Affiliation:
1. National Laboratory for High Energy Physics (KEK), Ibaraki, 305, Japan
Abstract
Possibility of strange star formation in the recently discovered LMC supernova is examined. If the proto-neutron star first formed is converted into a strange star about 1 sec after the core bounce, a large energy release with E tot ~1053 erg having QCD origin occurs. The high energy [Formula: see text]-events of long duration observed by Kamiokande II and IMB detectors can be naturally understood by the formation of the hot strange star.
Publisher
World Scientific Pub Co Pte Lt
Subject
General Physics and Astronomy,Astronomy and Astrophysics,Nuclear and High Energy Physics
Cited by
20 articles.
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