XXth International Conference on Neutrino Physics and Astrophysics
M.Selvi
Large Volume Detector at LNGS and Neutrino Oscillation
We study the impact of the LVD detector in the neutrino oscillation
scenario. LVD is optimised to detect neutrinos from supernova
explosion in the galaxy. The possibility to detect neutrinos in
different channels makes LVD sensitive to different scenarios for n
properties, such as normal or inverted n mass hierarchy, and adiabatic
or non-adiabatic MSW resonances associated to Ue3. Moreover, the
performances of the LVD detector as a useful monitor for the CNGS beam
are studied and presented. The detector efficiencies and expected
number of muons, due to neutrino interactions in the rock before LNGS,
are calculated using a full simulation of the neutrino CC interaction,
of the transport mechanism through the rock and of the detector
response.
Based on
"Effects of neutrino oscillations on the supernova signal in LVD"
[astro-ph/0112312]
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