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The mechanism required the existence of the $4^{th}$ quark. -\item At that point most of the people were skeptic about that. Fortunately in 1974 the discovery of the $\PJpsi$ meson silenced the skeptics. +\item At that point most of the people were skeptical about that. Fortunately in 1974 the discovery of the $\PJpsi$ meson silenced the skeptics. \end{footnotesize} \end{itemize} \column{0.3\textwidth} @@ -352,7 +353,7 @@ \item Similarly CP violation was discovered in 1960s in the neutral kaons decays. \item $2 \times 2$ Cabbibo matrix could not allow for any CP violation. -\item For the CP violation to be possible one needs atleast $3 \times 3$ unitary matrix \\ $\looparrowright$ Cabibbo-Kobayashi-Maskawa matrix (1973). +\item For the CP violation to be possible one needs at least a $3 \times 3$ unitary matrix \\ $\looparrowright$ Cabibbo-Kobayashi-Maskawa matrix (1973). \item It predicts existence of $\Pbottom$ (1977) and $\Ptop$ (1995) quarks. \end{small} @@ -388,12 +389,10 @@ \begin{small} - - -\item First the weak neutral currents were introduced in 1958 by Buldman. -\item Later on they were naturally build in unification of weak and electromagnetic interactions. +\item Weak neutral currents were first, introduced in 1958 by Buldman. +\item Later on they were naturally incorporated into unification of weak and electromagnetic interactions. \item 't Hooft proved that the GWS models was renormalizable. -\item Everything was there in theory side, only missing piece was the experiment, till 1973. +\item Everything was there on theory side, only missing piece was the experiment, till 1973. \end{small} \end{itemize} @@ -425,7 +424,7 @@ \item CP violation \item Lepton Flavour/Number or Lepton Universality violation. \end{itemize} -\item In general can probe physics beyond GPD reach. +\item In general can probe physics beyond General Purpose Detectors reach. \end{itemize} \column{0.5\textwidth} \includegraphics[width=0.99\textwidth]{{images/TauLFV_UL_2014001_averaged}.png} @@ -566,7 +565,8 @@ \column{0.4\textwidth} \begin{itemize} \item LHCb observed a deviation in $4.3-8.68~\GeV^2$ using $1~\invfb$ of data. -\item It turned out that the discrepancy occurred in an observable that was not constrained. +\item It turned out that the discrepancy occurred in an observable that was not constrained. +\item $q^2$ is the dimuon invariant mass. \end{itemize} \end{columns} @@ -658,7 +658,7 @@ {~} \begin{minipage}{\textwidth} -$\color{JungleGreen}{\Rrightarrow}$ The kinematics of $\PBzero \to \PKstar \Pmuon \APmuon$ decays is described in three angles $\thetal$, $\thetak$, $\phi$ and invariant mass of the dimuon system ($q^2)$. +$\color{JungleGreen}{\Rrightarrow}$ The kinematics of $\PBzero \to \PKstar \Pmuon \APmuon$ decay is described by three angles $\thetal$, $\thetak$, $\phi$ and invariant mass of the dimuon system ($q^2)$. \only<1>{ \begin{columns} @@ -686,7 +686,7 @@ &&\hspace{-2.7cm}+ J_9 \sin^2\theta_K \sin^2\theta_l \sin 2\phi \bigg]\,, } }} -$\color{JungleGreen}{\Rrightarrow}$ This is the most general expression of this kind of decays. +$\color{JungleGreen}{\Rrightarrow}$ This is the most general expression of this kind of decay. } @@ -867,8 +867,8 @@ \begin{large} \begin{itemize} -\item In total we found $2398\pm57$ candidates in the $0.1-19~\GeV^2$ $q^2$ region. -\item $624 \pm 30$ candidates in the theoretically the most interesting $1.1-6.0~\GeV^2$ region. +\item In total we found $2398\pm57$ candidates in the $(0.1,19)~\GeV^2$ $q^2$ region. +\item $624 \pm 30$ candidates in the theoretically the most interesting $(1.1-6.0)~\GeV^2$ region. \end{itemize} \end{large} @@ -946,7 +946,7 @@ %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% -\begin{frame}{Results in $\PB to \PKstar \Pmu \Pmu$} +\begin{frame}{Results in $\PB \to \PKstar \Pmu \Pmu$} \begin{minipage}{\textwidth} \begin{center} \includegraphics[angle=-90,width=0.65\textwidth]{images/Fig17.pdf}\\ @@ -954,7 +954,7 @@ \begin{itemize} \item Tension with $3~\invfb$ gets confirmed! -\item The two bins deviate both in $2.8~\sigma$ form SM prediction. +\item The two bins deviate both in $2.8~\sigma$ from SM prediction. \item Result compatible with previous result. \end{itemize} @@ -1053,7 +1053,7 @@ \begin{minipage}{\textwidth} \begin{itemize} -\item For the bins in which we have $>3~\sigma$ significance the forward-backward for the hadronic and leptonic system. +\item For the bins in which we have $>3~\sigma$ significance the forward backward asymmetry for the hadronic and leptonic system. \end{itemize} \begin{center} \includegraphics[width=0.9\textwidth]{{images/AFB_Lb}.png} @@ -1082,7 +1082,7 @@ \includegraphics[width=0.9\textwidth]{images/uni2.png} \item Challenging analysis due to bremsstrahlung. \item Migration of events modeled by MC. -\item Correct bremsstrahlung. +\item Correct for bremsstrahlung. \item Take double ratio with $\PBplus \to \PJpsi \PKplus$ to cancel systematics. \item In $3\invfb$, LHCb measures $R_K=0.745^{+0.090}_{-0.074}(stat.)^{+0.036}_{-0.036}(syst.)$ \item Consistent with SM at $2.6\sigma$. @@ -1135,7 +1135,7 @@ \includegraphics[width=0.5\textwidth]{images/Kstee.png}\\ \end{center} \begin{itemize} -\item Results in complete agreement with the SM. +\item Results in full agreement with the SM. \item Similar strength on $C_7$ Wilson coefficient as from $\Pbeauty \to \Pstrange \Pphoton$ decays. \end{itemize} @@ -1155,17 +1155,17 @@ \begin{minipage}{\textwidth} \pause \begin{itemize} -\item A preliminary fit prepared by \texttt{S. Descotes-Genon, L. Hofer, J. Matias, J. Virto}, presented at \href{https://indico.in2p3.fr/event/11781/session/0/contribution/15}{\color{blue}{link}} +\item A preliminary fit prepared by \texttt{S. Descotes-Genon, L. Hofer, J. Matias, J. Virto}, presented at \href{http://arxiv.org/abs/1510.04239}{\color{blue}{1510.04239}} \item Took into the fit: \begin{itemize} \item $\mathcal{B} ( \PB \to X_s \Pphoton) = (3.36 \pm 0.23) \times 10^{-4} $, Misiak et. al. 2015. \item $\mathcal{B} ( \PB \to\Pmu \Pmu)$, theory: Bobeth et al 2013, experiment: LHCb+CMS average (2015) \item $\mathcal{B} ( \PB \to X_s \Pmu \Pmu$), Huber et al 2015 \item $\mathcal{B} ( \PB \to \PK \Pmu \Pmu$),Bouchard et al 2013, 2015 -\item $PB_(s) \to \PKstar(\Pphi \Pmu \Pmu$, Horgan et al 2013 +\item $PB_{(s)} \to \PKstar(\Pphi) \Pmu \Pmu$, Horgan et al 2013 \item $\PB \to \PK \Pe \Pe$, $\PB \to \PKstar \Pe \Pe$ and $R_k$. \end{itemize} -\item Over all there is around $4.5~\sigma$ discrepancy wrt. SM. +\item Overall there is around $4.5~\sigma$ discrepancy wrt. SM. \end{itemize} @@ -1180,11 +1180,11 @@ \begin{frame}{Theory implications} {~} \begin{minipage}{\textwidth} -\pause + \begin{itemize} -\item A preliminary fit prepared by \texttt{S. Descotes-Genon, L. Hofer, J. Matias, J. Virto}, presented at \href{https://indico.in2p3.fr/event/11781/session/0/contribution/15}{\color{blue}{link}} +\item A preliminary fit prepared by \texttt{S. Descotes-Genon, L. Hofer, J. Matias, J. Virto}, presented at \href{http://arxiv.org/abs/1510.04239}{\color{blue}{1510.04239}} \item The data can be explained by modifying the $C_9$ Wilson coefficient. -\item Over all there is around $4.5~\sigma$ discrepancy wrt. SM. +\item Overall there is around $4.5~\sigma$ discrepancy wrt. SM. \end{itemize} \includegraphics[width=0.9\textwidth]{images/C9.png} @@ -1264,9 +1264,9 @@ \begin{minipage}{\textwidth} \begin{itemize} \item Clear tensions wrt. SM predictions! -\item Most of them cluster in the same direction. -\item We are not opening the champaign yet! -\item Need still improvement both on theory and experimental side. +\item Measurements cluster in the same direction. +\item We are not opening the champagne yet! +\item Still need improvement both on theory and experimental side. \item Time will tell if this is QCD+fluctuations or new Physics: \end{itemize} \pause