TY - JOUR
T1 - Solar neutrinos and low-energy nuclear cross sections
AU - Bahcall, J. N.
AU - Bahcall, N. A.
AU - Fowler, W. A.
AU - Shaviv, G.
N1 - Funding Information:
* Supported in part by the National Science Foundations [GP-7976, formerly GP-53911 and by the Office of Naval Research [Nonr-220(47)]. ** Also at Tel Aviv University, Tel Aviv, Israel. $ Supported by the National Science Foundation [GP-69281 with Cornell University.
Copyright:
Copyright 2017 Elsevier B.V., All rights reserved.
PY - 1968/2/19
Y1 - 1968/2/19
N2 - The rate of capture of solar neutrinos per 37Cl atom is found to be 0.7 × 10-35 sec-1 and 4.9 × 10-35 sec-1 for two extreme assumptions regarding the measured low-energy nuclear cross sections. The dependence of the 8B solar neutrino flux on the low-energy cross-section factor for 3He(α,γ)7Be, S34 is found to be S340.7.
AB - The rate of capture of solar neutrinos per 37Cl atom is found to be 0.7 × 10-35 sec-1 and 4.9 × 10-35 sec-1 for two extreme assumptions regarding the measured low-energy nuclear cross sections. The dependence of the 8B solar neutrino flux on the low-energy cross-section factor for 3He(α,γ)7Be, S34 is found to be S340.7.
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U2 - 10.1016/0370-2693(68)90610-2
DO - 10.1016/0370-2693(68)90610-2
M3 - Article
AN - SCOPUS:49949128257
SN - 0370-2693
VL - 26
SP - 359
EP - 361
JO - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
JF - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
IS - 6
ER -