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Presentations / Gambit / Adding_members / mchrzasz.tex
@mchrzasz mchrzasz on 20 Mar 2016 12 KB adding gambit memebers presentation
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\author{ {\fontspec{Trebuchet MS}Marcin Chrz\k{a}szcz} (Universit\"{a}t Z\"{u}rich)}
\institute{UZH}
\title[FlavBit expansions]{FlavBit expansion}
\date{28 September 2015}


\begin{document}
\tikzstyle{every picture}+=[remember picture]

{
\setbeamertemplate{sidebar right}{\llap{\includegraphics[width=\paperwidth,height=\paperheight]{bubble2}}}
\begin{frame}[c]%{\phantom{title page}} 
\begin{center}
\begin{center}
	\begin{columns}
		\begin{column}{0.9\textwidth}
			\flushright\fontspec{Trebuchet MS}\bfseries \Huge {FlavBit expansion}
		\end{column}
		\begin{column}{0.2\textwidth}
		  %\includegraphics[width=\textwidth]{SHiP-2}
		\end{column}
	\end{columns}
\end{center}
	\quad
	\vspace{3em}
\begin{columns}
\begin{column}{0.44\textwidth}
\flushright \vspace{-1.8em} {\fontspec{Trebuchet MS} \Large Marcin ChrzÄ…szcz\\\vspace{-0.1em}\small \href{mailto:mchrzasz@cern.ch}{mchrzasz@cern.ch}}

\end{column}
\begin{column}{0.53\textwidth}
\includegraphics[height=1.3cm]{uzh-transp}
\end{column}
\end{columns}

\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}{Gambit meeting, Gambit virtual meeting\\March 17, 2016}
\end{center}
\end{frame}
}

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\begin{frame}\frametitle{Quo vadis FlavBit?}
\begin{columns}
\column{0.1in}
{~}
\column{3.0in}
\ARROW Where we are:
\begin{itemize}
\item We are much smaller than other flavour fitting groups, e.g. MasterCode (John Ellis + Isidori + Diego Martinez +... + many other postdocs)
\item  Even so we now manage to have more or less the same capabilities (in flavour) but they are rapidly expanding.
\item MasterCode will have soon the \texttt{SuFla} implemented.
\item At present we do not have any target model that the flavour anomalies (see later)
\end{itemize}
\column{2.0in}
\includegraphics[width=0.95\textwidth]{images/quovadis.png}

\end{columns}



\end{frame}



%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\begin{frame}\frametitle{Quo vadis FlavBit?}
\begin{columns}
\column{0.1in}
{~}
\column{4.8in}
\ARROW What can we do?
\begin{itemize}
\item We can stick to what we have and eventually give the ground to them.
\item Or we can do better:

\item Backed and extend \texttt{EOS}!\\ Will give us control of all the harmonic uncertainties.
\item Implement the Kaon physics observables. \\Similar pattern of anomalies has been observed in the kaon sector, but there is no real attempt to link them.
\item Add the SM fits! Gambit is powerful fitting machine that can be used not only for SUSY. \\ We can be competition to HFAG in the LHCb+Belle2 area.
\item Combine measurements of LHCb + BelleII (Gambit could be used by these collaborations) once available. once available) 

\end{itemize}



\end{columns}



\end{frame}


%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\begin{frame}\frametitle{Quo vadis FlavBit?}
\begin{columns}
\column{0.1in}
{~}
\column{4.8in}
\ARROW How to do it?\\
\ARROW Expand:
\begin{itemize}
\item Add at least one experimentalist from BelleII to complement our experimental expertise, this will also allow to promptly implement BelleII and LHCb results and combine them. \\
Paul Jackson has kindly already made a list of potential excellent people form BelleII.
\item Add theorists with different expertise BSM, fits, hadronic uncertainty.
\item We believe that we need a critical mass in order to go to next step and implement most flavour observables.
\item We should start having bi-weekly flavour meeting to work toward this goal.
\end{itemize}

\end{columns}



\end{frame}


%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\begin{frame}\frametitle{List of current anomalies in Flavour sector}
\begin{itemize}
\item $\mathcal{R}(D^{\ast})= \dfrac{Br( \PB \to \PD^{\ast} \tau \nu) }{Br( \PB \to \PD^{\ast} \mu \nu) } $
\item Angular distributions $\PB \to \PKstar \mu \mu$.
\item All branching fractions of $\Pbeauty  \to \Pstrange \ell \ell$ decays.
\item $\varepsilon\prime/ \varepsilon$ in the $\PKlong \to \pi \pi$
\end{itemize}
\ARROW They all cluster in the same direction!

\end{frame}


%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\begin{frame}\frametitle{List of current anomalies in Flavour sector}
\ARROW People are starting to claim already $5~\sigma$ NP discoveries form Flavour:
\begin{center}
\includegraphics[width=0.9\textwidth]{images/NP.png}
\end{center}
\ARROW Thank God(or not...) this approach is not really well received by the community!\\
\ARROW The Flavour physics has one nice advantage: A single deviation will not convince anyone!\\
\ARROW We need a consistent shift of deviations and a bullet prove procedure with fitting them!

\end{frame}


%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\begin{frame}\frametitle{Proposal}
\begin{itemize}
%\item We propose to add at 3 theorists and one Belle2 experimentalist to the Flavour family.
\item Nico+Marcin have been in contact with Buras and Bobeth which are experts in Model building and BSM fits.
\item Jack contacted potential BelleII candidates.
\item Nazila contacted Aoife Bharucha.
\end{itemize}
\end{frame}

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\begin{frame}\frametitle{Quo vadis FlavBit?}
\ARROW Comments/Thoughts?\\

{~}\\{~}\\
\begin{center}
\includegraphics[width=0.95\textwidth]{images/quovadis2.png}
\end{center}

\end{frame}








\end{document}