257 research outputs found

    The regularized 3D Boussinesq equations with fractional Laplacian and no diffusion

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    In this paper, we study the 3D regularized Boussinesq equations. The velocity equation is regularized \`a la Leray through a smoothing kernel of order α\alpha in the nonlinear term and a β\beta-fractional Laplacian; we consider the critical case α+β=54\alpha+\beta=\frac{5}{4} and we assume 12<β<54\frac 12 <\beta<\frac 54. The temperature equation is a pure transport equation, where the transport velocity is regularized through the same smoothing kernel of order α\alpha. We prove global well posedness when the initial velocity is in HrH^r and the initial temperature is in HrβH^{r-\beta} for r>max(2β,β+1)r>\max(2\beta,\beta+1). This regularity is enough to prove uniqueness of solutions. We also prove a continuous dependence of the solutions on the initial conditions.Comment: 28 pages; final version accepted for publication in Journal of Differential Equation

    Remarks on Pressure Blow-Up Criterion of the 3D Zero-Diffusion Boussinesq Equations in Margin Besov Spaces

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    This study is focused on the pressure blow-up criterion for a smooth solution of three-dimensional zero-diffusion Boussinesq equations. With the aid of Littlewood-Paley decomposition together with the energy methods, it is proved that if the pressure satisfies the following condition on margin Besov spaces, π(x,t)∈L2/(2+r)(0,T;B˙∞,∞r) for r=±1, then the smooth solution can be continually extended to the interval (0,T⁎) for some T⁎>T. The findings extend largely the previous results

    Local and Nonlocal Dispersive Turbulence

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    We consider the evolution of a family of 2D dispersive turbulence models. The members of this family involve the nonlinear advection of a dynamically active scalar field, the locality of the streamfunction-scalar relation is denoted by α\alpha, with smaller α\alpha implying increased locality. The dispersive nature arises via a linear term whose strength is characterized by a parameter ϵ\epsilon. Setting 0<ϵ10 < \epsilon \le 1, we investigate the interplay of advection and dispersion for differing degrees of locality. Specifically, we study the forward (inverse) transfer of enstrophy (energy) under large-scale (small-scale) random forcing. Straightforward arguments suggest that for small α\alpha the scalar field should consist of progressively larger eddies, while for large α\alpha the scalar field is expected to have a filamentary structure resulting from a stretch and fold mechanism. Confirming this, we proceed to forced/dissipative dispersive numerical experiments under weakly non-local to local conditions. For ϵ1\epsilon \sim 1, there is quantitative agreement between non-dispersive estimates and observed slopes in the inverse energy transfer regime. On the other hand, forward enstrophy transfer regime always yields slopes that are significantly steeper than the corresponding non-dispersive estimate. Additional simulations show the scaling in the inverse regime to be sensitive to the strength of the dispersive term : specifically, as ϵ\epsilon decreases, the inertial-range shortens and we also observe that the slope of the power-law decreases. On the other hand, for the same range of ϵ\epsilon values, the forward regime scaling is fairly universal.Comment: 19 pages, 8 figures. Significantly revised with additional result

    The stochastic primitive equations with non-isothermal turbulent pressure

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    In this paper we introduce and study the primitive equations with non\textit{non}-isothermal turbulent pressure and transport noise. They are derived from the Navier-Stokes equations by employing stochastic versions of the Boussinesq and the hydrostatic approximations. The temperature dependence of the turbulent pressure can be seen as a consequence of an additive noise acting on the small vertical dynamics. For such model we prove global well-posedness in H1H^1 where the noise is considered in both the It\^{o} and Stratonovich formulations. Compared to previous variants of the primitive equations, the one considered here present a more intricate coupling between the velocity field and the temperature. The corresponding analysis is seriously more involved than in the deterministic setting. Finally, the continuous dependence on the initial data and the energy estimates proven here are new, even in the case of isothermal turbulent pressure.Comment: 55 pages, 1 figure. Some improvements in Section
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