diff --git a/Beach2022/mchrzasz.log b/Beach2022/mchrzasz.log
index b7363bf..222e7b7 100644
--- a/Beach2022/mchrzasz.log
+++ b/Beach2022/mchrzasz.log
@@ -1,4 +1,4 @@
-This is XeTeX, Version 3.14159265-2.6-0.999991 (TeX Live 2019/Debian) (preloaded format=xelatex 2022.1.5) 5 JUN 2022 15:46
+This is XeTeX, Version 3.14159265-2.6-0.999991 (TeX Live 2019/Debian) (preloaded format=xelatex 2022.1.5) 6 JUN 2022 08:44
entering extended mode
restricted \write18 enabled.
%&-line parsing enabled.
diff --git a/Beach2022/mchrzasz.pdf b/Beach2022/mchrzasz.pdf
index d3b415f..10a08df 100644
--- a/Beach2022/mchrzasz.pdf
+++ b/Beach2022/mchrzasz.pdf
Binary files differ
diff --git a/Beach2022/mchrzasz.synctex.gz b/Beach2022/mchrzasz.synctex.gz
deleted file mode 100644
index ac9bfbd..0000000
--- a/Beach2022/mchrzasz.synctex.gz
+++ /dev/null
Binary files differ
diff --git a/UK_VD/26.12.2022/Makefile b/UK_VD/26.12.2022/Makefile
new file mode 100644
index 0000000..e4cf8e8
--- /dev/null
+++ b/UK_VD/26.12.2022/Makefile
@@ -0,0 +1,9 @@
+all: mchrzasz.pdf
+
+mchrzasz.pdf: mchrzasz.tex
+ xelatex mchrzasz.tex
+# bibtex mchrzasz
+ xelatex mchrzasz.tex
+# xelatex mchrzasz.tex
+clean:
+ rm *.aux *.bbl *.blg *.log *.out *.pdf *.sh *.xml *.snm *.toc *.nav
diff --git a/UK_VD/26.12.2022/beamercolorthemeFlip.sty b/UK_VD/26.12.2022/beamercolorthemeFlip.sty
new file mode 100755
index 0000000..d6b9c50
--- /dev/null
+++ b/UK_VD/26.12.2022/beamercolorthemeFlip.sty
@@ -0,0 +1,179 @@
+% Color style file for the BEAMER FLIP THEME
+% Copyright 2012 by Flip Tanedo
+% This file may be distributed and/or modified
+% 1. under the LaTeX Project Public License and/or
+% 2. under the GNU Public License.
+
+
+
+\mode
+\newif\ifbeamer@Flip@dark
+\beamer@Flip@darkfalse
+\DeclareOptionBeamer{dark}{\beamer@Flip@darktrue}
+\ProcessOptionsBeamer
+
+
+% These are a few colors that I like.
+
+\definecolor{crimsonred}{RGB}{153,0,0} % Neurtal red, good for dark or light bg
+\definecolor{darkcharcoal}{RGB}{25,25,25} % Darker gray
+\definecolor{charcoal}{RGB}{51,51,51} % Darker gray
+\definecolor{ash}{RGB}{100,100,100} % medium gray
+\definecolor{paleblue}{RGB}{0,102,102} % More of an `ocean' color
+\definecolor{turtlegreen}{RGB}{51,153,0} % A more neutral green
+\definecolor{paleale}{RGB}{204,204,102} % Only for dark BG
+\definecolor{lager}{RGB}{140,110,10} % Use instead of pale ale for white BG
+\definecolor{regal}{RGB}{90,0,120} % A more neutral purple
+\definecolor{jeans}{RGB}{20,30,150} % A more neutral blue
+
+
+% Define some "invariant colors" so that a color that doen't work with a
+% light/dark background will automatically be substituted with one that does.
+% These will be rewritten in beamercolorthemeFlipDark
+
+\ifbeamer@Flip@dark
+ \definecolor{FlipSand}{RGB}{204,204,102} % paleale, Only for dark BG
+ \definecolor{FlipGreen}{RGB}{0,255,0} % Neon-like green, only for dark BG
+\else
+ \definecolor{FlipSand}{RGB}{140,110,10} % lager, Only for light BG
+ \definecolor{FlipGreen}{RGB}{51,153,0} % turtlegreen, works for both
+\fi
+
+%% Future revision: It would be nice to define these in terms of the palette.
+
+
+\ifbeamer@Flip@dark
+ \setbeamercolor{normal text}{fg=white, bg=black}
+ \setbeamercolor{structure}{fg=gray, bg=black} % fg controls bullets
+ \setbeamercolor*{footerlike}{fg=white,bg=black} % Controls the footerline
+\else
+ % Default to black on white
+ \setbeamercolor*{footerlike}{fg=white,bg=charcoal} % for charcoal footer
+ \setbeamercolor{structure}{fg=charcoal, bg=white} % fg controls bullets
+ % \setbeamercolor{normal text}{fg=white, bg=black}
+\fi
+
+
+
+
+
+% These defined colors can be used in \textcolor{colorname}{text in that color}.
