360 lines
16 KiB
TeX
360 lines
16 KiB
TeX
\documentclass[12pt]{article}
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\usepackage{latexsym,multicol,graphicx,rotating}
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\usepackage{hyperref}
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\usepackage{booktabs}
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\usepackage{tabularx}
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\usepackage[compact]{titlesec}
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\usepackage{wrapfig}
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\hypersetup{
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colorlinks = false,
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linkcolor = red,
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linktoc=page,
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linkbordercolor={1 0 0}
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%linkcolor=blue,
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}
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\oddsidemargin 0.0in
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\textwidth 6.5in
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\headheight 0.0in
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\topmargin 0.0in
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\textheight 9.0in
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\parindent 0in
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%%%%%%%%%%%%% user's command definitions
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%\setlength{\textwidth}{16cm}
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\newcommand{\ttbs}{\char'134}
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\newcommand{\AmS}{{\protect\the\textfont2
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A\kern-.1667em\lower.5ex\hbox{M}\kern-.125emS}}
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\newcommand{\lagr}{\cal{L}}
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\newcommand{\mueg}{$\mu^{+} \rightarrow e^{+}\gamma$~}
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\newcommand{\meee}{$\mu \rightarrow eee$~}
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\newcommand{\muenn}{$\mu \rightarrow e \nu \overline{\nu}$~}
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\newcommand{\muenng}{$\mu \rightarrow e \nu \overline{\nu} \gamma$~}
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\newcommand{\muec}{$\mu^{-} N \rightarrow e^{-} N$~}
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%%%%%%%%%%%%%%%%%%%%%%%%%%% Begin
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\begin{document}
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%\title{Proposal}
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%\author{Alcap}
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%\maketitle
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%\newpage
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%%%%%%%%%%%%%%%%%%%%%%%%%%% TOC
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%\tableofcontents
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%\newpage
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%%%%%%%%%%%%%%%%%%%%%%%%%%%
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\section{Scientific background and aim of the experiment}
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\label{sec:motivation}
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\subsection{Scientific background}
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Charged lepton flavor violation (CLFV) has yet to be observed and is known to
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be sensitive to new physics beyond the Standard Model (SM). The J-PARC E12
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experiment, COMET~\cite{come07}, is a new experiment to search for a CLFV process of
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neutrinoless muon-to-electron conversion in presence of a nucleus (\muec).
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Utilising multi-kW pulsed 8$-$9 GeV proton beams, COMET can achieve a branching
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ratio sensitivities lower than 10$^{-16}$, that is 10,000 better than current
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best limit established by SINDRUM II~\cite{sindrumii}.
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Recently, COMET collaboration has adopted a staged approach, in which the COMET
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Phase--I~\cite{phaseI12}, with a partial muon transport solenoid, will
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have physics runs in 2016. The tracking chamber for COMET Phase--I are designed
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to measure charged particles of their momenta in the range from 70 MeV/$c$ to
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105 MeV/$c$.
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In that momentum range, single hit
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rate of the tracking chamber would be dominated by protons after nuclear muon
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capture. In order to limit the single hit rate to an
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acceptable level, a proton absorber would be installed in
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front of the tracking chambers to reduce proton hit rate. However, the proton
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absorber would deteriorate the reconstructed momentum resolution of electrons
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at birth. And similarly the rate of proton emission is important to determine
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thickness of the muon stopping target made of aluminum. Therefore it is
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important to know the rate so that the detector system can be optimized in
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terms of both hit rate and momentum resolution.
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%Mu2e will be subject to significant backgrounds from the products of the
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%nuclear capture
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%process. Among them, the background for protons is a particularly acute one.
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%, and its detailed
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%investigation is the subject of this proposal, which is a joint proposal on
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%behalf of both the Mu2e and COMET collaborations.
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%The tracking chambers of COMET Phase--I~\cite{phaseI12} and Mu2e are designed
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%to be measure charged particles of their momenta greater than 70 MeV/$c$ and 53
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%MeV/$c$ respectively.
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\subsection{Goal of the experiment}
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The goal of the experiment is to measure the rate and energy spectra of the
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protons emitted after a muon is captured on aluminum and silicon targets.
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A precision of 5\% in the range from 3 to 6 MeV (momentum from 75 MeV/$c$ to
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105 MeV/$c$) is required for both the rate and the energy spectra.
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\subsection{Urgency}
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The construction of
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COMET experimental hall has started in 2013, a prototype of the tracking
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chamber is being designed, and chamber contruction should be finished by the
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end of 2015.
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The COMET collaboration needs to complete the final detector design as soon as
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possible. Therefore, measurements of proton emission rates and spectrum that
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can be done as early as possible become one of the critical path for the both
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experiments.
