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Presentations / For_Tom / For_Tom / group_meeting.tex
@mchrzasz mchrzasz on 10 Oct 2013 13 KB update before changing laptops
% This program can be redistributed and/or modified under the terms
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% see the macros.tex file for definitions
\include{macros }

% title slide definition
\title{Inflaton line.}
%\subtitle{a bias report}
\author{ Marcin Chrz\k{a}szcz$^{1,2}$ ,  Nicola Serra$^{1}$ }
\institute[UTH, IFJ]
{
 %\begin{tiny}
$ ^1$ University of Zurich , $ ^2$ Institute of Nuclear Physics, Krakow,  
 %\end{tiny}smallsmall
}
  

%\date{ 

%--------------------------------------------------------------------
%                           Introduction
%--------------------------------------------------------------------

\begin{document}




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\column{2.75in}
  \titlepage

  \begin{center}
  \includegraphics[height=1.0cm ]{pic/uzh.jpg}
  % \hspace{0.5cm}
  % \includegraphics[height=1.5cm]{pic/babar.jpg}
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  \vspace{10cm}
\column{2.0in}
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\end{frame}

%--------------------------------------------------------------------
%                          OUTLINE
%--------------------------------------------------------------------




\section[Outline]{}
%\begin{frame}
%\tableofcontents
%\end{frame}







%-------------------------------------------------------------------
%                          Introduction
%-------------------------------------------------------------------
%
% Set the background for the rest of the slides.
% Insert infoline
\setbeamertemplate{background}
 {\includegraphics[width=\paperwidth,height=\paperheight]{slide_bg}}
\setbeamertemplate{footline}[bunsentheme]

\title{Update on analysis}


%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%

\setbeamertemplate{background}
 {\includegraphics[width=\paperwidth,height=\paperheight]{slide_bg}}
\setbeamertemplate{footline}[bunsentheme]
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%2>%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%

\section{Inflaton analysis}
\subsection{Introduction}
\begin{frame}\frametitle{Inflaton analysis}
Motivation:
\begin{small}
\begin{itemize}
\item Probing low energy particle physics.
\end{itemize}
$ \mathcal{L}_{XSM} = \int\sqrt{-g}d^{4}x (\mathcal{L}_{SM} + \mathcal{L}_{X} + \mathcal{L}_{grav})$ \\

\begin{itemize}
\item Coupling to SM via scalar potential.
\item Solves cosmological problems.
\item Long lived particles. Life time $10^{-9}-10^{-10} s$
\item Mass $1-2 GeV$.
\item Reheats the early universe.\footnote{arXiv:0912.0390, arXiv:1303.4395}
\end{itemize}



\end{small}

	\textref {M.Chrz\k{a}szcz, N.Serra 2013}
\end{frame}

%\section{Work done so far}



%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%55
\begin{frame}
\subsection{Simulation}

\frametitle{Work done so far}
{~}
\begin{itemize}
\item We simulated Signal events of$B^0 \to K^{*} X(\mu\mu)$. Using different masses and different life time.
\item Arround $1\%$ of events survive the stripping.
 


\end{itemize}


		\textref {M.Chrz\k{a}szcz, N.Serra 2013}
\end{frame}

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%55
\begin{frame}
\subsection{Changes}

\frametitle{Proposed changes}
{~}

We propose to change:
\only<1>
{
\begin{itemize}
\item $\mu$ : MIPCHI2DV(PRIMARY) $ > 100 \to 90$
\item $\mu$  Add a cut: (ADOCACHI2CUT(25, '')
\item( AMAXDOCA('') $0.1 \to 0.11$
 \end{itemize}
 Downstream:
 \begin{itemize}
\item $\mu$  : MIPCHI2DV(PRIMARY) $ > 150 \to 135$
\item $\mu$  Add a cut: (ADOCACHI2CUT(25, '')
\item AMAXDOCA('') $0.2 \to 0.22$
\end{itemize}
}
\only<2>
{
$K^{*}$
\begin{itemize}
\item "MIPCHI2DV(PRIMARY)> $25 \to 23 $
 \end{itemize}
 $B^{0}$ :
 \begin{itemize}
\item  BPVIPCHI2()< $60 \to 50$.
\end{itemize}

}
		\textref {M.Chrz\k{a}szcz, N.Serra 2013}
\end{frame}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%


\begin{frame}
%\subsection{Results on retention}

\frametitle{Results on retention}
{~}
\begin{itemize}
\item timming: $0.747 \to 0.818$
\item Retention $0.0240 \to 0 .0410$
 
\end{itemize}

No micro dst possible. Very strange topology of the decay plus isolation parameter will be used.


