{ "id": "1411.3559", "version": "v1", "published": "2014-11-13T14:43:32.000Z", "updated": "2014-11-13T14:43:32.000Z", "title": "Gravito-inertial modes in a differentially rotating spherical shell", "authors": [ "Giovanni M. Mirouh", "Clément Baruteau", "Michel Rieutord", "Jérôme Ballot" ], "comment": "2 pages, 1 figure. Proceedings of the CoRoT Symposium 3 / Kepler KASC-7 joint meeting, Toulouse, 7-11 July 2014. To be published by EPJ Web of Conferences", "categories": [ "astro-ph.SR" ], "abstract": "While many intermediate- and high-mass main sequence stars are rapidly and differentially rotating, the effects of rotation on oscillation modes are poorly known. In this communication we present a first study of axisymmetric gravito-inertial modes in the radiative zone of a differentially rotating star. We consider a simplified model where the radiative zone of the star is a linearly stratified rotating fluid within a spherical shell, with differential rotation due to baroclinic effects. We solve the eigenvalue problem with high-resolution spectral computations and determine the propagation domain of the waves through the theory of characteristics. We explore the propagation properties of two kinds of modes: those that can propagate in the entire shell and those that are restricted to a subdomain. Some of the modes that we find concentrate kinetic energy around short-period shear layers known as attractors. We describe various geometries for the propagation domains, conditioning the surface visibility of the corresponding modes.", "revisions": [ { "version": "v1", "updated": "2014-11-13T14:43:32.000Z" } ], "analyses": { "keywords": [ "differentially rotating spherical shell", "high-mass main sequence stars", "propagation domain", "concentrate kinetic energy", "short-period shear layers" ], "note": { "typesetting": "TeX", "pages": 2, "language": "en", "license": "arXiv", "status": "editable" } } }