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- \author{ {\fontspec{Trebuchet MS}Marcin Chrz\k{a}szcz} (Universit\"{a}t Z\"{u}rich)}
- \institute{UZH}
- \title[$\PBzero \to \PKstar \Pmuon \APmuon$ MC requirements]{$\PBzero \to \PKstar \Pmuon \APmuon$ MC requirements}
- \date{25 September 2014}
-
-
- \begin{document}
- \tikzstyle{every picture}+=[remember picture]
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- {
- \setbeamertemplate{sidebar right}{\llap{\includegraphics[width=\paperwidth,height=\paperheight]{bubble2}}}
- \begin{frame}[c]%{\phantom{title page}}
- \begin{center}
- \begin{center}
- \begin{columns}
- \begin{column}{0.75\textwidth}
- \flushright\fontspec{Trebuchet MS}\bfseries \Huge {$\PBzero \to \PKstar \Pmuon \APmuon$\\ MC requirements}
- \end{column}
- \begin{column}{0.02\textwidth}
- {~}
- \end{column}
- \begin{column}{0.23\textwidth}
- % \hspace*{-1.cm}
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- \includegraphics[width=0.6\textwidth]{lhcb-logo}
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- \end{columns}
- \end{center}
- \quad
- \vspace{3em}
- \begin{columns}
- \begin{column}{0.44\textwidth}
- \flushright \vspace{-1.8em} {\fontspec{Trebuchet MS} \Large Marcin Chrząszcz\\\vspace{-0.1em}\small \href{mailto:mchrzasz@cern.ch}{mchrzasz@cern.ch}\\ \Large Thomas Blake \\ Nicola Serra }
-
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- \includegraphics[height=1.3cm]{uzh-transp}
- \end{column}
- \end{columns}
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- \vspace{1em}
- % \footnotesize\textcolor{gray}{With N. Serra, B. Storaci\\Thanks to the theory support from M. Shaposhnikov, D. Gorbunov}\normalsize\\
- \vspace{0.5em}
-
- \textcolor{normal text.fg!50!Comment}{EWP WG meeting, CERN\\November 24, 2016}
- \end{center}
- \end{frame}
- }
-
-
-
-
- \begin{frame}[c]{Plans 1}
- \begin{minipage}{\textwidth}
- \begin{footnotesize}
-
-
- \ARROW MC required for $\PB \to \PKstar \Pmu \Pmu$ 2015+2016 analysis.\\
- \ARROW Numbers are taken from previous round with scaling factor $\frac{4}{3}$ for the cross section increase.
- {~}\\
- \begin{small}
-
- \begin{tabular}{lrrr}\hline
- Decay & Event type & N.o. generated & N.o. stored\\ \hline\hline
- $\PB \to \PKstar \PJpsi$ (physics) & {\tt 11144001} & 2.6M & 0.8M \\
- {\color{JungleGreen}{$\PB \to \PKstar \mu \mu$ (acceptance)}} & {\color{JungleGreen}{{\tt 11114014}}} & {\color{JungleGreen}{160M}} & {\color{JungleGreen}{48M}} \\
- $\PB \to \PKstar \mu \mu$ (physics) & {\tt 11114001} & 1.5M & 0.5M\\
- $\PLambdab \to \PLambda(1530)\mu\mu$ & {\tt 15114000} & 1.5M & 0.5M\\
- $\PLambdab \to p K \mu\mu$ & {\tt 15114011} & 2M & 0.6M\\
- $\PBs \to \phi\mu\mu$ & {\tt 13114002} & 1M & 0.3M\\
- $\PB_u \to \PK \mu\mu$ & {\tt 12113001} & 1M & 0.3M\\\hline
- \hline\end{tabular}
- \end{small}
-
- \ARROW All productions will be filtered to save disk space.\\
- \ARROW The large sample will be used to correct the detector acceptance.\\
- \end{footnotesize}
- \end{minipage}
- \vspace*{2.cm}
- \end{frame}
-
-
- \begin{frame}[c]{Acceptance}
- \begin{minipage}{\textwidth}
-
- \begin{columns}
-
- \column{0.5\textwidth}
- \ARROW The kinematics of the decay $\PB \to \PKstar \Pmu \Pmu$ is described by 3 helicity angles($\cos \theta_k,~\cos \theta_l~\phi$) and the squared invariant mass of two muons ($q^2$).\\
- \ARROW Because of the 4D acceptance correction a lot of events are needed to populate the parameters space.\\
- \ARROW This sample will be enough to keep the related systematics order of magnitude below the expected statistical uncertainty.
-
- \column{0.5\textwidth}
-
- \includegraphics[width=0.99\textwidth]{images/det.png}
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- \end{columns}
- \end{minipage}
- \vspace*{2.cm}
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