+
+% Colors for Keynote background: DARK
+\definecolor{keynotebottom}{rgb}{0.32,0.3,0.38}
+\definecolor{keynotemiddle}{rgb}{0.08,0.08,0.16}
+\definecolor{keynotetop}{rgb}{0,0,0}
+%%% Example of usage:
+%% \setbeamertemplate{background canvas}[vertical shading]
+%% [bottom=keynotebottom, middle=keynotemiddle, top=keynotetop]
+
+
+
+
+% ALERT AND COMMENT COLORS (just copies of the above colors)
+% (I don't know how ot do this more elegantly)
+\ifbeamer@Flip@dark
+ \definecolor{ALERT}{RGB}{153,0,0} % crimsonred
+ \definecolor{Alert}{RGB}{51,153,0} % turtlegreen
+ \definecolor{alert}{RGB}{204,204,102} % paleale
+ \definecolor{charcoal}{RGB}{51,51,51} % charcoal
+ \definecolor{comment}{RGB}{80,80,80} % light charcoal
+ \definecolor{Comment}{RGB}{100,100,100} % ash
+ \definecolor{COMMENT}{RGB}{80,20,120} % regal
+\else
+% \definecolor{ALERT}{RGB}{153,0,0} % crimsonred
+ \definecolor{ALERT}{RGB}{28,134,238} % DodgerBlue2
+% \definecolor{Alert}{RGB}{51,153,0} % turtlegreen
+ \definecolor{Alert}{RGB}{255,127,36} % chocolate1
+% \definecolor{alert}{RGB}{140,110,10} % lager
+ \definecolor{alert}{RGB}{0,205,102} % SpringGreen3
+ \definecolor{charcoal}{RGB}{80,80,80} % light charcoal
+ \definecolor{comment}{RGB}{51,51,51} % charcoal
+ \definecolor{Comment}{RGB}{100,100,100} % ash
+ \definecolor{COMMENT}{RGB}{80,20,120} % regal
+\fi
+
+
+% \definecolor{crimsonred}{RGB}{153,0,0} % Neurtal red, good for dark or light bg
+% \definecolor{charcoal}{RGB}{51,51,51} % Darker gray
+% \definecolor{ash}{RGB}{100,100,100} % medium gray
+% \definecolor{paleblue}{RGB}{0,102,102} % More of an `ocean' color
+% \definecolor{turtlegreen}{RGB}{51,153,0} % A more neutral green
+% \definecolor{paleale}{RGB}{204,204,102} % Only for dark BG
+% \definecolor{lager}{RGB}{140,110,10} % Use instead of pale ale for white BG
+% \definecolor{regal}{RGB}{90,0,120} % A more neutral purple
+% \definecolor{jeans}{RGB}{20,30,150} % A more neutral blue
+
+
+% A few useful colors
+\setbeamercolor{alerted text}{fg=alert}
+
+%% I would like ot use these colors, but there seems to be a bug in Beamer
+%% where the footnote color infects the normal text color
+%% See: http://tex.stackexchange.com/questions/8264/beamer-changing-the-footnote-color-also-changes-the-normal-text-color/8268#8268
+
+% \setbeamercolor{footnote}{parent=normal text, fg=FlipSand}
+% \setbeamercolor{footnote mark}{parent=normal text, fg=FlipSand}
+
+% Blocks
+\setbeamercolor{block title}{fg=gray!30!white,bg=charcoal}
+\setbeamercolor{block body}{parent=normal text,bg=gray, fg=white}
+
+\setbeamercolor{block title example}{fg=turtlegreen!30!white,bg=turtlegreen!40!black}
+\setbeamercolor{block body example}{parent=normal text,bg=turtlegreen, fg=white}
+%
+\setbeamercolor{block title alerted}{fg=crimsonred!30!white,bg=crimsonred!40!black}
+\setbeamercolor{block body alerted}{parent=normal text,bg=crimsonred, fg=white}
+
+
+
+% These "setbeamercolor" commands are more standardized.
+
+
+%% From the Beamer User Guide:
+% Outer themes base the color of navigational elements and, possibly, also of other elements, on the
+% four palette colors. The “primary” palette should be used for the most important navigational elements,
+% which are usually the ones that change most often and hence require the most attention by the audience.
+% The “secondary” and “tertiary” are less important, the “quaternary” one is least important.
+% By default, the palette colors do not have a background and the foreground ranges from structure.fg to black.
+% For the sidebar, there is an extra set of palette colors, see palette sidebar primary.
+
+\setbeamercolor*{palette primary}{fg=crimsonred,bg=charcoal}
+\setbeamercolor*{palette secondary}{fg=paleale,bg=lager}
+\setbeamercolor*{palette tertiary}{fg=turtlegreen,bg=jeans}
+\setbeamercolor*{palette quaternary}{fg=paleblue,bg=regal}
+
+% \setbeamercolor*{palette primary}{fg=crimsonred,bg=white}
+% \setbeamercolor*{palette secondary}{fg=charcoal,bg=white}
+% \setbeamercolor*{palette tertiary}{fg=paleblue,bg=white}
+% \setbeamercolor*{palette quaternary}{fg=turtlegreen,bg=white}
+
+
+
+%% These are some structures that I define for use in the outer theme.
+
+\setbeamercolor*{crimsontown}{fg=paleblue,bg=crimsonred}
+\setbeamercolor*{bluetown}{fg=white,bg=DodgerBlue2}
+%\setbeamercolor*{titlelike}{fg=crimsonred}
+\setbeamercolor*{titlelike}{fg=DodgerBlue2}
+\setbeamercolor*{topbarlike}{fg=white, bg=charcoal}
+
+
+
+
+
+%% Some old definitions that I might want to get back to
+%
+% \setbeamercolor*{frametitle}{bg=white,fg=charcoal}
+% \setbeamercolor*{part title}{bg=white,fg=charcoal}
+% \setbeamercolor*{item}{fg=charcoal, bg=white}
+%
+% \setbeamercolor*{separation line}{}
+% \setbeamercolor*{fine separation line}{}
+
+
+
+
+
+\mode
+
diff --git a/UK_VD/26.12.2022/beamerinnerthemeFlip.sty b/UK_VD/26.12.2022/beamerinnerthemeFlip.sty
new file mode 100755
index 0000000..9910f4d
--- /dev/null
+++ b/UK_VD/26.12.2022/beamerinnerthemeFlip.sty
@@ -0,0 +1,95 @@
+% Inner style file for the BEAMER FLIP THEME
+% Copyright 2010 by Flip Tanedo
+% This file may be distributed and/or modified
+% 1. under the LaTeX Project Public License and/or
+% 2. under the GNU Public License.
