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Solar-Neutrino Detection: Experimental Determination of Gamow-Teller Strengths via the Mo98 and In115 (p, n) Reactions

J. Rapaport and P. Welch

J. Bahcall

E. Sugarbaker

T. N. Taddeucci

C. D. Goodman and C. F. Foster

D. Horen

C. Gaarde and J. Larsen

T. Masterson

  • Ohio University, Athens, Ohio 45701

  • Institute for Advanced Study, Princeton, New Jersey 08540

  • Ohio State University, Columbus, Ohio 43210

  • Ohio University, Athens, Ohio 45701, and Indiana University, Bloomington, Indiana 47405

  • Indiana University, Bloomington, Indiana 47405

  • Oak Ridge National Laboratory, Oak Ridge, Tennessee 37830

  • Niels Bohr Institute, DK-2100, Copenhagen, Denmark

  • University of Colorado, Boulder, Colorado 80309

Phys. Rev. Lett. 54, 2325 – Published 27 May, 1985

DOI: https://doi.org/10.1103/PhysRevLett.54.2325

Abstract

The empirical distributions of Gamow-Teller strengths in Tc98 and Sn115 have been obtained via the (p, n) reaction at Ep=120 MeV and Ep=200 MeV on Mo98 and In115 targets. This information is used to calculate the cross sections for absorption of solar neutrinos in Mo98 and In115, nuclides which are being considered as neutrino detectors to accomplish solar-neutrino spectroscopy.

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