Speaker
Nahuel Ferreiro Iachellini
(University of Milano-Bicocca)
Description
Recent development in the cryogenic detector’s technique opened the possibility to detect neutrinos via Coherent Elastic Neutrino-Nucleus Scattering (CEvNS) with cm3-scale detectors. RES-NOVA will leverage the high cross-section and low-radioactivity of Pb of archaeological origin to investigate the neutrino signal from the next galactic Supernova. Its unique features will allow for the first time the real-time, all-neutrino-flavor observation of this dramatic phenomenon with only a thousandth of the mass of conventional kton water-cherenkov detectors. In this contribution the key aspects of RES-NOVA that can investigate the invisible sector will be presented together with the novelties of this technology.
Primary author
Nahuel Ferreiro Iachellini
(University of Milano-Bicocca)
