1987/11/01 by T. HATSUDA, Tetsuo Hatsuda
Physics and Astronomy · #Gamma-ray bursts and supernovae #Pulsars and Gravitational Waves Research #Astrophysical Phenomena and Observations
paper · doi:10.1142/s0217732387001026
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 ~10 53 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.