+%
+% Based on: beamerinnerthemeFlip by Marco Barisione
+
+\mode
+
+% % Use alternative title page style.
+% \DeclareOptionBeamer{alternativetitlepage}[true]{\def\beamer@Flip@alternativetitlepage{#1}}
+
+% Logo to use in the alternative title page.
+% \def\beamer@Flip@titlepagelogo{}
+% \DeclareOptionBeamer{titlepagelogo}{\def\beamer@Flip@titlepagelogo{#1}}
+
+% Bullet shape.
+\DeclareOptionBeamer{bullet}{\def\beamer@Flip@bullet{#1}}
+\DeclareOptionBeamer{shadow}[true]{\def\beamer@themerounded@shadow{#1}}
+\ExecuteOptionsBeamer{shadow=false}
+
+
+% \ExecuteOptionsBeamer{alternativetitlepage=false,bullet=square}
+\ProcessOptionsBeamer
+
+
+
+% Margins.
+\newlength{\beamer@Flip@normalmargin}
+\setlength{\beamer@Flip@normalmargin}{.06\paperwidth}
+\setbeamersize{text margin left=\beamer@Flip@normalmargin}
+\setbeamersize{text margin right=\beamer@Flip@normalmargin}
+\setlength\leftmargini{.6\beamer@Flip@normalmargin}
+\setlength\leftmarginii{.6\beamer@Flip@normalmargin}
+\setlength\leftmarginiii{.6\beamer@Flip@normalmargin}
+
+% Normal title page.
+\defbeamertemplate*{title page normal}{Flip theme}[1][]
+{
+ \vbox{}
+ \vfill
+ \begin{centering}
+ \begin{beamercolorbox}[wd=\paperwidth,sep=8pt,center,#1]{title page header}
+ \usebeamerfont{title}\inserttitle\par%
+ \ifx\insertsubtitle\@empty%
+ \else%
+ \vskip0.25em%
+ {\usebeamerfont{subtitle}\usebeamercolor[fg]{subtitle}\insertsubtitle\par}%
+ \fi%
+ \end{beamercolorbox}%
+ \vskip1em\par
+ \begin{beamercolorbox}[sep=8pt,center,#1]{author}
+ \usebeamerfont{author}\insertauthor
+ \end{beamercolorbox}
+ \begin{beamercolorbox}[sep=8pt,center,#1]{institute}
+ \usebeamerfont{institute}\insertinstitute
+ \end{beamercolorbox}
+ \begin{beamercolorbox}[sep=8pt,center,#1]{date}
+ \usebeamerfont{date}\insertdate
+ \end{beamercolorbox}\vskip0.5em
+ {\usebeamercolor[fg]{titlegraphic}\inserttitlegraphic\par}
+ \end{centering}
+ \vfill
+}
+
+
+% Items.
+\defbeamertemplate{itemize item}{squarealt}%
+{\tiny\raise.5ex\hbox{\donotcoloroutermaths$\blacksquare$}}
+\defbeamertemplate{itemize subitem}{squarealt}%
+{\tiny\raise.4ex\hbox{\donotcoloroutermaths$\square$}}
+\defbeamertemplate{itemize subsubitem}{squarealt}%
+{\tiny\raise.3ex\hbox{\donotcoloroutermaths$\blacksquare$}}
+%
+\defbeamertemplate{itemize item}{circlealt}%
+{\small\raise.2ex\hbox{\donotcoloroutermaths$\bullet$}}
+\defbeamertemplate{itemize subitem}{circlealt}%
+{\small\raise.1ex\hbox{\donotcoloroutermaths$\circ$}}
+\defbeamertemplate{itemize subsubitem}{circlealt}%
+{\scriptsize\raise.1ex\hbox{\donotcoloroutermaths$\bullet$}}
+\setbeamertemplate{items}[circlealt]
+%
+\def\circletext{circle}
+\ifx\beamer@Flip@bullet\circletext
+ \setbeamertemplate{items}[circlealt]
+\else
+ \setbeamertemplate{items}[squarealt]
+\fi
+
+\setbeamertemplate{blocks}[rounded][shadow=\beamer@themerounded@shadow]
+
+
+\mode
+
diff --git a/UK_VD/26.12.2022/beamerouterthemeFlip.sty b/UK_VD/26.12.2022/beamerouterthemeFlip.sty
new file mode 100755
index 0000000..d12f6d6
--- /dev/null
+++ b/UK_VD/26.12.2022/beamerouterthemeFlip.sty
@@ -0,0 +1,189 @@
+% Outer style file for the BEAMER FLIP THEME 212
+% Copyright 2012 by Flip Tanedo
+% This file may be distributed and/or modified
+% 1. under the LaTeX Project Public License and/or
+% 2. under the GNU Public License.
+%
+% Based on: beamerouterthemesplit by Till Tantau
+
+
+\mode
+
+% Watermark
+\DeclareOptionBeamer{watermark}{\def\beamer@Flip@watermark{#1}}
+\ExecuteOptionsBeamer{watermark=} % Default value is empty
+
+
+\newif\ifbeamer@Flip@bigpagenumber
+\beamer@Flip@bigpagenumberfalse
+\DeclareOptionBeamer{bigpagenumber}{\beamer@Flip@bigpagenumbertrue}
+
+
+\def\beamer@Flip@truetext{true} % Kludge for true/false so I can use ifx
+
+\DeclareOptionBeamer{topline}[true]{\def\beamer@Flip@topline{#1}}
+\ExecuteOptionsBeamer{topline=false} % Default
+
+
+
+% \ExecuteOptionsBeamer{topline=} % Default value is empty
+
+
+\ProcessOptionsBeamer
+
+
+\usepackage{tikz} % For fancy decorations
+
+
+% I should fix these up to be more robust against color changes
+\setbeamercolor{section in head/foot}{parent=footerlike}
+\setbeamercolor{subsection in head/foot}{parent=footerlike}
+\setbeamercolor{author in head/foot}{parent=footerlike}
+\setbeamercolor{title in head/foot}{parent=footerlike}
+
+
+% \setbeamercolor{author in head/foot}{parent=section in head/foot}
+% \setbeamercolor{title in head/foot}{parent=subsection in head/foot}
+
+%\setbeamercolor{topbar}{parent=crimsontown}
+\setbeamercolor{topbar}{parent=bluetown}
+
+
+
+
+\usesectionheadtemplate
+ {\hfill\insertsectionhead}
+ {\hfill\color{fg!50!bg}\insertsectionhead}
+
+
+%%%%%%%%%%%%%%%%%%
+% The footer bar %
+%%%%%%%%%%%%%%%%%%
+
+\defbeamertemplate*{footline}{Flip theme}
+{%
+ \leavevmode%
+% OBSERVATION: the "%" symbols inside hbox are all very important here.
