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@@ -289,6 +289,7 @@ carried out.
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% subsection plastic_scintillators (end)
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%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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\section{Front-end electronics and data acquisition system}
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The front-end electronics of the AlCap experiment was simple since we employed
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a trigger-less read out system with waveform digitisers and flash ADCs
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@@ -413,6 +414,254 @@ automatically starts a new run with the same parameters after about 6 seconds.
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The short period of each run also allows the detection, and helps to reduce the
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influence of effects such as electronics drifting, temperature fluctuation.
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%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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\section{Detector calibration}
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\label{sec:detector_calibration}
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The calibration was done mainly for the silicon and germanium detectors
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because they would provide energy information. The plastic scintillators were
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only checked by oscilloscopes to make sure that the minimum ionisation
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particles (MIPs) could be observed. The upstream plastic scintillation
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counters and wire chamber, as mentioned, were well-tuned by the MuSun group.
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\subsection{Silicon detector}
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\label{sub:silicon_detector}
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The energy calibration for the silicon detectors were done routinely during the
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run, by:
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\begin{itemize}
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\item a \SI{79.5}{\becquerel} $^{241}\textrm{Am}$ alpha source. The most
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prominent alpha particles have energies of \SI{5.484}{\si{\MeV}} (85.2\%)
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and \SI{5.442}{\si{\MeV}} (12.5\%). The alpha particles from the source
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would lose about \SI{66}{\kilo\eV} in the \SI{0.5}{\um}-thick dead layer,
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and the peak would appear at \SI{5418}{\kilo\eV} (\cref{fig:toyMC_alpha});
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\item and a tail pulse generator, A tail pulse with amplitude of
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\SI{66}{\milli\volt}~was used to simulate the response of the silicon
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detectors' preamplifiers to a particle with \SI{1}{\MeV} energy deposition;
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\item During data taking period, electrons in the beam were were also used
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for energy calibration of thick silicon detectors where energy deposition
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is large enough. The muons at different momenta provided another mean of
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calibration in the beam tuning period.
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\end{itemize}
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\begin{figure}[htb]
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\centering
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\includegraphics[width=0.6\textwidth]{figs/toyMC_alpha}
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\caption{Energy loss of the alpha particles after a dead layer of
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\SI{0.5}{\um}.}
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\label{fig:toyMC_alpha}
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\end{figure}
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The calibration coefficients for the silicon channels are listed in
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\cref{tab:cal_coeff}.
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\begin{table}
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\begin{center}
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\pgfplotstabletypeset[
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% separator
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col sep=comma,
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% columns displayed
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display columns/0/.style={column name = \textbf{Detector}, string type,
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column type=l},
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display columns/1/.style={column name = \textbf{Slope}, column type=c,
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dec sep align},
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display columns/2/.style={column name = \textbf{Offset}, column type=r,
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dec sep align},
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% format the line breaks
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every head row/.style={
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before row={\toprule},
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after row={\midrule},
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columns/Detector/.style={column type=c},
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columns/Slope/.style={column type=c},
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columns/Offset/.style={column type=c}
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},
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every last row/.style={after row=\bottomrule},
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]{raw/si_cal_effs.csv}
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\caption{Calibration coefficients of the silicon detector channels}
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\label{tab:cal_coeff}
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\end{center}
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\end{table}
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% subsection silicon_detector (end)
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%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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\subsection{Germanium detector}
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\label{sub:germanium_detector}
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The germanium detector was calibrated using a $^{152}\textrm{Eu}$
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source
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\footnote{Energies and intensities of gamma rays are taken from the
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X-ray and Gamma-ray Decay Data Standards for Detector Calibration and Other
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Applications, which is published by IAEA at \\
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\url{https://www-nds.iaea.org/xgamma_standards/}},
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the recorded pulse height spectrum is shown in \cref{fig:ge_eu152_spec}. The
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source was placed at the target position so that the absolute efficiencies can
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be calculated. The peak centroids and areas were obtained by fitting a Gaussian
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peak on top of a first-order polynomial background. The only exception is the
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\SI{1085.84}{\keV} line because of the interference of \SI{1089.74}{\keV},
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the two were fitted with two Gaussian peaks on top of a first-order
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polynomial background.
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The relation between pulse height in ADC value and energy is found to be:
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\begin{equation}
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\textrm{ E [keV]} = 0.1219 \times \textrm{ADC} + 1.1621
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\end{equation}
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The energy resolution (full width at half maximum - FWHM) was better than
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2.6~\si{\keV}\ for all the $^{152}\textrm{Eu}$ peaks. It was
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a little worse at 3.1~\si{\keV}~for the annihilation photons at
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511.0~\si{\keV}.
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\begin{figure}[htb]
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\centering
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\includegraphics[width=0.70\textwidth]{figs/ge_eu152_spec}
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\caption{Energy spectrum of the $\rm^{152}\textrm{Eu}$ calibration source
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recorded by the germanium detector. The most prominent peaks of
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$^{152}\textrm{Eu}$ along with their energies are
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annotated in red; the 1460.82 \si{\keV}~line is background from
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$^{40}\textrm{K}$; and the annihilation 511.0~\si{\keV}~photons
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come both from the source and the surrounding environment.}
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\label{fig:ge_eu152_spec}
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\end{figure}
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\begin{figure}[htb]
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\centering
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\includegraphics[width=0.89\textwidth]{figs/ge_ecal_fwhm}
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\caption{Germanium energy calibration and resolution.}
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\label{fig:ge_fwhm}
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\end{figure}
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The absolute efficiencies of the referenced points, and calculated
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efficiencies at the X-ray of interest are presented in
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\cref{tab:xray_eff}.
