\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 S} \toprule {\textbf{Absorber}} &{\textbf{Inner wall}} & {\textbf{Total CFRP}}& {\textbf{Proton}} & {\textbf{Momentum}} & {\textbf{Integrated charge}}\\ {\textbf{thickness}} &{\textbf{thickness}} & {\textbf{thickness}}& {\textbf{hit rate}} &{\textbf{spread $\Delta p$}} &{\textbf{300 days}}\\ {(\si{\mm})} & {(\si{\mm})} & {(\si{\mm})} & {(\si{\Hz})} & {(\si{\keV\per\cc)}} &{(mC/cm)}\\ \midrule 1 &0.5&1.5 & 2 & 195 & 25\\ 0.5 &0.5&1.0 & 126 & 167 & 60\\ 0 &0.5&0.5 & 1436 & 133 & 160\\ %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} %\begin{table}[htb] %\begin{center} %\begin{tabular}{S S S S S} %\toprule %{\textbf{Absorber}} &{\textbf{Inner wall}} & {\textbf{Total CFRP}}& %{\textbf{Proton hit rate}} & {\textbf{Proton hit rate}}\\ %{\textbf{thickness}} &{\textbf{thickness}} & {\textbf{thickness}}& %{\textbf{Phase-I TDR}} & {\textbf{New estimation}}\\ %{(\si{\mm})} & {(\si{\mm})} & {(\si{\mm})} & {(\si{\Hz})}& {(\si{\Hz})}\\ %\midrule %1 &0.5&1.5 & 4E+3 & 2 \\ %0.5 &0.5&1.0 & 11E+3& 126 \\ %0 &0.5&0.5 & 30E+3& 1436 \\ %\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} %\begin{table}[htb] %\begin{center} %\begin{tabular}{S S S S S S} %\toprule %{\textbf{Absorber}} &{\textbf{Inner wall}} & {\textbf{Total CFRP}}& {\textbf{Proton}} & {\textbf{Momentum}} & {\textbf{Integrated charge}}\\ %{\textbf{thickness}} &{\textbf{thickness}} & {\textbf{thickness}}& {\textbf{hit rate}} &{\textbf{spread $\Delta p$}} &{\textbf{300 days}}\\ %{(\si{\mm})} & {(\si{\mm})} & {(\si{\mm})} & {(\si{\Hz})} & {(\si{\keV\per\cc)}} &{(mC/cm)}\\ %\midrule %1 &0.5&1.5 & 2 & 195 & 25\\ %0.5 &0.5&1.0 & 126 & 167 & 60\\ %0 &0.5&0.5 & 1436 & 133 & 160\\ %\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}.} %\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.