+% The \hbox enviroment will insert spaces whenever there's whitespace
+% Adding a % at the END of each line ensures that any hard returns aren't
+% interpreted as white space. This allows the color boxes to be flush against
+% one another. If a faint white line appears one could probably do something like
+% hspace{-1px} and add an additional pixel-or-two wide beamercolorbox.
+
+\hbox{%
+\begin{beamercolorbox}[wd=.4\paperwidth,ht=2.5ex,dp=1.125ex,leftskip=.3cm, rightskip=.3cm plus1fil]{author in head/foot}%
+ \usebeamerfont{author in head/foot}\insertshortauthor \end{beamercolorbox}%
+%
+\begin{beamercolorbox}[wd=.6\paperwidth,ht=2.5ex,dp=1.125ex,leftskip=.3cm,rightskip=.3cm plus1fil]{title in head/foot}%
+ \usebeamerfont{title in head/foot}{\textit \insertshorttitle}%
+ \hskip2ex plus1fill%
+ % \insertpagenumber\,/\,\insertpresentationendpage %% Want FRAME, not SLIDE number
+ \insertframenumber/\inserttotalframenumber
+ \end{beamercolorbox}%
+}%
+
+% This is a complete kludge for the faint white line which appears
+% between the beamer color boxes above. (It doesnt appear in presentation mode
+% but sometimes looks funny when the pdfs are viewed in a window)
+\begin{tikzpicture}[overlay]
+ \usebeamercolor[bg]{author in head/foot}
+ \draw[thick] (0,3.625ex) -- (\paperwidth,3.625ex);
+ \draw (.4\paperwidth,0) -- (.4\paperwidth,3.625ex);
+ \draw[thick] (0,0) -- (\paperwidth,0);
+\end{tikzpicture}
+
+
+
+\ifbeamer@Flip@bigpagenumber
+ \begin{tikzpicture}[overlay]
+ \usebeamercolor[bg]{author in head/foot}
+ \draw[fill] (\paperwidth-5ex,3.625ex) circle (6ex);
+ \usebeamercolor[fg]{author in head/foot}
+ \draw[fill] (\paperwidth-5ex,3.625ex) circle (5ex);
+ \usebeamercolor[bg]{author in head/foot}
+ \node at (\paperwidth-5ex,4ex) {\small$^\text{\insertframenumber}/_\text{\inserttotalframenumber}$};
+ \end{tikzpicture}
+\fi
+}
+
+
+
+\defbeamertemplate*{frametitle}{Flip theme}[1][left]
+{
+% \ifbeamercolorempty[bg]{frametitle}{}{\nointerlineskip}%
+\@tempdima=\textwidth%
+\advance\@tempdima by\beamer@leftmargin%
+\advance\@tempdima by\beamer@rightmargin%
+
+\vbox{}\vskip-3.5ex%
+%
+\begin{beamercolorbox}[sep=0.3cm,#1,wd=\the\@tempdima]{titlelike}
+ \usebeamerfont{frametitle}%
+ \vbox{}\vskip-1ex%
+ \if@tempswa\else\csname beamer@fte#1\endcsname\fi%
+ % \strut{\bf\insertframetitle}\strut\par% %% Include the \bf
+ \strut{\insertframetitle}\strut\par%
+ {%
+ \ifx\insertframesubtitle\@empty%
+ \else
+ {\usebeamerfont{framesubtitle}
+ \usebeamercolor[fg]{framesubtitle}
+ \insertframesubtitle\strut\par}%
+ \fi
+ }%
+ %
+ \vskip-1ex%
+ \if@tempswa\else\vskip-.3cm\fi% set inside beamercolorbox... evil here...
+\end{beamercolorbox}%
+%%
+
+% \def\beamer@fteright{\vskip0.35cm\advance\leftskip by 1.7cm\advance\rightskip by1.7cm}
+}
+
+
+
+
+% Sidebar right is important: anything placed here will be
+% visible *behind* the main text. This is where to put any
+% interesting watermarks.
+%
+%
+\defbeamertemplate*{sidebar right}{Flip theme}
+{
+% \llap{\includegraphics[width=50px]{footdecoration}}
+% \llap{\includegraphics[width=\paperwidth,height=\paperheight]{upperleft_watermark_transp}}
+%
+% THIS WOULD BE A NICE WAY TO PUT THE PARTICLE BUBBLE CHAMBER BG
+% ... make a png of the background with TRANSPARENT BG
+% ... then put the image here (use \hfill to get it on the left)
+% Now one can FURTHER apply a slight gradient in the BG
+%
+%
+% % Top Line
+\ifx\beamer@Flip@topline\beamer@Flip@truetext
+ \begin{tikzpicture}[overlay]
+ \usebeamercolor[fg]{titlelike} % alternately, topbarlike would be a good beamercolor
+% \usebeamercolor[fg]{topbarlike} % alternately, topbarlike would be a good beamercolor
+ \draw[fill] (-\paperwidth,0) rectangle (0,-3pt);
+ \end{tikzpicture}
+\fi
+%
+%
+ \vskip.2\beamer@leftmargin%
+ %\llap{\insertlogo\hskip.5\beamer@leftmargin}%
+ \llap{\insertlogo\hskip.08\beamer@leftmargin}%
+ \vfill%
+ \if \beamer@Flip@watermark\@empty
+ % This is kind of a kludge since if I put anything in here, I automatically get errors
+ % Somehow LaTeX wants to read the \else part!
