{ "id": "1905.07636", "version": "v1", "published": "2019-05-18T20:06:38.000Z", "updated": "2019-05-18T20:06:38.000Z", "title": "The interaction between shear and fingering (thermohaline) convection", "authors": [ "P. Garaud", "A. Kumar", "J. Sridhar" ], "comment": "Submitted to ApJ", "categories": [ "astro-ph.SR", "physics.flu-dyn" ], "abstract": "Fingering convection is a turbulent mixing process that can occur in stellar radiative regions whenever the mean molecular weight increases with radius. In some cases, it can have a significant observable impact on stellar structure and evolution. The efficiency of mixing by fingering convection as a standalone process has been studied by Brown et al. (2013), but other processes such as rotation, magnetic fields and shear can affect it. In this paper, we present a first study of the effect of shear on fingering (thermohaline) convection in astrophysics. Using Direct Numerical Simulations we find that a moderate amount of shear (that is not intrinsically shear-unstable) always decreases the mixing efficiency of fingering convection, as a result of the tilt it imparts to the fingering structures. We propose a simple analytical extension of the Brown et al. (2013) model in the presence of shear that satisfactorily explains the numerically-derived turbulent compositional mixing coefficient for moderate shearing rates, and can trivially be implemented in stellar evolution codes. We also measure from the numerical simulations a turbulent viscosity, and find that the latter is strongly tied to the turbulent compositional mixing coefficient. Observational implications and caveats of the model are discussed.", "revisions": [ { "version": "v1", "updated": "2019-05-18T20:06:38.000Z" } ], "analyses": { "keywords": [ "fingering convection", "thermohaline", "mean molecular weight increases", "interaction", "numerically-derived turbulent compositional mixing coefficient" ], "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable" } } }