Author/Authors :
Agafonova، نويسنده , , N.Yu. and Aglietta، نويسنده , , M. and Antonioli، نويسنده , , P. Di Bari، نويسنده , , G. and Boyarkin، نويسنده , , V.V. and Bruno، نويسنده , , G. and Fulgione، نويسنده , , W. and Galeotti، نويسنده , , P. and Garbini، نويسنده , , M. and Ghia، نويسنده , , P.L. and Giusti، نويسنده , , P. and Kemp، نويسنده , , E. and Kuznetsov، نويسنده , , V.V. and Kuznetsov، نويسنده , , V.A. and Malguin، نويسنده , , A.S. and Menghetti، نويسنده , , H. and Pesci، نويسنده , , A. and Pless، نويسنده , , I.A. and Porta، نويسنده , , A. and Ryasny، نويسنده , , V.G. and Ryazhskaya، نويسنده , , O.G. Morales-Saavedra، نويسنده , , O. and Sartorelli، نويسنده , , G. and Selvi، نويسنده , , M. and Vigorito، نويسنده , , C. and Vissani، نويسنده , , F. and Votano، نويسنده , , L. and Yakushev، نويسنده , , V.F. and Zatsepin، نويسنده , , G.T. and Zichichi، نويسنده , , A.، نويسنده ,
Abstract :
The LVD detector, located in the INFN Gran Sasso National Laboratory (Italy), studies supernova neutrinos through the interactions with protons and carbon nuclei in the liquid scintillator and interactions with the iron nuclei of the support structure. We investigate the effect of neutrino oscillations in the signal expected in the LVD detector. The MSW effect has been studied in detail for neutrinos travelling through the collapsing star and the Earth. We show that the expected number of events and their energy spectrum are sensitive to the oscillation parameters, in particular to the mass hierarchy and the value of θ 13 , presently unknown. Finally we discuss the astrophysical uncertainties, showing their importance and comparing it with the effect of neutrino oscillations on the expected signal. We do not discuss in this paper the determination of oscillation parameters from the results of the observations; this task seems to be very difficult until astrophysical uncertainties are significantly reduced.