+ \else%
+ \llap{\includegraphics[width=\paperwidth,height=\paperheight]{\beamer@Flip@watermark}}
+ \fi
+}
+
+
+
+\mode
+\endinput
+
+
diff --git a/UK_VD/26.12.2022/beamerouterthemedecolines.sty b/UK_VD/26.12.2022/beamerouterthemedecolines.sty
new file mode 100755
index 0000000..669e493
--- /dev/null
+++ b/UK_VD/26.12.2022/beamerouterthemedecolines.sty
@@ -0,0 +1,168 @@
+% Copyright 2007 by Marco Barisione
+%
+% This file may be distributed and/or modified
+%
+% 1. under the LaTeX Project Public License and/or
+% 2. under the GNU Public License.
+
+\mode
+
+% String used between the current page and the total page count.
+\def\beamer@decolines@pageofpages{/}
+\DeclareOptionBeamer{pageofpages}{\def\beamer@decolines@pageofpages{#1}}
+
+% Show a line below the frame title.
+\DeclareOptionBeamer{titleline}[true]{\def\beamer@decolines@titleline{#1}}
+
+% Image used for the watermark.
+\def\beamer@decolines@watermarkorig{}
+\DeclareOptionBeamer{watermark}{\def\beamer@decolines@watermarkorig{#1}}
+
+% Height of the watermark.
+\def\beamer@decolines@watermarkheight{100px}
+\DeclareOptionBeamer{watermarkheight}{\def\beamer@decolines@watermarkheight{#1}}
+
+% The original image height is watermarkheightmult * watermarkheight.
+\def\beamer@decolines@watermarkheightmult{1}
+\DeclareOptionBeamer{watermarkheightmult}{\def\beamer@decolines@watermarkheightmult{#1}}
+
+\ExecuteOptionsBeamer{titleline=false}
+\ProcessOptionsBeamer
+
+% Enable/disable the watermark.
+\def\watermarkon{%
+ \def\beamer@decolines@watermark{\beamer@decolines@watermarkorig}%
+}
+\def\watermarkoff{\def\beamer@decolines@watermark{}}
+
+% Initially enable the watermark.
+\watermarkon
+
+% Colors.
+\setbeamercolor*{lineup}{parent=palette primary}
+\setbeamercolor*{linemid}{parent=palette secondary}
+\setbeamercolor*{linebottom}{parent=palette tertiary}
+\setbeamercolor*{page header}{parent=titlelike}
+
+% Lengths
+\newlength{\headerheight}
+\setlength{\headerheight}{.045\paperheight}
+\newlength{\beamer@decolines@lineup}
+\setlength{\beamer@decolines@lineup}{.025\paperheight}
+\newlength{\beamer@decolines@linemid}
+\setlength{\beamer@decolines@linemid}{.015\paperheight}
+\newlength{\beamer@decolines@linebottom}
+\setlength{\beamer@decolines@linebottom}{.01\paperheight}
+
+% The height of the watermark part below the 3 bottom lines.
+\newlength{\beamer@decolines@watermarkheightbottom}
+\addtolength{\beamer@decolines@watermarkheightbottom}{\beamer@decolines@lineup}
+\addtolength{\beamer@decolines@watermarkheightbottom}{\beamer@decolines@linemid}
+\addtolength{\beamer@decolines@watermarkheightbottom}{\beamer@decolines@linebottom}
+
+% The height of the watermark part over the 3 bottom lines before shrinking.
+\newlength{\beamer@decolines@watermarkheightupperorig}
+\setlength{\beamer@decolines@watermarkheightupperorig}{\beamer@decolines@watermarkheight}
+\addtolength{\beamer@decolines@watermarkheightupperorig}{-\beamer@decolines@watermarkheightbottom}
+\multiply\beamer@decolines@watermarkheightupperorig by \beamer@decolines@watermarkheightmult
+
+% % Footer.
+% \defbeamertemplate*{footline}{decolines theme}
+% {
+% \leavevmode%
+% % Page number.
+% \hbox{%
+% \begin{beamercolorbox}[wd=.2\paperwidth,ht=0ex,dp=0ex,center]{}%
+% \usebeamerfont{palette primary}\insertframenumber{} \beamer@decolines@pageofpages{} \inserttotalframenumber%
+% \end{beamercolorbox}%
+% \begin{beamercolorbox}[wd=.8\paperwidth,ht=0ex,dp=0ex]{}%
+% \end{beamercolorbox}%
+% } %
+% % First line.
+% \hbox{%
+% \begin{beamercolorbox}[wd=.2\paperwidth,ht=\beamer@decolines@lineup,dp=0pt]{}%
+% \end{beamercolorbox}%
+% \begin{beamercolorbox}[wd=.8\paperwidth,ht=\beamer@decolines@lineup,dp=0pt]{lineup}%
+% \end{beamercolorbox}%
+% } %
+% % Second line.
+% \hbox{%
+% \begin{beamercolorbox}[wd=\paperwidth,ht=\beamer@decolines@linemid,dp=0pt]{linemid}%
+% \end{beamercolorbox}%
+% } %
+% % Third line.
+% \hbox{%
+% \begin{beamercolorbox}[wd=.1\paperwidth,ht=\beamer@decolines@linebottom,dp=0pt]{}%
+% \end{beamercolorbox}%
+% \begin{beamercolorbox}[wd=.9\paperwidth,ht=\beamer@decolines@linebottom,dp=0pt]{linebottom}%
+% \end{beamercolorbox}%
+% }%
+% % This seems to fix some alignment problems with the watermark. It has to be
+% % always applied if you do not want to see the footer moving up and down when
+% % moving from a page with watermark to a page without or vice versa.