		\textref {M.Chrz\k{a}szcz, N.Serra 2013}
\end{frame}


%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%


\begin{frame}

\frametitle{}

\begin{Huge}
BACKUP
\end{Huge}

		\textref {M.Chrz\k{a}szcz, N.Serra 2013}
\end{frame}


%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%5
\begin{frame}
\frametitle{Flight distance of Inflaton}
{~}


\begin{columns}
\column{2.5in}
Reconstructed
  \includegraphics[scale=0.25]{pic2/FD_XI_reco_down.png}


\column{2.5in}
Truth Matched 
 \includegraphics[scale=0.25]{pic2/FD_XI_true_down.png}


\end{columns}



		\textref {M.Chrz\k{a}szcz, N.Serra 2013}
\end{frame}






\begin{frame}
\frametitle{Flight distance of Inflaton, "normal" $\mu$}
{~}


\begin{columns}
\column{2.5in}
Reconstructed
  \includegraphics[scale=0.4]{pic2/FD_XI_reco.png}


\column{2.5in}
Truth Matched 
 \includegraphics[scale=0.4]{pic2/FD_XI_true.png}


\end{columns}



		\textref {M.Chrz\k{a}szcz, N.Serra 2013}
\end{frame}




\begin{frame}
\frametitle{Life time of Inflaton, "normal" $\mu$}
{~}


\begin{columns}
\column{2.5in}
Reconstructed
  \includegraphics[scale=0.4]{pic2/time_XI_reco.png}


\column{2.5in}
Truth Matched 
 \includegraphics[scale=0.4]{pic2/time_XI_true.png}


\end{columns}



		\textref {M.Chrz\k{a}szcz, N.Serra 2013}
\end{frame}

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%

\begin{frame}
\frametitle{Flight distance of Inflaton, downstream $\mu$}
{~}


\begin{columns}
\column{2.5in}
Reconstructed
  \includegraphics[scale=0.25]{pic2/FD_XI_reco_down.png}


\column{2.5in}
Truth Matched 
 \includegraphics[scale=0.25]{pic2/FD_XI_true_down.png}


\end{columns}



		\textref {M.Chrz\k{a}szcz, N.Serra 2013}
\end{frame}




\begin{frame}
\frametitle{Life time of Inflaton, downstream $\mu$}
{~}


\begin{columns}
\column{2.5in}
Reconstructed
  \includegraphics[scale=0.25]{pic2/time_XI_reco_down.png}


\column{2.5in}
Truth Matched 
 \includegraphics[scale=0.25]{pic2/time_XI_true_down.png}


\end{columns}



		\textref {M.Chrz\k{a}szcz, N.Serra 2013}
\end{frame}




\subsection{Resolution}
\begin{frame}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%5

\frametitle{Mass Resolution }
{~}

\begin{itemize}
\item Fitted separately for $\PB0$ and $\chi$
\item Fitting model: Double Gauss. 
\item Single Gauss didn't work.
\item We will account for MC/DATA difference.
\end{itemize}



		\textref {M.Chrz\k{a}szcz, N.Serra 2013}
\end{frame}


%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%5
\begin{frame}
\frametitle{Mass Resolution }
{~}


\begin{columns}
\column{2.5in}
StdMuons
  \includegraphics[scale=0.25]{pic2/B0_mass.png}
\begin{tiny} $mean_1= 5.288\times 10^{+03} \pm 0.21 MeV$, $mean_2= 5.27\times 10^{+03} \pm  1.56  MeV$\\ 
$\sigma_1=58.8 \pm 2.24 $, $\sigma_2= 15.5\pm  0.23$\\ 
$f= 0.79 \pm  0.01 $
\end{tiny}

\column{2.5in}
Downstream
 \includegraphics[scale=0.25]{pic2/B0_mass_d.png}
\begin{tiny} $mean_1=5.28\times 10^{+03} \pm 4.18 MeV$, $mean_2= 5.28\times 10^{+03} \pm  0.56  MeV$\\ 
$\sigma_1=66.6 \pm 7.56 $, $\sigma_2= 18.7\pm  0.65$\\ 
$f= 0.21 \pm  0.02 $
\end{tiny}
\end{columns}



		\textref {M.Chrz\k{a}szcz, N.Serra 2013}
\end{frame}




\begin{frame}


\frametitle{Mass Resolution }
{~}


\begin{columns}
\column{2.5in}
StdMuons
  \includegraphics[scale=0.25]{pic2/inflaton.png}
\begin{tiny} $mean_1=1.48893\times 10^{+03} \pm 1.1 MeV$, $mean_2= 1.50046\times 10^{+03} \pm  0.09  MeV$\\ 
$\sigma_1=25.7 \pm 0.83 $, $\sigma_2=  7.63\pm  0.01$\\ 
$f= 0.104 \pm  0.007 $

\end{tiny}

\column{2.5in}
Downstream
 \includegraphics[scale=0.25]{pic2/inflaton_d.png} \\
\begin{tiny} $mean_1=1.49880\times 10^{+03} \pm 1.41 MeV$, $mean_2= 1.49743\times 10^{+03} \pm  0.51  MeV$\\ 
$\sigma_1=27.3 \pm 2.57 $, $\sigma_2= 11.34\pm  0.88$\\ 
$f= 0.28 \pm  0.075 $

\end{tiny}
\end{columns}



		\textref {M.Chrz\k{a}szcz, N.Serra 2013}
\end{frame}




\section{Summary}
\begin{frame}\frametitle{Summary on inflaton}
\begin{itemize}
\item Good reconstruction of life time.  \Simley{1}
\item Excellent mass resolution. \Simley{1} 
\item Data from 2011 and 2012 are being processing with our preselection on DIRAC as we speak. \Simley{1} 
\item Poor efficiency: $\varepsilon_{rex} \times \varepsilon_{stripping} = 1\%$ 
 \Simley{-1}
 \item Need to investigate if this is due to reco or stripping.
\end{itemize}







		\textref {M.Chrz\k{a}szcz, N.Serra 2013}
\end{frame}

\end{document}