Quiescence and late time activity in collapsars due to critical angular momentum distributions

Details Quiescence and late time activity in collapsars due to critical angular momentum distributions Quiescence and late time activity in collapsars due to critical angular momentum distributions

2010-01-26

arxiv.org/abs/1001.4770v1

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

Proceedings for "The shocking Universe: Gamma-Ray Bursts and High Energy Shock Phenomena in the Universe", Venice 2009

Scientific paper

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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