+% \vskip-.5px%
+% % Watermark.
+% \if\beamer@decolines@watermark\@empty\else%
+% \vskip-\beamer@decolines@watermarkheightbottom%
+% \llap{\includegraphics[height=\beamer@decolines@watermarkheightbottom,clip=true,%
+% trim=0pt 0pt 0pt \beamer@decolines@watermarkheightupperorig]{\beamer@decolines@watermark}\hskip-\paperwidth}%
+% \fi%
+% }
+
+\defbeamertemplate*{headline}{decolines theme}
+{
+ \leavevmode%
+ \hbox{%
+ \begin{beamercolorbox}[wd=\paperwidth,ht=\headerheight,dp=0pt]{page header}%
+ \end{beamercolorbox}%
+ } %
+ \vskip0pt%
+}
+
+\defbeamertemplate*{frametitle}{decolines theme}[1][left]
+{
+ \ifbeamercolorempty[bg]{frametitle}{}{\nointerlineskip}%
+ \@tempdima=\textwidth%
+ \advance\@tempdima by\beamer@leftmargin%
+ \advance\@tempdima by\beamer@rightmargin%
+ \vbox{}\vskip-.5\beamer@leftmargin%
+ \begin{beamercolorbox}[sep=\beamer@leftmargin,#1,wd=\the\@tempdima]{}
+ \usebeamerfont{frametitle}\usebeamercolor[bg]{framesubtitle}%
+ \vbox{}\vskip0ex%
+ \if@tempswa\else\csname beamer@fte#1\endcsname\fi%
+ \strut\insertframetitle\strut\par%
+ {%
+ \ifx\insertframesubtitle\@empty%
+ \else%
+ {\usebeamerfont{framesubtitle}\usebeamercolor[bg]{framesubtitle}\insertframesubtitle\strut\par}%
+ \fi
+ }%
+ \vskip-1ex%
+ \if@tempswa\else\vskip-\beamer@leftmargin\fi
+ \end{beamercolorbox}%
+ \def\beamer@decolines@truetext{true}%
+ \ifx\beamer@decolines@titleline\beamer@decolines@truetext%
+ \vskip-.5\beamer@leftmargin%
+ \begin{beamercolorbox}[wd=\textwidth,ht=.1ex,dp=0ex]{linemid}%
+ \end{beamercolorbox}%
+ \fi
+}
+
+% Frame title continuations, default
+\defbeamertemplate*{frametitle continuation}{decolines theme}{(\insertcontinuationcount)}
+
+
+
+\defbeamertemplate*{sidebar right}{decolines theme}
+{
+ \vskip.1\beamer@leftmargin%
+ \llap{\insertlogo\hskip.5\beamer@leftmargin}%
+ \vfill%
+ \if\beamer@decolines@watermark\@empty\else%
+ \llap{\includegraphics[height=\beamer@decolines@watermarkheight]{\beamer@decolines@watermark}}%
+ \vskip-\beamer@decolines@watermarkheightbottom%
+ \fi
+}
+
+\mode
+
diff --git a/UK_VD/26.12.2022/beamerthemeFlip.sty b/UK_VD/26.12.2022/beamerthemeFlip.sty
new file mode 100755
index 0000000..a615ff5
--- /dev/null
+++ b/UK_VD/26.12.2022/beamerthemeFlip.sty
@@ -0,0 +1,59 @@
+% Main style file for the BEAMER FLIP THEME 2012
+% Copyright 2012 by Flip Tanedo
+% This file may be distributed and/or modified
+% 1. under the LaTeX Project Public License and/or
+% 2. under the GNU Public License.
+%
+% Comments: This is still a work in progress.
+% A good way to present: http://www.cs.hmc.edu/~oneill/freesoftware/pdftokeynote.html
+
+% \usepackage{beamerthemesplit}
+\mode
+
+
+%% These are the options that are fed in through the driver file
+%% Some of them get passed on to the other theme files
+\DeclareOptionBeamer{bullet}{\PassOptionsToPackage{bullet=#1}{beamerinnerthemeFlip}}
+\DeclareOptionBeamer{bigpagenumber}{\PassOptionsToPackage{bigpagenumber}{beamerouterthemeFlip}}
+\DeclareOptionBeamer{topline}[true]{\PassOptionsToPackage{topline=#1}{beamerouterthemeFlip}}
+\DeclareOptionBeamer{shadow}[false]{\PassOptionsToPackage{shadow=#1}{beamerinnerthemeFlip}}
+
+\DeclareOptionBeamer{watermark}{\PassOptionsToPackage{watermark=#1}{beamerouterthemeFlip}}
+
+\ProcessOptionsBeamer
+
+\useinnertheme{Flip} % Calls beamerinnerthemeFlip.sty
+\useoutertheme{Flip} % Calls beamerouterthemeFlip.sty
+\usecolortheme{Flip} % Calls beamercolorthemeFlip.sty
+
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%
+% Background Gradient %
+%%%%%%%%%%%%%%%%%%%%%%%%
+
+
+%% Usually I would leave this on
+%% However, there seems to be problems with XeLaTeX
+%% http://tex.stackexchange.com/questions/29497/xelatex-preventing-beamer-from-using-different-backgrounds
+\setbeamertemplate{background canvas}[vertical shading][bottom=blue!.1, middle=white, top=white]
+
+%% HOWEVER: it seems to make it impossible to change this later on in the document
+
+
+%% For a dark background:
+% \setbeamertemplate{background canvas}[vertical shading][bottom=keynotebottom, middle=keynotemiddle, top=keynotetop]
+
+
+%% An alternate way: \beamertemplateshadingbackground{blue!.1}{red!2}
+%% In general: you want the gradient to be subtle!
