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2D Navier-Stokes with viscosity-dependent Navier slip: strong convergence for unbounded initial velocity

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Abstract

For the two-dimensional incompressible Navier-Stokes equations with Navier friction on a smooth, bounded, simply connected domain, we establish strong vorticity convergence along a subsequence in the vanishing viscosity limit for initial vorticity in LpL^p with p>1p>1. The friction coefficients may grow as viscosity vanishes under an explicit growth restriction depending on pp, which includes regimes of vanishing slip length. The main challenge, even for viscosity-independent friction, is to control the vorticity generated at the boundary. We split the vorticity into contributions from the initial data and the boundary. By combining renormalization and estimates for the normal velocity near the boundary, we show that the boundary contribution vanishes in the inviscid limit. As a consequence, the limiting Euler solutions conserve kinetic energy.

Introduction

Let Ω⊂R2\Omega\subset\mathbb{R}^2 be a bounded, simply connected domain with smooth boundary ∂Ω\partial\Omega. We consider the two-dimensional, incompressible Navier–Stokes system with Navier (friction) boundary conditions

{∂tuν+(uν⋅∇)uν+∇pν=νΔuνin (0,T)×Ω,div⁡uν=0in (0,T)×Ω,uν⋅n=0on (0,T)×∂Ω,2(Duν)Sn⋅τ+ανuν⋅τ=0on (0,T)×∂Ω,uν(0,⋅)=u0in Ω.(1)\begin{cases} \partial_t u^\nu+ (u^\nu\cdot\nabla)u^\nu+ \nabla p^\nu= \nu\Delta u^\nu& \text{in } (0,T) \times\Omega,\\ \operatorname{div} u^\nu= 0 & \text{in } (0,T) \times\Omega,\\ u^\nu\cdot n = 0 & \text{on } (0,T) \times\partial\Omega,\\ 2(Du^\nu)_S n \cdot\tau+ \alpha^\nu u^\nu\cdot\tau= 0 & \text{on } (0,T) \times\partial\Omega,\\ u^\nu(0,\cdot) = u_0 & \text{in } \Omega. \tag*{(1)} \end{cases}

The unknowns are the fluid velocity uνu^\nu and the pressure pνp^\nu. We denote by ν>0\nu> 0 the viscosity, by nn the unit normal vector field, by τ\tau the tangent vector field, and by (Dv)S=12(∇v+∇vT)(Dv)_S = \frac{1}{2}(\nabla v + \nabla v^T) the rate-of-strain tensor. The friction coefficient αν∈C2(∂Ω)\alpha^\nu\in C^2(\partial\Omega) is given and may depend on viscosity.

A key feature of the Navier boundary condition is that it implies a boundary condition for the vorticity [8], Lemma 2.1 due to the formal equality

curl⁡uν=2(Duν)sn⋅τ+2κuν⋅τ on ∂Ω,\operatorname{curl} u^\nu= 2(Du^\nu)sn \cdot\tau+ 2\kappa u^\nu\cdot\tau\text{ on } \partial\Omega,

where κ\kappa is the curvature of ∂Ω\partial\Omega. Applying the curl to the momentum equation, we get the vorticity formulation

{∂tων+uν⋅∇ων=νΔων in (0,T)×Ω,ων=curl⁡uν in (0,T)×Ω,uν⋅n=0 on (0,T)×∂Ω,ων=(2κ−αν)uν⋅τ on (0,T)×∂Ω,ων(0,⋅)=ω0 in Ω.(2)\begin{cases} \partial_t\omega^\nu+ u^\nu\cdot\nabla\omega^\nu= \nu\Delta\omega^\nu\text{ in } (0,T)\times\Omega,\\ \omega^\nu= \operatorname{curl}u^\nu\text{ in } (0,T)\times\Omega,\\ u^\nu\cdot n = 0 \text{ on } (0,T)\times\partial\Omega,\\ \omega^\nu= (2\kappa-\alpha^\nu)u^\nu\cdot\tau\text{ on } (0,T)\times\partial\Omega,\\ \omega^\nu(0,\cdot)=\omega_0 \text{ in }\Omega. \tag*{(2)} \end{cases}

