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Journal Article

Magnetic Field Instabilities in Neutron Stars

MPS-Authors

Ciolfi,  Riccardo
AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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1401.5276.pdf
(Preprint), 2MB

CiolfiAN.pdf
(Any fulltext), 189KB

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Citation

Ciolfi, R. (2014). Magnetic Field Instabilities in Neutron Stars. Astronomische Nachrichten, 335(3), 285-290. doi:10.1002/asna.201312033.


Cite as: http://hdl.handle.net/11858/00-001M-0000-002B-0061-5
Abstract
Magnetic fields represent a crucial aspect of the physics and astrophysics of neutron stars. Despite its great relevance, the internal magnetic field configuration of neutron stars is very poorly constrained by the observations, and understanding its properties is a long-standing theoretical challenge. The investigation on the subject is focused on the search for those magnetic field geometries which are stable on several Alfv\`en timescales, thus constituting a viable description of neutron star interiors. Assesing the stability of a given magnetic field geometry is therefore an important part of this research. So far only simple configurations, such as the purely poloidal or purely toroidal ones, have been studied in detail in perturbation theory and, most recently, by means of nonlinear magnetohydrodynamic simulations. Here we review the basic results of the state-of-the-art general relativistic nonlinear studies, discussing the present status of the field and its future directions.