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@@ -22,20 +22,26 @@ was made. The main results are:
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\item obtaining preliminary results on proton emission rate and spectrum:
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the proton spectrum has a peak at \SI{3.7}{\MeV}, then reduces exponentially
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with a decay constant of \SI{2.6}{\MeV}. The partial emission rate in the
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energy range from \SIrange{4}{8}{\MeV} is $(1.7 \pm 0.1)\%$, and the total
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energy range from \SIrange{4}{8}{\MeV} is $(1.7 \pm 0.1)\%$ per nuclear
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muon capture, and the total
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emission rate assuming the shape holds for the whole spectrum is
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$(3.5\pm0.2)\%$.
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$(3.5\pm0.2)\%$ per nuclear muon capture.
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\end{enumerate}
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The emission rate is consistent with the lower limit of 2.8\% set by
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Wyttenbach et al.~\cite{WyttenbachBaertschi.etal.1978}. It is also compatible
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with the theoretical calculation by Lifshitz and
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Singer~\cite{LifshitzSinger.1980}. Compared with the emission rate from
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silicon, our result is smaller.
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Singer~\cite{LifshitzSinger.1980}. Compared with the existing result on
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silicon~\cite{SobottkaWills.1968}, the emission rate from aluminium is
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significantly smaller and the spectrum is softer.
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The proton rate and spectrum have been used to optimise the planned proton
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absorber for the drift chamber of the COMET Phase-I. The resulted proton hit
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rate with the baseline configuration is very small compared with the current
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figure. It is safe to remove the proton absorber altogether. This would make
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a strong impact to the drift chamber design. The AlCap experiment is going to
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figure.The recommendation to the COMET Phase-I is to remove the proton
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absorber altogether. The momentum resolution of the drift chamber will be
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slightly improved, and the level of integrated charge will still remain below
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the safe level for the chamber.
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The AlCap experiment is going to
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submit a beam time request for the 2015 run to collect more data and other
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measurements for neutrons and gamma rays.
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