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% section motivation (end)
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%%%%%%%%%%%%%%%%%%%%%%%%%%%
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\section{Present status of the research}
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At present, the yield, energy spectrum and composition of the charged
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particles emitted in muon capture on aluminum have not been measured in the
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relevant energy range for COMET Phase--I.
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Figure~\ref{fg:silicon-proton} shows the spectrum of charged particle emission
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from muons being stopped and captured in a silicon detector \cite{sobo68}. The
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peak below 1.4 MeV is from the recoiling heavy ions, mainly $^{27}$Al, when no
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charged particles were emitted. Hungerford~\cite{hung34} fitted the silicon
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spectrum in Fig.~\ref{fg:silicon-proton} with an empirical function given by
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%
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\begin{equation} p(T) = A(1-{T_{th} \over T})^{\alpha} e^{-(T/T_0)}
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\label{eq:protons} \end{equation}
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%
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\begin{wrapfigure}{l}{0.5\textwidth}
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\vspace{-10pt}
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\centering
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\includegraphics[width=0.48\textwidth]{figs/si-proton.pdf}
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\caption{Charged particle spectrum from muon capture on an active silicon
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target~\cite{sobo68}.}
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\label{fg:silicon-proton}
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\vspace{-10pt}
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\end{wrapfigure}
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where $T$ is the kinetic energy and the fitted parameters are $A=0.105$
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MeV$^{-1}$, $T_{th}$ = 1.4 MeV, $\alpha$=1.328 and $T_0$ = 3.1 MeV. The
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spectrum is normalized to 0.1 per muon capture. Some other results in the past
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experiments are summarized in a comprehensive review by D.F.
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Measday~\cite{measday}.
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%\begin{figure}[tb] \centering
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%\includegraphics[width=0.7\textwidth]{figs/si-proton.pdf} \caption{charged
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%particle spectrum from muons stopping and being captured in a silicon
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%detector~\cite{sobo68}.} \label{fg:silicon-proton} \end{figure}
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%\begin{wrapfigure}{l}{0.5\textwidth}
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%\vspace{-25pt}
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%\begin{center}
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%\includegraphics[width=0.48\textwidth]{figs/si-proton.pdf}
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%\end{center}
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%\vspace{-20pt}
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%\caption{Charged particle spectrum from muon capture on an active silicon
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%target ~\cite{sobo68}.}
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%\label{fg:silicon-proton}
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%\vspace{-10pt}
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%\end{wrapfigure}
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%\begin{table}[tb]
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%\centering \caption{Probabilities in unites of $10^{-3}$ per
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%muon capture for inclusive proton emission calculated by Lifshitz and Singer.
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%The numbers in crescent parenthesis are estimates for the total inclusive
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%rate derived from the measured exclusive channels by the use of the
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%approximate regularity, such as $(\mu, \nu p):(\mu, \nu p n):(\mu, \nu p
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%2n):(\mu. \nu p 3n) = 1:6:4:4$.}\label{tb:proton} \vskip 3mm
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%\begin{tabularx}{\textwidth}{|c|c|c|c|X|}\hline Target nucleus & Calculation & Experiment
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%& Estimate & Comments \\ \hline $_{10}$Ne & & $200\pm 40$ & & \\
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%$^{27}_{13}$Al & 40 & $>28 \pm 4$ & (70) & 7.5 for $T>40$ MeV \\
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%$^{28}_{14}$Si & 144 & $150\pm30$ & & 3.1 and 0.34 $d$ for $T>18$ MeV \\
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%$^{31}_{15}$P & 35 & $>61\pm6$ & (91) & \\ $^{46}_{22}$Ti & & & & \\
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%$^{51}_{23}$V & 25 & $>20\pm1.8$ & (32) & \\ \hline \end{tabularx}
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%\end{table}
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The limited information available makes it difficult to draw
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quantitative conclusive detector design. At this moment
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the above analytical spectrum has been used to estimate proton
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emission in COMET Phase--I detector designs.
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For this measurement, a DC muon beam, such as at TRIUMF or PSI, is the best
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choice. A test experiment has been conducted at PSI in 2009 by Mu2e, but
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without a conclusive result. We have discussed with them to have a better
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understanding of the instrumentations and possible backgrounds involved. An
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experiment similar to the one in 2009 is scheduled at PSI in the end of
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2013. This is a joint effort of the two collaborations, COMET and Mu2e.
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The experiment in this proposal could serve two purposes: (a) cross check
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for the PSI experiment, and (b) back up plan in case that the PSI experiment
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could not be carried out.
