Proto-Magnetars as GRB Central Engines: Uncertainties, Limitations, and Particulars
arXiv:1008.5138 · doi:10.1063/1.3509357
Abstract
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.
8 pages. Proceedings for Deciphering the Ancient Universe with GRBs, Kyoto, Japan, April, 2010
References in corpus (4)
- Afterglow Observations of Fermi-LAT Gamma-Ray Bursts and the Emerging Class of Hyper-Energetic Events
- GRB Afterglows with Energy Injection from a spinning down NS
- Nickel-Rich Outflows Produced by the Accretion-Induced Collapse of White Dwarfs: Lightcurves and Spectra
- Gamma-Ray Burst Central Engines: Black Hole Vs. Magnetar