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\chapter{Discussions on the impact to the COMET Phase-I}
\label{cha:discussions_on_the_impact_to_the_comet_phase_i}
The measured proton emission rate of 3.5\% is about 5 times
smaller than the figure using to make the baseline design of the CDC in COMET
Phase-I. The spectrum shape
peaks around \SI{4}{\MeV} rather than at \SI{2.5}{\MeV}, and decays more
quickly in compared with the silicon spectrum(\cref{fig:sobottka_spec}).
Therefore CDC hit rate due to proton should be smaller than the current
estimation.
The CDC proton hit rate is calculated by a toy MC study. The dimensions of the
geometry shown in \cref{fig:cdc_toy_mc} are from \cref{ssub:CDC_configuration}.
The inner wall of the CDC is \SI{0.5}{\mm} thick CFRP.
A proton absorber made
of CFRP is placed \SI{5}{\cm} far from the inner wall of the CDC. The
absorber's thickness is varied from 0 (no absorber) to \SI{1}{\mm}.
\begin{figure}[htb]
\centering
\includegraphics[width=0.55\textwidth]{figs/cdc_toy_mc}
\caption{Geometry of the toy MC study for hit rate study.}
\label{fig:cdc_toy_mc}
\end{figure}
The protons with the energy spectrum shape as in
\cref{sub:proton_emission_rate} are generated inside the COMET's muon stopping
targets which are 17 200-\si{\um}-thick aluminium discs. The spatial
distribution of protons resembles the stopping distribution of muons inside the
target discs calculated from the full MC simulation of the COMET detectors
(\cref{fig:cdc_toy_mc_init_pos}).
\begin{figure}[htb]
\centering
\includegraphics[width=0.65\textwidth]{figs/cdc_toy_mc_init_pos_xy}
\includegraphics[width=0.60\textwidth]{figs/cdc_toy_mc_init_pos_z}
\caption{Spatial distribution of the generated protons in X, Y (top) and
Z (bottom). Z is the axis of the CDC, X, Y are the horizontal and vertical
axes respectively.}
\label{fig:cdc_toy_mc_init_pos}
\end{figure}
The protons are then tracked in a \SI{1}{\tesla} magnetic field. The protons
reaching the absorber, inner wall and the sensitive volume of the CDC are
recorded (see \cref{fig:cdc_toy_mc_p_spec_500um}).
\begin{figure}[!htb]
\centering
\includegraphics[width=0.75\textwidth]{figs/cdc_toy_mc_p_spec_500um}
\caption{Proton energy spectra at different stages from birth to the
sensitive volume of the CDC. The baseline design of \SI{0.5}{\mm} thick
absorber and \SI{0.5}{\mm} thick inner wall was used to produce this
plot.}
\label{fig:cdc_toy_mc_p_spec_500um}
\end{figure}
A muon stopping rate of \SI{1.3E9}{\Hz} is assumed as in the COMET Phase I's
TDR. The number of proton emitted is then $\num{1.3E9} \times 0.609 \times
0.035 = \SI{2.8E7}{\Hz}$. The hit rates on a single cell in the inner most
layer due to these protons with
different absorber thickness are shown in \cref{tab:proton_cdc_hitrate}.
\begin{table}[htb]
\begin{center}
\begin{tabular}{S S S S S}
\toprule
{\textbf{Absorber}} &{\textbf{Inner wall}} & {\textbf{Total CFRP}}&
{\textbf{Proton}} & {\textbf{Momentum}}\\
{\textbf{thickness}} &{\textbf{thickness}} & {\textbf{thickness}}&
{\textbf{hit rate}} &{\textbf{spread $\Delta p$}}\\
{(\si{\mm})} & {(\si{\mm})} & {(\si{\mm})} & {(\si{\Hz})}
& {(\si{\keV\per\cc)}}\\
\midrule
1 &0.5&1.5 & 2 & 195\\
0.5 &0.5&1.0 & 126 & 167\\
0 &0.5&0.5 & 1436 & 133\\
0 &0.3&0.3 & 8281 & {-}\\
0 &0.1&0.1 & 15011& {-}\\
\bottomrule
\end{tabular}
\end{center}
\caption{CDC proton hit rates at different configuration of proton absorber
and inner wall. The momentum spreads for \SI{0.5}{\mm} thick inner wall are
taken from \cref{tab:comet_absorber_impact}.}
\label{tab:proton_cdc_hitrate}
\end{table}
At the baseline design of \SI{0.5}{\mm}, the hit rate is only \SI{126}{\Hz},
much smaller than the current estimation at \SI{34}{\kHz}. Even without the
absorber, proton hit rate remains low at \SI{1.4}{\kHz}.
%Therefore a proton
%absorber is not needed for the COMET Phase I's CDC.
If the proton absorber is not used, the momentum spread of the signal electron
reduces from \SI{167}{\keV} to \SI{131}{\keV}. In case a lower momentum spread
is desired, it is possible to reduce the thickness of the inner wall. The last
two rows of \cref{tab:proton_cdc_hitrate} show that even with thinner walls at
\SI{0.3}{\mm} and \SI{0.1}{\mm} the hit rate by protons are still at
manageable levels. However, reducing the wall thickness would be governed by
other requirements such as mechanical structure and gas-tightness.
In summary, the toy MC study with the preliminary proton rate and spectrum
shows that a proton absorber is not needed. It confirms the known fact that the
estimation used in COMET Phase-I is conservative, and provides a solid
prediction of the hit rate caused by protons.