Nuclear responses of ^100Mo for low energy ν's, and the MOON Project.

Details Nuclear responses of ^100Mo for low energy ν's, and the MOON Project. Nuclear responses of ^100Mo for low energy ν's, and the MOON Project.

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aps..haw.kc009e&link_type=abstract

American Physical Society, First Joint Meeting of the Nuclear Physicists of the American and Japanese Physical Societies October

Physics

Scientific paper

^100Mo is shown to have large responses for β β ν , low energy solar ν, and supernova ν . This is due to large spin-isospin strengths and large phase-space volumes. The charged-current weak responses were evaluated on the basis of the spin-isospin strengths measured by charge-exchange hadronic reactions. Thus MOON (Mo Observatory Of Neutrinos) provides opportunities for highly sensitive studies of the Majorana ν mass by the neutrinoless β β decay of ^100Mo and low-energy solar and supernova ν 's by the inverse β decay of ^100Mo.

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