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%The absolute efficiencies for the $(2p-1s)$ lines of aluminium
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%(\SI{346.828}{\keV}) and silicon (\SI{400.177}{\keV})
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%are presented in \cref{tab:xray_eff}.
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In the process of efficiency calibration,
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corrections for true coincidence summing and self-absorption were not applied.
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The true coincidence summing probability is estimated to be very
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small, about \num{5.4d-6}, thanks to the far geometry of the calibration. The
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absorption in the source cover made of \SI{22}{\mg\per\cm^2}
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polyethylene is less than \num{4d-4} for a \SI{100}{\keV} photon.
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A Monte Carlo (MC) study on the acceptance of the germanium detector with two
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purposes:
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\begin{enumerate}
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\item compare between measured and MC efficiencies: a point source made of
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$^152$Eu is placed at the target position
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\item estimate the uncertainty due to finite-size geometry: the source is
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made of silicon with the same dimensions as those of the thick silicon
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detector, namely \SI[product-units=power]{1.5 x 50 x 50}{\mm}; then the
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primary vertex of $^152$Eu is generated inside the source.
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\end{enumerate}
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\begin{table}[htb]
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\begin{center}
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\pgfplotstabletypeset[
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% separator
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col sep=comma,
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% columns displayed
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% column type={S} means leave formatting to siunitx
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display columns/0/.style={column name = \textbf{Photons (\si{\keV})},
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string type,
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column type={S[table-format=4.3, table-alignment=center]}},
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display columns/1/.style={column name = \textbf{Efficiency},
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string type,
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column type={S[parse-numbers = true,
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round-precision=3,
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round-mode=figures,
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fixed-exponent=-4,
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scientific-notation=fixed,
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table-format=1.2e-1,
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%table-omit-exponent,
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]}},
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display columns/2/.style={column name = \textbf{Uncertainty},
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string type,
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column type={S[parse-numbers = true,
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round-precision=3,
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round-mode=figures,
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fixed-exponent=-5,
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scientific-notation=fixed,
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table-format=1.3e-1,
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%table-omit-exponent,
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]}},
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% format the line breaks
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every head row/.style={
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before row={\toprule},
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after row={
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%\textbf{\si{\keV}} & \textbf{\num{E-4}} & \textbf{\num{E-4}}\\
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\midrule},
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columns/0/.style={column type=r},
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columns/1/.style={column type=c},
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columns/2/.style={column type=c}
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},
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every last row/.style={after row=\bottomrule},
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every nth row={8}{before row={\midrule}},
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]{raw/ge_eff.csv}
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\end{center}
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\caption{Absolute efficiencies of the germanium detector in case of
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a point-like source placed at the centre of the target (upper half), and
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the calculated efficiencies for the X-rays of interest (lower half).}
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\label{tab:xray_eff}
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\end{table}
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\begin{figure}[htb]
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\centering
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\includegraphics[width=0.40\textwidth]{figs/ge_eff_cal}
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\includegraphics[width=0.40\textwidth]{figs/ge_eff_mc_finitesize_vs_pointlike_root}
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\caption{Absolute efficiency of the germanium detector, the fit was done with
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7 energy points from 244~keV, the shaded area is
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95\% confidence interval of the fit.}
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%because it is known that the linearity between
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%$ln(\textrm{E})$ and $ln(\textrm{eff})$ holds better.
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\label{fig:ge_eff_cal}
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\end{figure}
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% subsection germanium_detector (end)
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%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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%\subsection{Beam tuning and muon momentum scanning}
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%\label{sub:muon_momentum_scanning}
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%Before taking any data, we carried out the muon momentum scanning to understand
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%the muon beam, as well as calibrate the detector system. The nominal muon
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%momentum used in the Run 2013 had been tuned to 28~MeV\cc\ before the run. By
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%changing simultaneously the strength of the key magnet elements in the $\pi$E1
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%beam line with the same factor, the muon beam momentum would be scaled with the
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%same factor.
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%The first study was on the range of muons in an active silicon target. The SiL2
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%detector was placed perpendicular to the nominal beam path, after an oval
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%collimator. The beam momentum scaling factor was scanned from 1.10 to 1.60,
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%muon momenta and energies in the measured points are listed in
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%\cref{tab:mu_scales}.
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%\begin{table}[htbp]
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%\begin{center}
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%\begin{tabular}{c c c c}
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%\toprule
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%\textbf{Scaling} & \textbf{Momentum} & \textbf{Kinetic energy}
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%& \textbf{Momentum spread}\\
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%\textbf{factor} & \textbf{(MeV\per\cc)} & \textbf{(MeV)}
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%& \textbf{(MeV\per\cc, 3\% FWHM)}\\
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%\midrule
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%1.03 & 28.84 & 3.87& 0.87\\
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%1.05 & 29.40 & 4.01& 0.88\\
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%1.06 & 29.68 & 4.09& 0.89\\
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%1.07 & 29.96 & 4.17& 0.90\\
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%1.10 & 30.80 & 4.40& 0.92\\
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%1.15 & 32.20 & 4.80& 0.97\\
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%1.20 & 33.60 & 5.21& 1.01\\
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%1.30 & 36.40 & 6.09& 1.09\\
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%1.40 & 39.20 & 7.04& 1.18\\
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%1.43 & 40.04 & 7.33& 1.20\\
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%1.45 & 40.60 & 7.53& 1.22\\
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%1.47 & 41.16 & 7.73& 1.23\\
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%1.50 & 42.00 & 8.04& 1.26\\
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%\bottomrule
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%\end{tabular}
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%\end{center}
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%\caption{Muon beam scaling factors, energies and momenta.}
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%\label{tab:mu_scales}
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%\end{table}
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% subsection muon_momentum_scanning (end)
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%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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% section detector_calibration (end)
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%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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\section{Data sets and statistics}
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\label{sec:data_sets}
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