Abstract:Abstract. We deal with a class of abstract nonlinear stochastic models, which covers many 2D hydrodynamical models including 2D Navier-Stokes equations, 2D MHD models and 2D magnetic Bénard problem and also some shell models of turbulence. We first prove the existence and uniqueness theorem for the class considered. Our main result is a Wentzell-Freidlin type large deviation principle for small multiplicative noise which we prove by weak convergence method.
“…It also covers the 3D Leray-α model for the Navier-Stokes equations and some shell models of turbulence. For details, we refer to ( [8], Sec. 2.1).…”
Section: Du(t) + Au(t)dt + B(u(t) U(t))dt = Z σ(T U(t−) Z) N (Dt Dz)mentioning
confidence: 99%
“…As it was explained in [8], Condition (A) covers many 2D hydrodynamical models including the 2D Navier-Stokes equations, the 2D magnetohydrodynamic equations, the 2D Boussinesq model of the Bénard convection, the 2D magnetic Bénard problem, the 3D Leray-α model for the Navier-Stokes equations and several shell models of turbulence.…”
We propose and analyze a numerical scheme for the approximation of the solution for the stochastic 2D hydrodynamical type systems driven by non-Gaussian Lévy noise. We prove the convergence of the scheme which is a linear evolution equation with additive noise.
“…It also covers the 3D Leray-α model for the Navier-Stokes equations and some shell models of turbulence. For details, we refer to ( [8], Sec. 2.1).…”
Section: Du(t) + Au(t)dt + B(u(t) U(t))dt = Z σ(T U(t−) Z) N (Dt Dz)mentioning
confidence: 99%
“…As it was explained in [8], Condition (A) covers many 2D hydrodynamical models including the 2D Navier-Stokes equations, the 2D magnetohydrodynamic equations, the 2D Boussinesq model of the Bénard convection, the 2D magnetic Bénard problem, the 3D Leray-α model for the Navier-Stokes equations and several shell models of turbulence.…”
We propose and analyze a numerical scheme for the approximation of the solution for the stochastic 2D hydrodynamical type systems driven by non-Gaussian Lévy noise. We prove the convergence of the scheme which is a linear evolution equation with additive noise.
We establish the existence, uniqueness and approximation of the strong solutions for the stochastic 3D LANS-α model driven by a non-Gaussian Lévy noise. Moreover, we also study the stability of solutions. In particular, we prove that under some conditions on the forcing terms, the strong solution converges exponentially in the mean square and almost surely exponentially to the stationary solution.
“…Here, we present the details for the SABRA shell model (see [24]), but the same results hold for the GOY shell model (see [21,25]). In recent years, there has been an increasing interest in these fluid dynamical models, both for the deterministic and the stochastic case (see also [3,5,9,10]). From the analytic point of view as well as for numerical computations, they are easier to analyze than the Navier-Stokes or Euler equations.…”
Section: An Example: Shell Models Of Turbulencementioning
Gaussian measures μ β,ν are associated to some stochastic 2D models of turbulence. They are Gibbs measures constructed by means of an invariant quantity of the system depending on some parameter β (related to the 2D nature of the fluid) and the viscosity ν. We prove the existence and the uniqueness of the global flow for the stochastic viscous system; moreover the measure μ β,ν is invariant for this flow and is the unique invariant measure. Finally, we prove that the deterministic inviscid equation has a μ β,ν -stationary solution (for any ν > 0).
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