . In addition, let be rotationally symmetric, i.e., they depend only on and , and be even in .
By substituting
given by (6) and
into boundary conditions (5), we obtain the equations for the surface
of the domain
and for the interface
between the fluids:
Rotationally symmetry implies that do not depend on . It is clear that , since the first two components of are proportional to ones of the radial vector of the circles to be horizontal sections of . Therefore on .
Obviously, the density is given by the formulas
with arbitrary positive constants
and
, equations (9) taking the form
One can determine the constants
by prescribing the masses of fluids to be the same as that of the nested spherical liquid layers (3):
We consider the angular momentum to be one more parameter of the problem. It is given:
where
is the
ith solid rotation vector,
. Then the angular velocity
is a function of
.
We denote by
,
,
, the Hölder space of functions
f on the sphere
with the norm
where
is
th derivative of
f calculated in local coordinates on the subdomain
,
. Under
, we mean the subspace of
consisting of rotationally symmetric functions that are even with respect to
.
Theorem 1.
Let , , and let the data of problem (4), (5) be such that condition (26) holds. Then for an arbitrary β satisfying the estimate
with small enough ε, there exists a unique solution to system (11)–(13). It obeys the inequality