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\section{Experimental method} % (fold) \label{sec:expdescpription}
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\begin{wrapfigure}{r}{0.4\textwidth}
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\centering
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\includegraphics[width=0.38\textwidth]{figs/setup_gr}
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\caption{Schematic layout of the experimental setup}
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\label{fg:setup}
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\vspace{-10pt}
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\end{wrapfigure}
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A schematic layout of the experimental setup is shown in Fig.~\ref{fg:setup}.
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Low energy negative muons (28 MeV/$c$) will enter a vacuum vessel
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though a thin mylar window, and will be stopped in passive Al foils of 25
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-- 200 $\mu m$
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thickness, positioned under 45 degrees to the beam direction.
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As a cross check, an active silicon target of 140 $\mu m$ will also be used.
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A long duct is prepared to avoid potential background from muons that are not
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stopped in the target.
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Two packages
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of charged particle detectors are positioned on opposite sides, parallel
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to the target surface. The thin Si detectors (65 $\mu m$) will provide dE/dx
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information. The thick Si detectors (1500 $\mu m$) stop protons up to about 12
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MeV. According to a simple Geant4 simulation, we can use dE/dx method to do
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PID (Fig.~\ref{fg:dedx}).
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%Plastic scintillators positioned
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%behind these Si detector observe potential higher energy protons and veto
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%through--going electrons.
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The symmetry
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between the left and right Si stations allows for a powerful monitor of
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systematic effects. Differences between the detectors would indicate background
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due to different stopping material, non--uniform stopping distribution or
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differences due to muon scattering.
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Muon bunch signal will be used as the trigger for the DAQ system. The DAQ
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system collects data in a fixed period of time after this trigger.
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Timing and energy information from silicon detectors will be read out by
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flash ADCs (FADC).
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Particle identification can also be done using TOF method. In this case,
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extended pipes need to be connected to the chamber, and distance between dE and
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E detectors would be increased to about 15 cm.
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Careful shielding of direct or scattered
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muons is required, as the stopping fraction is small and proton emission is a
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rare capture branch. As shown, we are considering a geometry, where there is no
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direct line of sight between any low Z material exposed to muons, with all
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shielding done with lead.
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In order to normalize a number of muons stopping in the aluminum target, a
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germanium detector to measure muonic X-rays from muons stopping in the aluminum
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target is installed.
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\begin{wrapfigure}{r}{0.4\textwidth}
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\centering
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\includegraphics[width=0.38\textwidth]{figs/dEdx-mlf}
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\caption{PID using two silicon detectors: 65 $\mu m$ and 1500 $\mu m$ thick}
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\label{fg:dedx}
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\vspace{-10pt}
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\end{wrapfigure}
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The main systematic issues are as follows.
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\begin{itemize}
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\setlength{\itemsep}{1pt}
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\setlength{\parskip}{0pt}
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\setlength{\parsep}{0pt}
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\item Deconvolute the orginal proton spectrum $f(T_i)$: the use of an active
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Si target allow the experimental calibration of the response function,
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because both initial energy $T_i$ and final energy $T_f$ of protons are
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accessible.
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\item Absolute calibration: the number of
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muon stops will be determined with
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the Ge detector. Again, the use of an active Si target allows for a cross
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calibration. The proton detection efficiency will be simulated by Geant4 and
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calibrated with the active Si target.
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\item The PID of emitted charged particles will be determined by dE/dx.
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\item Background: a dangerous background comes from muons stop in walls and
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scatter into the Si detectors.
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\end{itemize}
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%A realistic Geant4 simulation is being developed. It will serve as an important
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%tool to optimize the geometry, in particular regarding background and response
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%function. Currently the geometry of the PSI test run is being implemented for a
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%realistic check of the simulation.
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%We have a vacuum chamber and Si detectors, which were used for a
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%similar measurement done at PSI in 2009. For a coming beam test, the
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%vacuum chamber is being tested now at University of Washington
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%(UW). The two exiting Si detectors are also being tested at UW. A
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%possibility to prepare another set of Si detectors is being
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%sought. Amplifiers for the existing Si detects are available. The
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%Osaka University (OU) group is preparing DAQ system based on a PSI
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%standard data acquisition system (MIDAS). The OU group is making
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%arrangement of getting a Ge detector for muonic X-ray measurement,
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%either borrowing from someone or purchasing a new one. Monte Carlo
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%simulations necessary to optimize detector configuration is undergoing
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%at OU and University College London (UCL).
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%Some test beam run to examine a number of muons of low momentum is
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%being requested in September, 2012 and
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%will be performed with a simplified set-up. The full set-up will be
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%ready beginning December 2012.
