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[12 @@ -2537,7 +2546,7 @@ Overfull \vbox (19.18185pt too high) has occurred while \output is active [] -LaTeX Info: Redefining \HepProcess on input line 517. +LaTeX Info: Redefining \HepProcess on input line 556. [13 @@ -2546,7 +2555,7 @@ Overfull \vbox (19.18185pt too high) has occurred while \output is active [] -LaTeX Info: Redefining \HepProcess on input line 517. +LaTeX Info: Redefining \HepProcess on input line 556. [14 @@ -2555,20 +2564,29 @@ Overfull \vbox (19.18185pt too high) has occurred while \output is active [] -LaTeX Info: Redefining \HepProcess on input line 517. +LaTeX Info: Redefining \HepProcess on input line 556. [15 ] +File: images/BG_lower.png Graphic file (type QTm) + +Overfull \vbox (19.18185pt too high) has occurred while \output is active [] + +LaTeX Info: Redefining \HepProcess on input line 556. + +[16 + +] File: images/C9C10-Fit35-Plot.jpeg Graphic file (type QTm) File: images/BG_lower.png Graphic file (type QTm) Overfull \vbox (19.18185pt too high) has occurred while \output is active [] -LaTeX Info: Redefining \HepProcess on input line 517. +LaTeX Info: Redefining \HepProcess on input line 556. -[16 +[17 ] File: images/straub.png Graphic file (type QTm) @@ -2577,26 +2595,26 @@ Overfull \vbox (19.18185pt too high) has occurred while \output is active [] -LaTeX Info: Redefining \HepProcess on input line 544. +LaTeX Info: Redefining \HepProcess on input line 583. -[17 +[18 ] LaTeX Font Info: External font `plex10' loaded for size -(Font) <24.88> on input line 564. +(Font) <24.88> on input line 603. 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stack positions out of 5000i,500n,10000p,200000b,80000s -Output written on mchrzasz.pdf (23 pages). +Output written on mchrzasz.pdf (26 pages). diff --git a/Kstarmumu_Run2/P5prim_QuaVadis/mchrzasz.nav b/Kstarmumu_Run2/P5prim_QuaVadis/mchrzasz.nav index ff6b0a9..01a2755 100644 --- a/Kstarmumu_Run2/P5prim_QuaVadis/mchrzasz.nav +++ b/Kstarmumu_Run2/P5prim_QuaVadis/mchrzasz.nav @@ -10,10 +10,10 @@ \headcommand {\beamer@framepages {10}{10}} \headcommand {\slideentry {0}{0}{5}{11/11}{}{0}} \headcommand {\beamer@framepages {11}{11}} -\headcommand {\slideentry {0}{0}{6}{12/16}{}{0}} -\headcommand {\beamer@framepages {12}{16}} -\headcommand {\slideentry {0}{0}{7}{17/17}{}{0}} -\headcommand {\beamer@framepages {17}{17}} +\headcommand {\slideentry {0}{0}{6}{12/12}{}{0}} +\headcommand {\beamer@framepages {12}{12}} +\headcommand {\slideentry {0}{0}{7}{13/17}{}{0}} +\headcommand {\beamer@framepages {13}{17}} \headcommand {\slideentry {0}{0}{8}{18/18}{}{0}} \headcommand {\beamer@framepages {18}{18}} \headcommand {\slideentry {0}{0}{9}{19/19}{}{0}} @@ -26,8 +26,14 @@ \headcommand {\beamer@framepages {22}{22}} \headcommand {\slideentry {0}{0}{13}{23/23}{}{0}} \headcommand {\beamer@framepages {23}{23}} -\headcommand {\beamer@partpages {1}{23}} -\headcommand {\beamer@subsectionpages {1}{23}} -\headcommand {\beamer@sectionpages {1}{23}} -\headcommand {\beamer@documentpages {23}} -\headcommand {\def \inserttotalframenumber {12}} +\headcommand {\slideentry {0}{0}{14}{24/24}{}{0}} +\headcommand {\beamer@framepages {24}{24}} +\headcommand {\slideentry {0}{0}{15}{25/25}{}{0}} +\headcommand {\beamer@framepages {25}{25}} +\headcommand {\slideentry {0}{0}{16}{26/26}{}{0}} +\headcommand {\beamer@framepages {26}{26}} +\headcommand {\beamer@partpages {1}{26}} +\headcommand {\beamer@subsectionpages {1}{26}} +\headcommand {\beamer@sectionpages {1}{26}} +\headcommand {\beamer@documentpages {26}} +\headcommand {\def \inserttotalframenumber {15}} diff --git a/Kstarmumu_Run2/P5prim_QuaVadis/mchrzasz.pdf b/Kstarmumu_Run2/P5prim_QuaVadis/mchrzasz.pdf index 6c0a973..330afd3 100644 --- a/Kstarmumu_Run2/P5prim_QuaVadis/mchrzasz.pdf +++ b/Kstarmumu_Run2/P5prim_QuaVadis/mchrzasz.pdf Binary files differ diff --git a/Kstarmumu_Run2/P5prim_QuaVadis/mchrzasz.synctex.gz b/Kstarmumu_Run2/P5prim_QuaVadis/mchrzasz.synctex.gz index 194f227..fb3db5b 100644 --- a/Kstarmumu_Run2/P5prim_QuaVadis/mchrzasz.synctex.gz +++ b/Kstarmumu_Run2/P5prim_QuaVadis/mchrzasz.synctex.gz Binary files differ diff --git a/Kstarmumu_Run2/P5prim_QuaVadis/mchrzasz.tex b/Kstarmumu_Run2/P5prim_QuaVadis/mchrzasz.tex index a5084b2..30b0e82 100644 --- a/Kstarmumu_Run2/P5prim_QuaVadis/mchrzasz.tex +++ b/Kstarmumu_Run2/P5prim_QuaVadis/mchrzasz.tex @@ -282,15 +282,15 @@ \onslide<1,2,3>{ \ARROW Several theory authors proposed to measure a ''clean'' observable: \begin{align*} -\P5prime= \frac{S_5}{F_L(1-F_L)} +\P5prime= \frac{S_5}{\sqrt{F_L(1-F_L)}} \end{align*} -\ARROW At leading order of $\alpha_s$ and $m_b$ expansion the form factor cancel \href{https://arxiv.org/abs/1207.2753}{arxiv::1207.2753} +\ARROW At leading order of $\alpha_s$ and $m_b$ expansion the form factors cancel \href{https://arxiv.org/abs/1207.2753}{arxiv::1207.2753} } \onslide<2,3>{ -\ARROW LHCb: \href{https://arxiv.org/pdf/1308.1707.pdf}{arXiv::1308.1707} +\ARROW LHCb: \href{https://arxiv.org/pdf/1308.1707.pdf}{arXiv::1308.1707} ($1~\rm fb^{-1}$) \includegraphics[width=0.95\textwidth]{images/P5p1.png} } @@ -322,7 +322,7 @@ \only<2,3,4,5>{{\color{gray}{\ARROW 2013 LHCb: \href{https://arxiv.org/pdf/1308.1707.pdf}{arXiv::1308.1707}}}\\} \only<2,3,4,5>{\ARROW 2015 LHCb: \href{https://arxiv.org/abs/1512.04442}{arXiv::1512.0444}\\} \only<4,5>{{\color{red}{\ARROW 2016 Belle: \href{https://arxiv.org/abs/1604.04042}{arXiv::1604.04042}}}\\} -\only<5>{\ARROW 2017: {\color{blue}{\href{https://atlas.web.cern.ch/Atlas/GROUPS/PHYSICS/CONFNOTES/ATLAS-CONF-2017-023/}{ATLAS-CONF-2017-023}}} and {\color{OliveGreen}{\href{http://cds.cern.ch/record/2256738?ln=en}{CMS-PAS-BPH-15-008}}}} +\only<5>{\ARROW 2017: {\color{blue}{\href{https://atlas.web.cern.ch/Atlas/GROUPS/PHYSICS/CONFNOTES/ATLAS-CONF-2017-023/}{ATLAS-CONF-2017-023}}} $(20.5~\rm fb^{-1})$ and {\color{OliveGreen}{\href{http://cds.cern.ch/record/2256738?ln=en}{CMS-PAS-BPH-15-008}}} $(20.8~\rm fb^{-1})$} @@ -375,14 +375,14 @@ \ARROW The results are based on Run1 data.\\ \ARROW The measurement of $\P5prime$ is possible knowing the $\PB$ flavour.\\ -\ARROW In LHCb we have RICH, but ATLAS and CMS don't, so the flavour is assigned by checking two possible mass hypothesis for $\PKstar$ and choosing the one closer to the SM value ($13\%$ for CMS and $11\%$ for CMS).\\ +\ARROW In LHCb we have the RICH, but ATLAS and CMS don't, so the flavour is assigned by checking two possible mass hypothesis for $\PKstar$ and choosing the one closer to the SM value ($13\%$ for CMS and $11\%$ for ATLAS).\\ \ARROW The analysis follows our LHCb results from $1~\rm fb^{-1}$: \begin{itemize} \item {\color{red}{Not enough events to perform the full angular fit.