+
+
+%%%%%%%%%%%%%%%%%%%%%%%
+% Navigation symbols %
+%%%%%%%%%%%%%%%%%%%%%%%
+
+\setbeamertemplate{navigation symbols}{} % Turns off PDF navigation symbols
+
+\mode
+\endinput
\ No newline at end of file
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@@ -0,0 +1,13 @@
+#!/bin/bash
+#FILES=*.pdf
+FILES="$(find . -name '*.pdf')"
+for f in $FILES
+do
+ echo "Processing $f ..."
+ gs -sDEVICE=pdfwrite -dCompatibilityLevel=1.4 -dUseCIEColor -dPDFSETTINGS=/printer -dSAFER -dNOPAUSE -dQUIET -dBATCH -sOutputFile="temp.pdf" "$f"
+ mv temp.pdf "$f"
+# pdf2ps "$f" temp.ps
+# ps2pdf temp.ps "$f"
+# rm temp.ps
+done
+#rm temp.pdf
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+++ b/UK_VD/26.12.2022/images/getFromAFS.sh
@@ -0,0 +1,4 @@
+kinit egraveri@CERN.CH
+aklog
+cp -r /afs/cern.ch/user/e/egraveri/cmtuser/STMonitoring/NewTTAlignment/Out/Plots/AlignVSSimCond-D0Align ./img/
+cp -r /afs/cern.ch/user/e/egraveri/cmtuser/STMonitoring/NewTTAlignment/Out/Plots/AlignVSSimCond-D0AlignNoTT ./img/
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+\usepackage[absolute,overlay]{textpos}
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+\usepackage{amsmath}
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+% http://www.felixl.de/commu.pdf
+\usetikzlibrary{positioning} % For "above of=" commands
+\usetikzlibrary{calc,through} % For coordinates
+\usetikzlibrary{decorations.pathreplacing} % For curly braces
+% http://www.math.ucla.edu/~getreuer/tikz.html
+\usepackage{pgffor} % For repeating patterns
+
+\usetikzlibrary{decorations.pathmorphing} % For Feynman Diagrams
+\usetikzlibrary{decorations.markings}
+\tikzset{
+ % >=stealth', %% Uncomment for more conventional arrows
+ vector/.style={decorate, decoration={snake}, draw},
+ provector/.style={decorate, decoration={snake,amplitude=2.5pt}, draw},
+ antivector/.style={decorate, decoration={snake,amplitude=-2.5pt}, draw},
+ fermion/.style={draw=gray, postaction={decorate},
+ decoration={markings,mark=at position .55 with {\arrow[draw=gray]{>}}}},
+ fermionbar/.style={draw=gray, postaction={decorate},
+ decoration={markings,mark=at position .55 with {\arrow[draw=gray]{<}}}},
+ fermionnoarrow/.style={draw=gray},
+ gluon/.style={decorate, draw=black,
+ decoration={coil,amplitude=4pt, segment length=5pt}},
+ scalar/.style={dashed,draw=black, postaction={decorate},
+ decoration={markings,mark=at position .55 with {\arrow[draw=black]{>}}}},
+ scalarbar/.style={dashed,draw=black, postaction={decorate},
+ decoration={markings,mark=at position .55 with {\arrow[draw=black]{<}}}},
+ scalarnoarrow/.style={dashed,draw=black},
+ electron/.style={draw=black, postaction={decorate},
+ decoration={markings,mark=at position .55 with {\arrow[draw=black]{>}}}},
+ bigvector/.style={decorate, decoration={snake,amplitude=4pt}, draw},
+}
+
+% TIKZ - for block diagrams,
+% from http://www.texample.net/tikz/examples/control-system-principles/
+% \usetikzlibrary{shapes,arrows}
+\tikzstyle{block} = [draw, rectangle,
+minimum height=3em, minimum width=6em]
+
+
+
+
+\usetikzlibrary{backgrounds}
+\usetikzlibrary{mindmap,trees} % For mind map
+\newcommand{\degree}{\ensuremath{^\circ}}
+\newcommand{\E}{\mathrm{E}}
+\newcommand{\Var}{\mathrm{Var}}
+\newcommand{\Cov}{\mathrm{Cov}}
+\newcommand\Ts{\rule{0pt}{2.6ex}} % Top strut
+\newcommand\Bs{\rule[-1.2ex]{0pt}{0pt}} % Bottom strut
+
+\graphicspath{{images/}} % Put all images in this directory. Avoids clutter.
+
+% SOME COMMANDS THAT I FIND HANDY
+% \renewcommand{\tilde}{\widetilde} % dinky tildes look silly, dosn't work with fontspec
+\newcommand{\comment}[1]{\textcolor{comment}{\footnotesize{#1}\normalsize}} % comment mild
+\newcommand{\Comment}[1]{\textcolor{Comment}{\footnotesize{#1}\normalsize}} % comment bold
+\newcommand{\COMMENT}[1]{\textcolor{COMMENT}{\footnotesize{#1}\normalsize}} % comment crazy bold
+\newcommand{\Alert}[1]{\textcolor{Alert}{#1}} % louder alert
+\newcommand{\ALERT}[1]{\textcolor{ALERT}{#1}} % loudest alert
+%% "\alert" is already a beamer pre-defined
+\newcommand*{\Scale}[2][4]{\scalebox{#1}{$#2$}}%
+
+\def\Put(#1,#2)#3{\leavevmode\makebox(0,0){\put(#1,#2){#3}}}
+
+\usepackage{gmp}
+\usepackage[final]{feynmp-auto}
+
+\usepackage[backend=bibtex,style=numeric-comp,firstinits=true]{biblatex}
+\bibliography{bib}
+\setbeamertemplate{bibliography item}[text]
+
+\makeatletter\let\frametextheight\beamer@frametextheight\makeatother
+
+% suppress frame numbering for backup slides
+% you always need the appendix for this!
