Magnetorotational Collapse of Very Massive Stars:. Formation of Jets and Black Holes

Details Magnetorotational Collapse of Very Massive Stars:. Formation of Jets and Black Holes Magnetorotational Collapse of Very Massive Stars:. Formation of Jets and Black Holes

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ebhe.conf..357s&link_type=abstract

ENERGY BUDGET IN THE HIGH ENERGY UNIVERSE . Proceedings of the International Workshop. Held 22-24 February 2006 in Kashiwa, Japa

Computer Science

Scientific paper

Population III stars are thought to be very massive stars. However, their properties are not clarified yet. In this research, we investigate the features of magnetorotational dynamics of such stars with computer simulations. We find jet-like explosion in a few models and reveal what type of initial model undergo explosion. In addition, we inquire features of newborn black holes as a remnant of core-collapse.

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