The vorticity formulation is formally equivalent, as the velocity uνu^\nu can be recovered from the vorticity ων\omega^\nu using the Biot–Savart law (see also Lemma A.2). Explicitly, we write

uν(t)=KΩ(ων(t)), with KΩ(f)(y):=∫Ω∇yGΩ(x,y)f(x) dx,u^\nu(t)=K_\Omega(\omega^\nu(t)),\text{ with }K_\Omega(f)(y):=\int_\Omega\nabla_yG_\Omega(x,y)f(x)\,dx,

where GΩG_\Omega is the Dirichlet Green’s function. In particular, an initial vorticity ω0∈Lp(Ω)\omega_0\in L^p(\Omega) with p>1p>1 identifies an initial velocity u0=KΩ(ω0)∈W1,p(Ω)⊂L2(Ω)u_0=K_\Omega(\omega_0)\in W^{1,p}(\Omega)\subset L^2(\Omega).

Our goal is to study the vanishing viscosity limit, i.e. ν→0\nu\to0, in which the Navier–Stokes system formally reduces to the Euler system

{∂tu+u⋅∇u+∇p=0 in (0,T)×Ω,div⁡u=0 in (0,T)×Ω,u⋅n=0 on (0,T)×∂Ω,u(0,⋅)=u0 in Ω.(3)\begin{cases} \partial_tu+u\cdot\nabla u+\nabla p=0 \text{ in } (0,T)\times\Omega,\\ \operatorname{div}u=0 \text{ in } (0,T)\times\Omega,\\ u\cdot n=0 \text{ on } (0,T)\times\partial\Omega,\\ u(0,\cdot)=u_0 \text{ in }\Omega. \tag*{(3)} \end{cases}

The transition from Navier–Stokes to Euler as viscosity vanishes has been a classical problem with extensive research for decades (see [22] for an overview). Without physical boundaries, convergence in two dimensions is known for regular Euler solutions [24], and also for weak Euler solution classes with some control on the initial vorticity [6, 7, 28]. With physical boundaries, the Navier–Stokes and Euler boundary conditions generally do not match, because the viscous term disappears in the limit. This mismatch leads to boundary layer effects and makes the inviscid limit more difficult. For the no-slip condition uν=0u^\nu=0, they are so challenging that convergence (or nonconvergence) of velocity is generally still open even in two dimensions when the limiting Euler solution is smooth.

One difficulty here is that the no-slip condition does not prescribe boundary values for the vorticity, which blocks the usual compactness approach based on viscosity-independent a priori estimates for the vorticity.

As already mentioned, the Navier boundary condition, originally introduced by C. Navier in 1827 [26], admits a formulation in terms of vorticity that makes the analysis more manageable. It can also be seen as a relaxation of the no-slip condition, as uν⋅τ=0u^\nu\cdot\tau= 0 is formally recovered for αν=∞\alpha^\nu= \infty. For friction coefficients independent of viscosity, there are the prominent results from Clopeau, Mikelić, and Robert [8], showing strong convergence of velocity for bounded initial vorticity, and Lopes Filho, Nussenzveig Lopes, and Planas [12], extending it to initial vorticity in Lp(Ω)L^p(\Omega) for p>2p > 2. The proof in [12] is based on a uniform vorticity bound

∥ων∥L∞(0,T;Lp(Ω))≤C(∥ω0∥Lp(Ω))for p>2,\|\omega^\nu\|_{L^\infty(0,T;L^p(\Omega))} \le C\left(\|\omega_0\|_{L^p(\Omega)}\right) \quad\text{for } p > 2,

where the constant C>0C > 0 is independent of viscosity ν\nu. The restriction p>2p > 2 is used to bound the boundary velocity in L∞L^\infty by the LpL^p-norm of the vorticity, an estimate that is unavailable for p∈(1,2]p \in(1,2]. Whether the bound can be extended to p∈(1,2]p \in(1,2] is explicitly raised in [12 Section 4, Remark 1] and was the starting point for this work, and we can remove this restriction (Corollary 5.3). Moreover, we can strengthen the velocity convergence in [12] to strong convergence of vorticity: Let ω0∈Lp(Ω)\omega_0 \in L^p(\Omega) with p∈(1,∞)p \in(1,\infty). Then there exists a sequence νk→0\nu_k \to0 such that

