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Presentations / Kstmumu / Answers_to_questions_v2 / group_meeting.tex
  1. % This program can be redistributed and/or modified under the terms
  2. % of the GNU Public License, version 3.
  3. %
  4. % Seth Brown, Ph.D.
  5. % sethbrown@drbunsen.org
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  149. % see the macros.tex file for definitions
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  151.  
  152. % title slide definition
  153. \title{Answeres to questions raised by conveners on EW penguin.}
  154. %\subtitle{a bias report}
  155. \author{ Marcin Chrz\k{a}szcz$^{1,2}$ , Nicola Serra$^{1}$ }
  156. \institute[UTH, IFJ]
  157. {
  158. %\begin{tiny}
  159. $ ^1$ University of Zurich , $ ^2$ Institute of Nuclear Physics, Krakow,
  160. %\end{tiny}smallsmall
  161. }
  162.  
  163. \date{ \begin{small} \today \end{small}}
  164.  
  165. %--------------------------------------------------------------------
  166. % Introduction
  167. %--------------------------------------------------------------------
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  169. \begin{document}
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  198. %--------------------------------------------------------------------
  199. % OUTLINE
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  205. %\section[Outline]{}
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  207. %\tableofcontents
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  213. %-------------------------------------------------------------------
  214. % Introduction
  215. %-------------------------------------------------------------------
  216. %
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  222.  
  223. \title{Update on analysis}
  224.  
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  235. \begin{frame}\frametitle{More Robust calculation of efficiency}
  236. \only<1>{
  237. We investigated further the events that have one real $\mu$ as candidate.
  238. \begin{columns}
  239. \column{2in}
  240. \begin{enumerate}
  241. \item We observed $\PJpsi$ peak after vetoing this resonance.
  242. \item Most of the non $\mu$ had TRUEID==0.
  243. \item If we account for truth matching problems we obtain the following efficiency.
  244. \end{enumerate}
  245.  
  246.  
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  248.  
  249. \includegraphics[scale=0.25]{kstmumu/jpsi2.png}
  250.  
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  253. }
  254. \only<2>
  255. {
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  259.  
  260. \begin{center}
  261. \begin{tabular}{ | c | c |}
  262. \hline
  263. \multicolumn{2}{|c| }{Efficiency for 2 real $\mu$ ID as $\mu$} \\
  264. \hline
  265. PID$\mu$>-3 & 95.3\% \\ \hline
  266. PID$\mu$>0 & 97.4\% \\ \hline
  267. PID$\mu$>5\footnote{2011 analysis had similar cut inside BDT} & 99.2\% \\ \hline
  268.  
  269. \end{tabular}
  270. \end{center}
  271.  
  272.  
  273.  
  274. Conclusion: Our bck is purely dimuon!\\
  275. PS. If you think about asking what the remaining $0.8\%$ are.., just don't.
  276.  
  277. }
  278.  
  279. \textref {M.Chrz\k{a}szcz, N.Serra 2013}
  280.  
  281. \end{frame}
  282.  
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  287.  
  288. \begin{frame}\frametitle{More advanced generator cuts? }
  289. \only<1>{
  290.  
  291. We tried two approaches:
  292. \begin{itemize}
  293. \item Require additional track close to dimuon pair.
  294. \end{itemize}
  295.  
  296. }
  297. \only<2>{
  298.  
  299. We tried two approaches:
  300. \begin{itemize}
  301. \item Require additional track close to dimuon pair.
  302. \end{itemize}
  303.  
  304.  
  305. Requring 3 tracks doesn't help at all. $98\%$ of the cases the DOCA between 3 tracks is the dimuon doca(what you would expected). in $80\%$ of cases the minimum DOCA of three tracks is 0(because of semi-leptonic decays).
  306.  
  307.  
  308. }
  309.  
  310.  
  311.  
  312.  
  313. \textref {M.Chrz\k{a}szcz, N.Serra 2013}
  314.  
  315. \end{frame}
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  332. \end{document}