}} \item {\color{OliveGreen}{Fold the angles to reduce the number of observables}} \item {\color{red}{In this procedure you lose correlations between the observables}} \end{itemize} -\ARROW The acceptance corrections both in CMS and ATLAS paramterized as $\epsilon(\cos \theta_l, \cos \theta_k, \phi, m)$ in each of the $q^2$ bin.\\ +\ARROW The acceptance corrections both in CMS and ATLAS parametrized as $\epsilon(\cos \theta_l, \cos \theta_k, \phi, m)$ in each of the $q^2$ bin.\\ %\ARROWR ATLAS uses the normal polynomial, while CMS uses KDE and histogram binning. @@ -414,7 +414,7 @@ \begin{small} \ARROW Angular acceptance parametrized by KDE and sampled histograms.\\ \ARROW Determination of only $P_1$ and $P^{\prime}_5$.\\ -\ARROW Swave fraction inferred from other analysis.\\ +\ARROW Swave fraction inferred from previous measurement.\\ \ARROW Main systematics: Control channel differences.\\ \ARROW $\PB \to \PKstar \PJpsi$ used for systematics. @@ -429,10 +429,49 @@ \end{frame} +\begin{frame}\frametitle{Global analysis} +\ARROW Two main players on the market: +\begin{columns} +\column{0.5\textwidth} +\ARROWR J. Matias, et. al.\\ +\column{0.5\textwidth} +\ARROWR D. Straub, et. al.\\ + + +\end{columns} +{~}\\ +\begin{columns} +\column{0.5\textwidth} +\ARROW Measurements taken into the analysis: +\begin{itemize} +\item Angular and Br of $\PB \to \PKstar \mu \mu$ +\item Angular and Br of $\PBs \to \Pphi \mu \mu$ +\item Angular and Br of $\PB \to \PK \mu \mu$ +\item Br $\PB \to X_s \mu \mu$ and $\Pbeauty \to \Pstrange \gamma$ +\item $\PBs \to \mu \mu$ +\end{itemize} + + +\column{0.5\textwidth} +\ARROW Measurements taken into the analysis: +\begin{itemize} +\item Angular and Br of $\PB \to \PKstar \mu \mu$ +\item Angular and Br of $\PBs \to \Pphi \mu \mu$ +\item Angular and Br of $\PB \to \PK \mu \mu$ +\item Br $\PB \to X_s \mu \mu$ +\end{itemize} + + +\end{columns} + +\ARROW There are also subtle difference in the theory treatment of form factors. + + +\end{frame} @@ -535,7 +574,7 @@ \end{center} -\ARROW Both groups came to the similar conclusion! +\ARROW Both groups came to a similar conclusion! } @@ -567,13 +606,13 @@ -\begin{frame}\frametitle{Comments about the CMS result 1/3} +\begin{frame}\frametitle{Comments about the CMS result 1/4} \begin{columns} \column{0.4\textwidth} \begin{small} -\ARROW Both ATLAS and CMS use our folding technique that was used in $1~\rm fb^{-1}$ analysis. %CMS does not cite us for the method...\\ +\ARROW Both ATLAS and CMS use our folding technique that was used in the $1~\rm fb^{-1}$ analysis. %CMS does not cite us for the method...\\ \ARROW CMS when performing the angular fit fixes the $F_L$, $F_S$ and $A_s$ from the previous analysis on the same data!\\ -\ARROWR They claim that they check with TOYMC it is correct. However some doubts remain.\\ +\ARROWR They claim that they check with TOYMC that it is correct. However some doubts remain.\\ \ARROWR Feldman-Cousin procedure can underestimate the errors in this case.\\ \ARROW More details on toy validation and or bootstrapping the data would be nice! \end{small} @@ -591,12 +630,12 @@ -\begin{frame}\frametitle{Comments about the CMS result 2/3} +\begin{frame}\frametitle{Comments about the CMS result 2/4} \begin{columns} \column{0.4\textwidth} \begin{small} \ARROW There seems to be a structure in the $\cos \theta_l$ distribution.