Nuclear responses for solar-ν, supernova-ν and ββ-ν

Details Nuclear responses for solar-ν, supernova-ν and ββ-ν Nuclear responses for solar-ν, supernova-ν and ββ-ν

Jun 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..570..881e&link_type=abstract

The fourteenth international spin physics symposium, SPIN2000. AIP Conference Proceedings, Volume 570, pp. 881-881 (2001).

Physics

Neutrino Scattering, Weak-Interaction And Lepton Aspects, 90<=A<=149, Spin, Parity, And Isobaric Spin

Scientific paper

Nuclear weak responses for neutrinos in nuclei, which are mainly axial vector spin isospin responses, are crucial for neutrino studies in nuclei. Nuclear spin isospin responses for solar-ν, supernova-ν, and ββ-ν have been studied by using charge-exchange spin-flip reactions. 100Mo is found to have large responses for these neutrinos. Then MOON(Mo Observatory Of Neutrinos) composed of supermodules of scintillators and 100Mo isotopes is used for real-time studies of low energy solar-ν and supernova-ν and for spectroscopic studies of ββ-ν with a ν-mass sensitivity of 0.03 eV. .

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