ωνk→curl⁡u strongly in C([0,T];Lp(Ω)).\omega^{\nu_k} \to\operatorname{curl} u \text{ strongly in } C([0,T];L^p(\Omega)).

For p>2p > 2, strong convergence of vorticity has already been established in [3, 9].

When the friction coefficient is positive, 1/αν1/\alpha^\nu denotes the slip length. Experimental and numerical studies show that a decrease in viscosity can lead to a decrease in slip length [14, 30]. This motivates the study of coefficients αν\alpha^\nu that may grow with vanishing viscosity ν\nu. We will impose the following growth bound

∥αν∥L∞(∂Ω)≤Cν−q,q≥0,(4)\|\alpha^\nu\|_{L^\infty(\partial\Omega)} \le C\nu^{-q}, \qquad q \ge0, \tag*{(4)}

where the constant C>0C > 0 is independent of ν\nu. By our choice of (4), we include for q>0q > 0 the possibility of vanishing slip (for positive friction) in the vanishing viscosity limit, which allows the boundary vorticity to grow as ν→0\nu\to0. Nevertheless, our main result establishes strong vorticity convergence below a threshold on qq determined by the integrability of the initial vorticity.

Theorem 1.1. Let Ω⊂R2\Omega\subset\mathbb{R}^{2} be a bounded, simply connected domain with smooth boundary, T∈(0,∞)T \in(0,\infty), ω0∈Lp(Ω)\omega_{0} \in L^{p}(\Omega) for p∈(1,∞)p \in(1,\infty), and let uνu^{\nu} be the unique solution to (1.1) for uν(0,⋅)=KΩ(ω0)u^{\nu}(0,\cdot)=K_{\Omega}(\omega_{0}) with αν∈C2(∂Ω)\alpha^{\nu} \in C^{2}(\partial\Omega) which satisfies (1.4). Then, for ρ∈(1,p]\rho\in(1,p] and q≥0q \geq0 satisfying ρq<min⁡{p−12p,14}\rho q < \min\left\{\frac{p-1}{2p},\frac{1}{4}\right\}, there exists a sequence νk→0\nu_{k}\to0 such that

uνk→u strongly in C([0,T];W1,ρ(Ω)) as k→∞,u^{\nu_{k}} \to u \text{ strongly in } C([0,T];W^{1,\rho}(\Omega)) \text{ as } k\to\infty,

and u∈C([0,T];W1,p(Ω))u \in C([0,T];W^{1,p}(\Omega)) is a weak solution of (1.3) for u(0,⋅)=KΩ(ω0)u(0,\cdot)=K_{\Omega}(\omega_{0}). In particular,

ωνk→curl⁡u strongly in C([0,T];Lρ(Ω)) as k→∞,\omega^{\nu_{k}} \to\operatorname{curl}u \text{ strongly in } C([0,T];L^{\rho}(\Omega)) \text{ as } k\to\infty,

and the limiting vorticity ω=curl⁡u\omega=\operatorname{curl}u is a renormalized solution of ∂tω+u⋅∇ω=0\partial_{t}\omega+u\cdot\nabla\omega=0 with initial datum ω0\omega_{0}. Consequently,

∥ω(t)∥Lp(Ω)=∥ω0∥Lp(Ω)for every t∈[0,T].\|\omega(t)\|_{L^{p}(\Omega)}=\|\omega_{0}\|_{L^{p}(\Omega)} \quad\text{for every } t\in[0,T].

The underlying estimates also yield conservation of kinetic energy for the limiting Euler solution.

Analogous results for vanishing-viscosity limits without physical boundaries were established in [5, 6].

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