Search results for "Enstrophy"

showing 3 items of 3 documents

Viscous-Inviscid Interactions in a Boundary-Layer Flow Induced by a Vortex Array

2014

In this paper we investigate the asymptotic validity of boundary layer theory. For a flow induced by a periodic row of point-vortices, we compare Prandtl's solution to Navier-Stokes solutions at different $Re$ numbers. We show how Prandtl's solution develops a finite time separation singularity. On the other hand Navier-Stokes solution is characterized by the presence of two kinds of viscous-inviscid interactions between the boundary layer and the outer flow. These interactions can be detected by the analysis of the enstrophy and of the pressure gradient on the wall. Moreover we apply the complex singularity tracking method to Prandtl and Navier-Stokes solutions and analyze the previous int…

Complex singularitieApplied MathematicsPrandtl numberFluid Dynamics (physics.flu-dyn)Mathematics::Analysis of PDEsFOS: Physical sciencesReynolds numberPhysics - Fluid DynamicsMathematical Physics (math-ph)MechanicsEnstrophyVortexPhysics::Fluid Dynamicssymbols.namesakeBoundary layerFlow separationBoundary-layer separationSingularityInviscid flowsymbolsSettore MAT/07 - Fisica MatematicaMathematical PhysicsViscous-inviscid interactionsMathematicsActa Applicandae Mathematicae
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Troubled cosmic flows: turbulence, enstrophy and helicity from the assembly history of the intracluster medium

2021

Both simulations and observations have shown that turbulence is a pervasive phenomenon in cosmic scenarios, yet it is particularly difficult to model numerically due to its intrinsically multiscale character which demands high resolutions. Additionally, turbulence is tightly connected to the dynamical state and the formation history of galaxies and galaxy clusters, producing a diverse phenomenlogy which requires large samples of such structures to attain robust conclusions. In this work, we use an adaptive mesh refinement (AMR) cosmological simulation to explore the generation and dissipation of turbulence in galaxy clusters, in connection to its assembly history. We find that major mergers…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Accretion (meteorology)TurbulenceFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsVorticityEnstrophyAstrophysics - Astrophysics of GalaxiesGalaxySpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Vortex stretchingIntracluster mediumGalaxy clusterAstrophysics::Galaxy AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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On a rough perturbation of the Navier-Stokes system and its vorticity formulation

2019

We introduce a rough perturbation of the Navier-Stokes system and justify its physical relevance from balance of momentum and conservation of circulation in the inviscid limit. We present a framework for a well-posedness analysis of the system. In particular, we define an intrinsic notion of solution based on ideas from the rough path theory and study the system in an equivalent vorticity formulation. In two space dimensions, we prove that well-posedness and enstrophy balance holds. Moreover, we derive rough path continuity of the equation, which yields a Wong-Zakai result for Brownian driving paths, and show that for a large class of driving signals, the system generates a continuous rando…

Statistics and ProbabilityRough pathMathematical analysisProbability (math.PR)VorticityEnstrophyMomentumPhysics::Fluid DynamicsMathematics - Analysis of PDEsInviscid flowFOS: MathematicsLimit (mathematics)Statistics Probability and UncertaintyRandom dynamical systemBrownian motionMathematics - ProbabilityMathematicsAnalysis of PDEs (math.AP)
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