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Using the Double Chooz detector, designed to measure the neutrino mixing angle θ₁₃, the products of μ^- capture on ¹²C,¹³C,¹⁴N, and ¹⁶O have been measured. Over a period of 489.5 days, 2.3×10⁶ stopping cosmic μ^- have been collected, of which 1.8×10⁵ captured on carbon, nitrogen, or oxygen nuclei in the inner detector scintillator or acrylic vessels. The resulting isotopes were tagged using prompt neutron emission (when applicable), the subsequent β decays, and, in some cases, β-delayed neutrons. The most precise measurement of the rate of ¹²C(μ^-,ν)¹²B to date is reported: 6.57_-0.21+0.11×10³0.28em0exs^-1, or (17.35_-0.59+0.35)% of nuclear captures. By tagging excited states emitting γs, the ground state transition rate to ¹²B has been determined to be 5.68_-0.23+0.14×10³0.28em0exs^-1. The heretofore unobserved reactions $¹²C({{μ}}^{{-}},{ν}{α})⁸Li,¹³C({{μ}}^{{-}},{ν}n{α})⁸Li$, and $¹³C({{μ}}^{{-}},{ν}n)¹²B$ are measured. Further, a population of ${β}n$ decays following stopping muons is identified with $5.5{σ}$ significance. Statistics limit our ability to identify these decays definitively. Assuming negligible production of $⁸He$, the reaction $¹³C({{μ}}^{{-}},{ν}{α})⁹Li$ is found to be present at the $2.7{σ}$ level. Limits are set on a variety of other processes.
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Abrahão et al. (2016) studied this question.
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