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arXiv · 0902.0840

Frequency spectrum of toroidal Alfvén mode in a neutron star with Ferraro's form of nonhomogeneous poloidal magnetic field

S. I. Bastrukov·H. -K. Chang·I. V. Molodtsova·E. H. Wu·G. -T. Chen·S. -H. Lan
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Abstract

Using the energy variational method of magneto-solid-mechanical theory of a perfectly conducting elastic medium threaded by magnetic field, the frequency spectrum of Lorentz-force-driven global torsional nodeless vibrations of a neutron star with Ferraro's form of axisymmetric poloidal nonhomogeneous internal and dipole-like external magnetic field is obtained and compared with that for this toroidal Alfvén mode in a neutron star with homogeneous internal and dipolar external magnetic field. The relevance of considered asteroseismic models to quasi-periodic oscillations of the X-ray flux during the ultra powerful outbursts of SGR 1806-20 and SGR 1900+14 is discussed.

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S. I. Bastrukov, H. -K. Chang, I. V. Molodtsova, E. H. Wu, G. -T. Chen, S. -H. Lan. 2009-07-15. Frequency spectrum of toroidal Alfvén mode in a neutron star with Ferraro's form of nonhomogeneous poloidal magnetic field. https://doi.org/10.1007/s10509-009-0069-8

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