Relatore
Descrizione
With its unprecedented sensitivity to MeV-scale neutrinos, the Jiangmen Underground Neutrino Observatory (JUNO) will play an essential role in the emerging field of multi-messenger astronomy, especially in capturing next galactic core-collapse supernova (CCSN). Two real-time monitoring systems have been designed to detect the forecasted burst of neutrinos from a CCSN in JUNO. Here we present a dedicated CCSN monitoring system and its sensitivity to supernova neutrinos including a variety of supernova models. Assuming a yearly false alert rate, JUNO expects to be sensitive to neutrinos from a 30 $M_\odot$ progenitor up to 370 (360) kiloparsecs, with normal (inverted) mass ordering. The possibility to boost the CCSN sensitivity will be presented, including the one to low energy all-flavour neutrino events, made accessible with JUNO’s Multi-messenger trigger system, which aims to reduce energy thresholds to approximately 20 keV.
| Poster prize | Yes |
|---|---|
| Given name | Shishen |
| Surname | Xian |
| First affiliation | Tsung-Dao Lee Institute |
| Second affiliation | Shanghai Jiao Tong University |
| Institutional email | shishen_xian@sjtu.edu.cn |
| Gender | Male |
| Collaboration (if any) | Jiangmen Underground Neutrino Observatory Collaboration |
