15–21 Oct 2017
Monastero dei Benedettini, University of Catania, Catania, Italy
Europe/Rome timezone
Proceedings published online

The HALO and HALO-1kT Supernova Detectors

20 Oct 2017, 12:00
30m
Auditorium (Monastero dei Benedettini, University of Catania)

Auditorium

Monastero dei Benedettini, University of Catania

Oral Plenary

Speaker

Dr Clarence Virtue (Laurentian University / SNOLAB)

Description

This talk will present the case for lead-based supernova detectors.  Such detectors are robust and economical to build and maintain over long timescales. By instrumenting tonnes of lead with He-3 neutron detectors supernova neutrinos create bursts of neutrons which can be detected with high efficiency. Electron anti-neutrino charged current reactions are Pauli-blocked by the neutron excess in lead. Neutrons from neutral current and electron neutrino charged current excitations provide complimentary sensitivity to water Cherenkov and liquid scintillator-based detectors.  The HALO detector, constructed with 79 tonnes of lead, has been running at SNOLAB since May 2012. HALO-1kT is a proposal for a scaled up detector which would utilize 1000 tonnes of INFN lead from the decommissioned OPERA detector. With increased mass and improved neutron capture efficiency HALO-1kT would provide over a 20-fold increase in event statistics from the next galactic supernova.

Primary author

Dr Clarence Virtue (Laurentian University / SNOLAB)

Presentation materials