Speaker
Mr
Yan Zhang
(Institute of High Energy Physics, Chinese Academy of Sciences)
Description
Supernova neutrino is one of the focal points in the field of neutrino research in recent years. Many experiments hope to detect neutrino burst once again caused by core-collapse supernova (i.e. type Ib/c and type II). Many methods have been applied to estimate galactic core-collapse supernova rate, this article discusses four kinds of reliable method: Detection of supernova neutrinos, SN statistics, Historical galactic SN and Gamma rays detection methods. Combination of four different calculating methods we estimate that the frequency of core-collapse supernovae to be 1.98 events per century.
| Authorship annotation | Yan Zhang, Institute of High Energy Physics, Chinese Academy of Sciences |
|---|---|
| Session and Location | Wednesday Session, Poster Wall #14 (Robert-Schumann-Room) |
| Poster included in proceedings: | no |
Primary author
Mr
Yan Zhang
(Institute of High Energy Physics, Chinese Academy of Sciences)
Co-authors
Mr
Liang-Jian Wen
(Institute of High Energy Physics, Chinese Academy of Sciences)
Mr
Shun Zhou
(Institute of High Energy Physics, Chinese Academy of Sciences)
Mr
Yu-Feng Li
(Institute of High Energy Physics, Chinese Academy of Sciences)
