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2011
The discovery of neutrinos emitted from the Supernova 1987A (SN 1987A) explosion is an outstanding milestone in both neutrino physics and neutrino astronomy. On the one hand, this fortunate observation of supernova neutrinos provides a strong support for the modern theory of supernova explosions.
Zhi-Zhong Xing, Shun Zhou
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The discovery of neutrinos emitted from the Supernova 1987A (SN 1987A) explosion is an outstanding milestone in both neutrino physics and neutrino astronomy. On the one hand, this fortunate observation of supernova neutrinos provides a strong support for the modern theory of supernova explosions.
Zhi-Zhong Xing, Shun Zhou
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Plenary talk at the Neutrino 2024 conference. Session 10: Neutrino cosmology.
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Nuclear Physics B - Proceedings Supplements, 2013
Abstract Detecting neutrinos is the key to understanding core-collapse supernovae, but this is notoriously difficult due to the small interaction cross section of neutrinos and the low frequency of supernovae in galaxies. The revolutionary implications of the detection of about 20 neutrinos from SN 1987A tell us that this quest is worthy.
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Abstract Detecting neutrinos is the key to understanding core-collapse supernovae, but this is notoriously difficult due to the small interaction cross section of neutrinos and the low frequency of supernovae in galaxies. The revolutionary implications of the detection of about 20 neutrinos from SN 1987A tell us that this quest is worthy.
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1990
Exploding stars were suggested by Baade and Zwicky (1934) as the source of bright optical displays (1049 ergs emitted in light energy, 1051 ergs in kinetic energy of particle motion) abruptly appearing inside galaxies and then fading away on time-scales of hundreds of days.
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Exploding stars were suggested by Baade and Zwicky (1934) as the source of bright optical displays (1049 ergs emitted in light energy, 1051 ergs in kinetic energy of particle motion) abruptly appearing inside galaxies and then fading away on time-scales of hundreds of days.
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