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June 22, 2020 to July 2, 2020
US/Central timezone

HALO-1kT and other supernova detectors

Not scheduled
10m

Speaker

Dr Andrea Gallo Rosso (Laurentian University)

Description

When the next galactic supernova explodes, we'll need to be ready to get the most of its neutrino signal. HALO-1kT is a 1 kton lead-based supernova detector that will be possibly be built at Laboratori Nazionali del Gran Sasso (LNGS) in Italy. Its sensitivity to Charged-Current electron neutrinos makes it complementary to most of the other supernova detectors, mainly based on water or liquid scintillator. In the present work, we implement multi-dimensional, Monte Carlo based likelihood analyses in order to assess the contribution HALO-1kT can give in reconstructing the detected time-integrated fluxes (fluences) both alone or combined with two major supernova detectors as Super-Kamiokande and the Jiangmen Underground Neutrino Observatory (JUNO).

Mini-abstract

Proposed HALO-1kT is a robust detector that could help constrain the $\nu_\mathrm{e}$ fluence.

Experiment/Collaboration HALO-1kT collaboration

Primary author

Dr Andrea Gallo Rosso (Laurentian University)

Presentation Materials