The Proto-Magnetar Model for Gamma-Ray Bursts

@article{Metzger2010ThePM,
  title={The Proto-Magnetar Model for Gamma-Ray Bursts},
  author={Brian D. Metzger and Dimitrios Giannios and Todd A. Thompson and Niccolo’ Bucciantini and Eliot Quataert},
  journal={arXiv: High Energy Astrophysical Phenomena},
  year={2010}
}
Long duration Gamma-Ray Bursts (GRBs) originate from the core collapse of massive stars, but the identity of the central engine remains elusive. Previous work has shown that rapidly spinning, strongly magnetized proto-neutron stars (`millisecond proto-magnetars') produce outflows with energies, timescales, and magnetizations sigma_0 (maximum Lorentz factor) that are consistent with those required to produce long GRBs. Here we extend this work in order to construct a self-consistent model that… Expand
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