Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-12-17
Phys.Lett. B530 (2002) 27-32
Astronomy and Astrophysics
Astrophysics
7 pages, 1 figure
Scientific paper
10.1016/S0370-2693(02)01349-7
We show that supernova neutrinos can be studied by observing their charged-current interactions with $^{100}$Mo, which has strong spin-isospin giant resonances. Information about both the effective temperature of the electron neutrino sphere and the oscillation into electron neutrinos of other flavors can be extracted from the electron (inverse $\beta$) spectrum. We use measured hadronic charge-exchange spectra and the Quasiparticle Random Phase Approximation to calculate the charged-current response of $^{100}$Mo to electron neutrinos from supernovae, with and without the assumption of oscillations. A scaled up version of the MOON detector for $\beta \beta$ and solar-neutrino studies could potentially be useful for spectroscopic studies of supernova neutrinos as well.
Ejiri Hiro
Engel Johannes
Kudomi Nobuyuki
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