{ "id": "1802.04957", "version": "v1", "published": "2018-02-14T05:02:48.000Z", "updated": "2018-02-14T05:02:48.000Z", "title": "Axisymmetric magnetic modes of neutron stars having mixed poloidal and toroidal magnetic fields", "authors": [ "Umin Lee" ], "comment": "17 pages, 10 figures, submitted to MNRAS", "categories": [ "astro-ph.HE" ], "abstract": "We calculate axisymmetric magnetic modes of a neutron star possessing a mixed poloidal and toroidal magnetic field, where the toroidal field is assumed to be proportional to a dimensionless parameter $\\zeta_0$. Here, we assume an isentropic structure for the neutron star and consider no effects of rotation. Ignoring the equilibrium deformation due to the magnetic field, we employ a polytrope of the index $n=1$ as the background model for our modal analyses. For the mixed poloidal and toroidal magnetic field with $\\zeta_0\\not=0$, axisymmetric spheroidal and toroidal modes are coupled. We compute axisymmetric spheroidal and toroidal magnetic modes as a function of the parameter $\\zeta_0$ from $0$ to $\\sim 1$ for the surface field strengths $B_S=10^{14}$G and $10^{15}$G. We find that the frequency $\\omega$ of the magnetic modes decreases with increasing $\\zeta_0$. We also find that the frequency of the spheroidal magnetic modes is almost exactly proportional to $B_S$ for $\\zeta_0\\lesssim 1$ but that this proportionality holds only when $\\zeta_0\\ll 1$ for the toroidal magnetic modes. The wave patterns of the spheroidal magnetic modes and toroidal magnetic modes are not strongly affected by the coupling so long as $\\zeta_0\\lesssim 1$. We find no unstable modes having $\\omega^2<0$.", "revisions": [ { "version": "v1", "updated": "2018-02-14T05:02:48.000Z" } ], "analyses": { "keywords": [ "toroidal magnetic field", "axisymmetric magnetic modes", "neutron star", "mixed poloidal", "toroidal magnetic modes" ], "note": { "typesetting": "TeX", "pages": 17, "language": "en", "license": "arXiv", "status": "editable" } } }