Sensitivity to core-collapse supernovae neutrino signals in DarkSide-20k

Not scheduled
20m
Procida

Procida

Hotel La Torre, Via Giovanni da Procida, 22 , Procida, Italy
Abstract for a Poster Poster Session and Aperitif

Speaker

Giuseppe Matteucci (Istituto Nazionale di Fisica Nucleare)

Description

DarkSide-20k (DS-20k) will explore the dark matter WIMP hypothesis with a dual-phase time projection chamber detector filled with 50 tonnes of low-radioactivity liquid argon extracted from underground sources. Besides the primary physics goal of DS-20k, the low-energy threshold ( ~1 keV) of the detector will allow it to observe neutrinos from core-collapse supernovae (CCSN) via coherent elastic neutrino-nucleus scattering (CEνNS). In this way, DarkSide-20k will produce a flavour-blind measurement of the unoscillated neutrino flux from a CCSN providing the normalisation for current and future giant detectors which are mostly sensitive to electron (anti-)neutrinos. In addition, DS-20k will be able to join the network of the SuperNova Early Warning System 2.0 (SNEWS2.0), providing additional input for triangulating core-collapse supernovae.

Primary authors

Giuseppe Matteucci (Istituto Nazionale di Fisica Nucleare) Roberta Calabrese (Istituto Nazionale di Fisica Nucleare)

Presentation materials

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