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- W2021215510 abstract "A search for a $^{3}mathrm{He}$ + $^{3}mathrm{He}$ resonance just above threshold was made by means of the reaction $^{6}mathrm{Li}(^{3}mathrm{He},t)^{6}mathrm{Be}^{*}$ with 46.3-MeV $^{3}mathrm{He}$. No resonance was found; the c.m. cross section is ensuremath{le}1.6 ensuremath{mu}b/sr at 8.4ifmmode^circelsetextdegreefi{} c.m. This corresponds to an upper limit on the spectroscopic factor for $^{6}mathrm{Be}^{*}ensuremath{rightarrow}^{3}mathrm{He}+^{3}mathrm{He}$ of 0.0003 to 0.001, depending on the parameters adopted for a distorted-wave Born-approximation calculation. The maximum possible effect of such a resonance on the production of high-energy solar neutrinos is too small to explain the discrepancy between solar-model predictions and the experimental results of Davis et al.[NUCLEAR REACTIONS: $^{6}mathrm{Li}(^{3}mathrm{He},t)$, $E=46.3$ MeV; measured $ensuremath{sigma}({E}_{t},ensuremath{theta}={5}^{ensuremath{circ}})$. Deduced: no $^{3}mathrm{He}$-$^{3}mathrm{He}$ resonance in $^{6}mathrm{Be}$.]" @default.
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- W2021215510 date "1973-10-01" @default.
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- W2021215510 title "Li6(He3,t)Reaction and the Solar Neutrino Puzzle" @default.
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- W2021215510 doi "https://doi.org/10.1103/physrevc.8.1226" @default.
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