Abstract

We consider an initial-boundary value problem for the nonstationary Stokes system in a bounded domain $$\Omega \subset \mathbb R ^3$$ with slip boundary conditions. We prove the existence in the Hilbert–Sobolev–Slobodetski spaces with fractional derivatives. The proof is divided into two main steps. In the first step by applying the compatibility conditions an extension of initial data transforms the considered problem to a problem with vanishing initial data such that the right-hand sides data functions can be extended by zero on the negative half-axis of time in the above mentioned spaces. The problem with vanishing initial data is transformed to a functional equation by applying an appropriate partition of unity. The existence of solutions of the equation is proved by a fixed point theorem. We prove the existence of such solutions that $$v\in H^{l+2,l/2+1}(\Omega \times (0,T)),\,\nabla p\in H^{l,l/2}(\Omega \times (0,T)),\,v$$ —velocity, $$p$$ —pressure, $$l\in \mathbb R _+\cup \{0\},\,l \ne [l]+\frac{1}{2}$$ and the spaces are introduced by Slobodetski and used extensively by Lions–Magenes. We should underline that to show solvability of the Stokes system we need only solvability of the heat and the Poisson equations in $$\mathbb R ^3$$ and $$\mathbb R _+^3$$ . This is possible because the slip boundary conditions are considered.

Highlights

  • We prove the existence of such solutions that v ∈ Hl+2,l/2+1( × (0, T )), ∇ p ∈ Hl,l/2( × (0, T )), v—velocity, p—pressure, l

  • To prove the existence of solutions to (3.1) some fixed point argument must be applied. To make this possible the pressure p occuring in the r.h.s. of Eqs. (3.8), (3.10), (3.18), (3.20) must be expressed in terms of v. This is possible for slip boundary conditions because in this case p can be calculated from the Neumann problem to the Poisson equations

  • We eliminate the dependence on T for system (1.1) with g0 = 0, h03 = 0

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Summary

Introduction

The main goal of this paper is to prove the existence of solutions to problem (3.1) using only the existence of solutions to the heat equations in R3 × R, R3+ × R and to the Poisson equation in R3, R3+ This can be made by applying the Fourier–Laplace transform and use estimates in spaces Hγσ,σ/2 and Hγσ respectively. After the Laplace transform with respect to t and the Fourier transforms with respect to variables x1, x2 tangent to the plane x3 = 0 a system of ordinary differential equations with respect to x3 is formulated Solving this system (see [12] for the Neumann boundary conditions and [7] for some parabolic system with slip boundary condition) and applying the definition of Hγσ,σ/2 the appropriate estimate follows. In the fourth-coming paper we are going to extend the presented in this paper proof to the L p-case

Notation and auxiliary results
Local considerations
Existence of solutions with vanishing initial data
Proof of Theorem A
Conclusions
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