Gamow-Teller strength function in Ge-71 via the (p,n) reaction at medium energies

Details Gamow-Teller strength function in Ge-71 via the (p,n) reaction at medium energies Gamow-Teller strength function in Ge-71 via the (p,n) reaction at medium energies

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985phrvl..55.1051k&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 55, Sept. 2, 1985, p. 1051-1054. Research supported by the Statens Naturvidenskab

Physics

50

Absorption Cross Sections, Capture Effect, Germanium, Solar Neutrinos, Solar Physics, Stellar Models, Gallium, Radioactive Decay

Scientific paper

The Gamow-Teller strength function in Ge-71 has been measured by use of the reaction Ga-71 (p,n) at E(p) = 120 and 200 MeV. While a significant fraction of the total strength is associated with excited states located below particle-emission threshold, the first excited state exhibits little strength. Excited-state contributions to the total solar-neutrino capture rate for a Ga-71 detector are about 14 solar neutrino units for the neutrino spectrum of the standard solar model and about 3-4 solar neutrino units for representative nonstandard solar models.

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