Nuovo Cim. 111A, 835 (1998)

M.Lewitowicz, W.Trinder, M.Bhattacharya, E.G.Adelberger, J.C.Angelique, R.Anne, J.Aysto, C.Borcea, J.M.Daugas, C.Donzaud, A.Garcia, S.Grevy, R.Grzywacz, D.Guillemaud-Mueller, A.Jokinen, N.I.Kaloskamis, S.Leenhardt, M.J.Lopez, A.C.Mueller, F.de Oliveira, A.Ostrowski, F.Pougheon, M.G.Saint-Laurent, T.Siiskonen, O.Sorlin, H.E.Swanson

Beta-Decay of Light Nuclei Close to the Proton Drip-Line: ⁴⁰Ti and ³⁵Ca

RADIOACTIVITY ⁴⁰Ti, ³⁵Ca(β⁺) [from Ni(⁵⁰Cr, X), (⁴⁰Ca, X)]; measured β-delayed proton spectra, Eγ, T_1/2, B(F), B(GT). ³⁵K deduced IAS. Implications for solar neutrino detector efficiency discussed.