\\ -\ARROWR A.Bevan suggested this might be due to existence of a $\PB \to \PD(\PK \pi \pi) \pi$\\ +\ARROWR A.Bevan suggested this might be due to a $\PB \to \PD(\PK \pi \pi) \pi$\\ \ARROW Can be easily checked with MC. \end{small} @@ -615,16 +654,16 @@ -\begin{frame}\frametitle{Comments about the CMS result 3/3} +\begin{frame}\frametitle{Comments about the CMS result 3/4} \begin{columns} \column{0.4\textwidth} \begin{small} \ARROW In the decay of $\PB \to \PKstar \PJpsi$ they fail to reproduce the value of $F_L$.\\ \ARROW They assign the difference as a systematic uncertainty.\\ -\ARROWR There is no guaranty that this has no $q^2$ dependence.\\ -\ARROW They tag the $\PKstar$ via which of the configurations: $\PK^+ \pi^-$, $\PK^- \pi^+$ is closer to nominal $\PKstar$ mass.\\ -\ARROW They model the miss-tag fractions from MC.\\ -\ARROWR The mistag is modelled by MC. Systematic assign from $\PB \to \PKstar \PJpsi$ (no $q^2$ dependence assumed). +\ARROWR There is no guarantee that this has no $q^2$ dependence.\\ +\ARROW They tag the $\PKstar$ via which of the configurations: $\PK^+ \pi^-$, $\PK^- \pi^+$ is closer to the nominal $\PKstar$ mass.\\ +\ARROW They model the mis-tag fractions from MC.\\ +\ARROWR The mis-tag is modelled by MC. Systematic assign from $\PB \to \PKstar \PJpsi$ (no $q^2$ dependence assumed). \end{small} \column{0.6\textwidth} \includegraphics[angle=-90,width=0.95\textwidth]{images/jspi.pdf} @@ -638,15 +677,65 @@ +\begin{frame}\frametitle{Comments about the CMS result 4/4} +\begin{columns} +\column{0.4\textwidth} +\begin{small} +\ARROW CMS uses a long range mass window in the $m_{\PK \pi \mu \mu}$ fits.\\ +\ARROW In LHCb we saw non negligible amount of PARTRECO events.\\ +\ARROW In their fits they don't account for it. + + + +\end{small} +\column{0.6\textwidth} +\includegraphics[width=0.95\textwidth]{images/CMS.png}\\ +\includegraphics[width=0.95\textwidth]{images/LHCb.png} + + +\end{columns} + + + +\end{frame} + + + + + + + + +\begin{frame}\frametitle{Comments about the ATLAS result} +\begin{columns} +\column{0.4\textwidth} +\begin{small} +\ARROW ATLAS has much worse mass resolution compared to CMS and LHCb.\\ +\ARROW They cut tight on the $m_{\PK \pi\mu\mu}$ as we did.\\ +\ARROW How ever it is not obvious that they are not affected because of the resolution. +\end{small} + + +\column{0.6\textwidth} +\includegraphics[width=0.95\textwidth]{images/ATLAS.png}\\ +\includegraphics[width=0.95\textwidth]{images/LHCb.png} + + +\end{columns} + + + +\end{frame} + + \begin{frame}\frametitle{Conclusion} \ARROW The anomaly is alive and well!\\ -\ARROW New results overall increase the significance.\\ +\ARROW Inclusion of new results increases the significance.\\ \ARROW Tension with SM seen in $\P5prime$ by Atlas, Belle and LHCb. CMS result in good agreement with SM, but consistent with our results.\\ \ARROW Some discussion on aspects of the CMS analysis ongoing.\\ -\ARROW Run2 data will shade definite light if the anomaly is there or not (of course the nature of the anomaly is different question). - +\ARROW Run2 data will confirm or disprove the anomaly (of course the nature of the anomaly is a different question). \end{frame}