Stability of magnetic fields in non-barotropic stars: an analytic treatment

@article{Akgun2013StabilityOM,
  title={Stability of magnetic fields in non-barotropic stars: an analytic treatment},
  author={Taner Akgun and Andreas Reisenegger and Alpha Mastrano and Pablo Marchant},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2013},
  volume={433},
  pages={2445-2466}
}
Magnetic fields in upper main-sequence stars, white dwarfs, and neutron stars are known to persist for timescales comparable to their lifetimes. From a theoretical perspective this is problematic, as it can be shown that simple magnetic field configurations are always unstable. In non-barotropic stars, stable stratification allows for a much wider range of magnetic field structures than in barotropic stars, and helps stabilize them by making it harder to induce radial displacements. Recent… 

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