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%\begin{figure}[htb]
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%\begin{center}
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%\includegraphics[width=0.9\textwidth]{figs/dedx.png}
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%\caption{2-dim. plots of
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%S1 (vertical) vs S2 (horizontal) counters. The plot in top left is for all
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%charged particles. The ones in top right, bottom left and bottom right are
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%for only protons, proton+deuteron, proton+deuteron+muons.}
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%\label{fg:dedx}
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%\end{center}
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%\end{figure}
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%Figure~\ref{fg:dedx} shows Monte Carlo simulation studies of two-dimensional
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%plots of energy of the S1 counter (dE/dX) vs. energy of the S2 counter. From
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%Fig.~\ref{fg:dedx}, it is clearly seen that we can discriminate protons,
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%deuterons and scattered muons and electrons by this particle identification
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%method. And the range of proton energy from 2.5 MeV to 20 MeV can be detected.
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%The event rates are estimated based on Monte Carlo simulation. Preliminary
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%results are summarized in Table~\ref{tb:rates}. They will be updated once we
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%have full information about the PSI beam properties. As seen in
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%Table~\ref{tb:rates}, proton rates of $T>2.5$ MeV are not large. A muon beam
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%whose momentum is low and momentum width is narrow is of critical importance.
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%And also a ratio of signal to background is 1:50. Therefore, a good particle
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%identification is important. From Monte Carlo simulation, a combination of
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%dE/dX and E counters has a sufficient capability of discriminating protons from
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%the other charged particles.
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% section expdescpription (end)
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%%%%%%%%%%%%%%%%%%%%%%%%%%%
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\section{Beam time estimation}
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We are requesting a 6--day beam time (two consecutive blocks). This is based on
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the estimation as follows:
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\begin{itemize}
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\setlength{\itemsep}{1pt}
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\setlength{\parskip}{0pt}
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\setlength{\parsep}{0pt}
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\item 1 days of beam tuning and adjustment of electronics,
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\item 5 days of data taking: the proton hit rate on the detectors estimated
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by the Geant4 simulation is $2 \times 10^{-3}$ per muon bunch. We want to
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accumulate 5000 events in 20 bins from 3 MeV to 6 MeV, that means 10000
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proton events in total. So, we will need $5 \times 10^{6}$ bunches, or $2
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\times 10^5$ seconds = 2.3 days ( at 25 Hz beam frequency) for one sample. We
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intend to have two measurements with two targets: active silicon, and
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aluminum 200 $\mu m$.
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\end{itemize}
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\begin{thebibliography}{9}
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%\bibitem{Kuno:1999jp}
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%Y.~Kuno and Y.~Okada,
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%``Muon decay and physics beyond the standard model,''
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%{\it Rev.\ Mod.\ Phys.\ }{\bf 73}, 151 (2001)
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%\bibitem{masi06} L.~Calibbi, A.~Faccia, A.~Masierro, and S.K. Vempati, Phys.
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%Rev. {\bf D74} 116002 (2006).
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%
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%\bibitem{mu2e08} R.M.~Carry {\it et al.} (Mu2e collaboration), ``Proposal to
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%Search for \muec with a Single Event Sensitivity Below $10^{-16}$, FNAL
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%proposal, 2008.
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%
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\bibitem{come07} Y.~Kuno {\it et al.} (COMET collaboration), ``A Experimental
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Search for Lepton Flavor Violating \muec Conversion at Sensitivity of
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$10^{-16}$ with A Slow-Extracted Bunched Proton Beam'', J-PARC Proposal, 2007
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and J-PARC Conceptual Design Report, 2009.
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\bibitem{sindrumii} W.~Bertl {\it et al.} (SINDRUM-II collaboration), ``A
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search for $\mu - e$ conversion in muonic gold'', The European Physical
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Journal C 47 (2006).
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337-346.\\
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%
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\bibitem{phaseI12} Y.~Kuno {\it et al.} (COMET collaboration), ``Letter of
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Intent of Phase--I for the COMET Experiment at J-PARC'', March
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2012.
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%
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\bibitem{sobo68} S.E. Sobotka and E.L. Willis, Phys. Rev. Lett. {\bf 20}
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596-598, (1968).
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%
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%\bibitem{bala67} V. Balashov and R. Eramzhyan. Atomic Energy Reviews 5, 1967.
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%
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\bibitem{hung34} E. Hungerford, ``Comment on Proton Emission after Muon
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Capture'', MECO note 34.
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\bibitem{measday} D.F. Measday, {\it Phys. Rep. }{\bf 354} (2001)
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\end{thebibliography}
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\end{document}
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