arXiv · 1001.4770
Quiescence and late time activity in collapsars due to critical angular momentum distributions
Abstract
Even thought a large amount of long gamma ray bursts (LGRBs) present quiescent periods, their origin remains unclear. In this talk, it is shown how different angular momentum distributions, as a function of the stellar radius), can lead to neutrino luminosity variability and the possibility of quiescent epochs in LGRBs.
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D. Lopez-Camara. 2010-01-26. Quiescence and late time activity in collapsars due to critical angular momentum distributions. https://arxiv.org/abs/1001.4770
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