Abstract
It is been shown previoulsy that the existence of a tiny abundance of nuclei which have an additional embedded hadronic particle, $Q$-nuclei, can solve the solar-neutrino problem. We present here detailed predictions of solar-neutrino detection rates for detectors of $^{37}\mathrm{Cl}$, $^{71}\mathrm{Ga}$, and $^{115}\mathrm{In}$. It is found that, while $Q$-nuclei could reduce the $^{37}\mathrm{Cl}$ detection rate from that of the standard model to the experimental value, they would also produce a dramatic increase in the rates for the $^{71}\mathrm{Ga}$ and $^{115}\mathrm{In}$ detectors.
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