Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2003-11-13
JCAP 0401 (2004) 004
Physics
High Energy Physics
High Energy Physics - Phenomenology
17 pages, 9 figures
Scientific paper
10.1088/1475-7516/2004/01/004
The Earth matter effects on supernova (SN) neutrinos can be identified at a single detector through peaks in the Fourier transform of their ``inverse energy'' spectrum. The positions of these peaks are independent of the SN models and therefore the peaks can be used as a robust signature of the Earth matter effects, which in turn can distinguish between different neutrino mixing scenarios. Whereas only one genuine peak is observable when the neutrinos traverse only the Earth mantle, traversing also the core gives rise to multiple peaks. We calculate the strengths and positions of these peaks analytically and explore their features at a large scintillation detector as well as at a megaton water Cherenkov detector through Monte Carlo simulations. We propose a simple algorithm to identify the peaks in the actual data and quantify the chances of a peak identification as a function of the location of the SN in the sky.
Dighe Amol S.
Kachelriess Michael
Raffelt Georg
Tomas Ricard
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