Effects of neutrino oscillations on the supernova signal in LVD

Details Effects of neutrino oscillations on the supernova signal in LVD Effects of neutrino oscillations on the supernova signal in LVD

2001-12-13

arxiv.org/abs/astro-ph/0112312v1

Nucl.Phys.Proc.Suppl. 110 (2002) 410-413

Astronomy and Astrophysics

Astrophysics

4 pages, 3 figures. Presented at TAUP 2001 (7th international workshop on Topics in Astroparticle and Underground Physics), Se

Scientific paper

We study the impact of neutrino oscillations on the supernova neutrino signal in the Large Volume Detector (LVD). The number of expected events for a galactic supernova (D=10 kpc) is calculated, assuming neutrino masses and mixing that explain solar and atmospheric neutrino results. The possibility to detect neutrinos in different channels makes LVD sensitive to different scenarios for neutrino properties, such as normal or inverted neutrino mass hierarchy, and/or adiabatic or non adiabatic MSW resonances associated to U(e3). Of particular importance are the charged current reactions on carbon: oscillations increase by almost one order of magnitude the number of events expected from this channel.

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