16–22 giu 2024
Milano
Europe/Rome fuso orario

New limits on the low-energy astrophysical electron antineutrinos at SK-Gd experiment

18 giu 2024, 17:30
2O
Near Aula Magna (U6 building) (University of Milano-Bicocca)

Near Aula Magna (U6 building)

University of Milano-Bicocca

Piazza dell’Ateneo Nuovo 1, Milano, 20126
Poster Supernova neutrinos Poster session and reception 1

Relatori

Andrew Santos Masayuki Harada Yuki Kanemura (ICRR Univ.Tokyo)

Descrizione

The Super-Kamiokande (SK) experiment has the world's leading sensitivity to the astrophysical electron anti-neutrinos up to a few tens MeV, such like supernova originating neutrinos. In 2020, SK was upgraded to enhance its neutron capture signal by loading gadolinium, termed as the SK-Gd phase. Since 2022, more Gd has been loaded to achieve about 75% of neutron captures on Gd. Thanks to this, we continue reducing muon spallation backgrounds while increasing signal efficiency. One of the remaining dominant backgrounds are also atmospheric neutral-current quasi-elastic (NCQE) neutrino interactions. In this poster, we present a new method to reduce these NCQE events by up to a further factor of 10 as well as a dedicated neutron detection neural network to reduce 10^4 of muon spallation events. Finally, we show the results for the upper limits on the electron anti-neutrino flux that we can set with these improvements in the SK-Gd era

Poster prize Yes
Collaboration (if any) SuperKamiokaNDE

Autori principali

Materiali di presentazione