Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-11-16
Phys.Atom.Nucl.70:140-149,2007
Astronomy and Astrophysics
Astrophysics
10 LaTex pages, 11 post script figures. To appear in the proceedings of NANP05, Dubna, Russia
Scientific paper
10.1134/S1063778807010164
Supernova neutrinos can easily be detected by a spherical gaseous TPC detector measuring very low energy nuclear recoils. The expected rates are quite large for a neutron rich target since the neutrino nucleus neutral current interaction yields a coherent contribution of all neutrons. As a matter of fact for a typical supernova at 10 kpc, about 1000 events are expected using a spherical detector of radius 4 m with Xe gas at a pressure of 10 Atm. A world wide network of several such simple, stable and low cost supernova detectors with a running time of a few centuries is quite feasible.
Giomataris Y.
Vergados John D.
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