Producing Magnetar Magnetic Fields in the Merger of Binary Neutron Stars

@article{Giacomazzo2014ProducingMM,
  title={Producing Magnetar Magnetic Fields in the Merger of Binary Neutron Stars},
  author={Bruno Giacomazzo and Jonathan Zrake and Paul C. Duffell and Andrew MacFadyen and Rosalba Perna},
  journal={arXiv: High Energy Astrophysical Phenomena},
  year={2014}
}
The merger of binary neutron stars (BNSs) can lead to large amplifications of the magnetic field due to the development of turbulence and instabilities in the fluid, such as the Kelvin-Helmholtz shear instability, which drive small-scale dynamo activity. In order to properly resolve such instabilities and obtain the correct magnetic field amplification, one would need to employ resolutions that are currently unfeasible in global general relativistic magnetohydrodynamic (GRMHD) simulations of… Expand

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TLDR
During and after merger, phenomena driven by the magnetic field are observed, including Kelvin-Helmholtz instabilities in shear layers, winding of the field lines, and transition from poloidal to toroidal magnetic fields. Expand
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