Proto-Magnetars as GRB Central Engines: Uncertainties, Limitations, and Particulars

Details Proto-Magnetars as GRB Central Engines: Uncertainties, Limitations, and Particulars Proto-Magnetars as GRB Central Engines: Uncertainties, Limitations, and Particulars

2010-08-30

arxiv.org/abs/1008.5138v1

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

8 pages. Proceedings for Deciphering the Ancient Universe with GRBs, Kyoto, Japan, April, 2010

Scientific paper

The millisecond proto-magnetar model for the central engine of long-duration gamma-ray bursts is briefly reviewed. Limitations and uncertainties in the model are highlighted. A short discussion of the maximum energy, maximum duration, radiative efficiency, jet formation mechanism, late-time energy injection, and (non-)association with supernovae of millisecond magnetar-powered GRBs is provided.

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