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Event Type High Energy Experimental Seminar
Date and Time 28-Mar-2008  from 11:10 to 12:00
Location MP912
Host John Martin

HALO - Helium and Lead Observatory for Supernova Neutrinos

Stan Yen

TRIUMF

halo_poster.jpg Existing neutrino detectors are mostly of the water Cerenkov and liquid scintillator types, which are primarily sensitive to electron anti-neutrinos via charged-current interactions on the hydrogen nuclei in these materials. By contrast, the large neutron excess of a heavy nucleus like Pb acts to Pauli-block p→n transitions induced by electron anti-neutrinos, making it primarily sensitive to electron neutrinos. This channel is expected to show the most interesting effects of flavour-swapping and spectral splitting due to MSW-like collective neutrino-neutrino interactions in the core of the supernova, the only place in the universe where there is a sufficient density of neutrinos for this to occur. The observation of a galactic core-collapse supernova by a Pb-based neutrino detector, as a complement to other neutrino detectors, would provide a wealth of data for both particle physicists and astrophysicists. The data would provide a test for θ 13 ≠0 and an inverted neutrino mass hierarchy, and the ratio of 1-neutron to 2-neutron events would be a measure of the temperature of the cooling neutron star. HALO is a detector of opportunity proposed for SNOLAB, which will utilize 80 tons of surplus Pb blocks, together with the neutral-current detectors from the SNO experiment and the SNO data acquisition system, to provide a low-cost, low-maintenance, long-lived, high-livetime detector. A supernova at 10 kpc would result in 43 neutrons in the absence of collective ν-ν interactions, and many more in their presence. A future upgrade to 1 kiloton would be sensitive to supernova anywhere in our galaxy.

Contact Info
Name John Martin
Email martin@physics.utoronto.ca
Phone 8-2954

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