+\newcommand{\backupbegin}{
+ \newcounter{framenumberappendix}
+ \setcounter{framenumberappendix}{\value{framenumber}}
+}
+\newcommand{\backupend}{
+ \addtocounter{framenumberappendix}{-\value{framenumber}}
+ \addtocounter{framenumber}{\value{framenumberappendix}}
+}
+
+
+\definecolor{links}{HTML}{2A1B81}
+%\hypersetup{colorlinks,linkcolor=,urlcolor=links}
+
+% For shapo's formulas:
+\def\lsi{\raise0.3ex\hbox{$<$\kern-0.75em\raise-1.1ex\hbox{$\sim$}}}
+\def\gsi{\raise0.3ex\hbox{$>$\kern-0.75em\raise-1.1ex\hbox{$\sim$}}}
+\newcommand{\lsim}{\mathop{\lsi}}
+\newcommand{\gsim}{\mathop{\gsi}}
+\newcommand{\wt}{\widetilde}
+%\newcommand{\ol}{\overline}
+\newcommand{\Tr}{\rm{Tr}}
+\newcommand{\tr}{\rm{tr}}
+\newcommand{\eqn}[1]{&\hspace{-0.7em}#1\hspace{-0.7em}&}
+\newcommand{\vev}[1]{\rm{$\langle #1 \rangle$}}
+\newcommand{\abs}[1]{\rm{$\left| #1 \right|$}}
+\newcommand{\eV}{\rm{eV}}
+\newcommand{\keV}{\rm{keV}}
+\newcommand{\GeV}{\rm{GeV}}
+\newcommand{\MeV}{\rm{MeV}}
+\newcommand{\im}{\rm{Im}}
+\newcommand{\re}{{\rm Re}}
+\newcommand{\invfb}{\rm{fb^{-1}}}
+\newcommand{\fixme}{\rm{{\color{red}{FIXME!}}}}
+\newcommand{\thetal}{\theta_l}
+\newcommand{\thetak}{\theta_k}
+\newcommand{\nn}{\nonumber}
+\newcommand{\eq}[1]{\begin{equation} #1 \end{equation}}
+%\newcommand{\eqn}[1]{\begin{displaymath} #1 \end{displaymath}}
+\newcommand{\eqa}[1]{\begin{eqnarray} #1 \end{eqnarray}}
+\newcommand{\apeL}{{A_\perp^L}}
+\newcommand{\apeR}{{A_\perp^R}}
+\newcommand{\apeLR}{{A_\perp^{L,R}}}
+\newcommand{\apaL}{{A_\|^L}}
+\newcommand{\apaR}{{A_\|^R}}
+\newcommand{\apaLR}{{A_\|^{L,R}}}
+\newcommand{\azeL}{{A_0^L}}
+\newcommand{\azeR}{{A_0^R}}
+\newcommand{\azeLR}{{A_0^{L,R}}}
+\newcommand{\Real}{\ensuremath{\mathcal{R}e}\xspace}
+\newcommand{\Imag}{\ensuremath{\mathcal{I}m}\xspace}
+
+\renewcommand{\C}[1]{{\cal C}_{#1}}
+\newcommand{\Ceff}[1]{{\cal C}^{\rm eff}_{#1}}
+\newcommand{\Cpeff}[1]{{\cal C}^{\rm eff\prime}_{#1}}
+\newcommand{\Cp}[1]{{\cal C}^{\prime}_{#1}}
+\def\FL {\ensuremath{F_{\mathrm{L}}}\xspace}
+\def\ATDPH {\ensuremath{A_{\mathrm{T,PR}}^{(2)}}\xspace}
+\def\ATImPH {\ensuremath{A_{\mathrm{T,PR}}^{\mathrm{Im}}}\xspace}
+\def\ATRePH {\ensuremath{A_{\mathrm{T,PR}}^{\mathrm{Re}}}\xspace}
+\def\FLPH {\ensuremath{F_{\mathrm{L,PR}}}\xspace}
+\def\ATDKG {\ensuremath{A_{\mathrm{T,\Kstarz \gamma}}^{(2)}}\xspace}
+\def\ATImKG {\ensuremath{A_{\mathrm{T,\Kstarz \gamma}}^{\mathrm{Im}}}\xspace}
+\def\ATReKG {\ensuremath{A_{\mathrm{T,\Kstarz \gamma}}^{\mathrm{Re}}}\xspace}
+\def\FLKG {\ensuremath{F_{\mathrm{L,\Kstarz \gamma}}}\xspace}
+\def\ATD {\ensuremath{A_{\mathrm{T}}^{(2)}}\xspace}
+\def\ATIm {\ensuremath{A_{\mathrm{T}}^{\mathrm{Im}}}\xspace}
+\def\ATRe {\ensuremath{A_{\mathrm{T}}^{\mathrm{Re}}}\xspace}
+
+\def\cgreen{\color{green}}
+\definecolor{green}{rgb}{0.2,0.6,0.2}
+
+
+\newcommand{\disp}{\displaystyle}
+\def\be{\begin{equation}}
+\def\ee{\end{equation}}
+\def\ba{\begin{eqnarray}}
+\def\ea{\end{eqnarray}}
+\def\d{\partial}
+\def\l{\left(}
+\def\r{\right)}
+\def\la{\langle}
+\def\ra{\rangle}
+\def\e{{\rm e}}
+\def\Br{{\mathcal{B}}}
+
+\def\ARROW{{\color{JungleGreen}{$\Rrightarrow$}}\xspace}
+\def\ARROWR{{\color{WildStrawberry}{$\Rrightarrow$}}\xspace}
+
+\newcommand\textref[1]{%
+ \begin{textblock*}{\paperwidth}(0pt,0.025\textheight)
+ \raggedleft \small{{\color{RoyalBlue} \emph{#1}}}\hspace{1.5em}
+ \end{textblock*}}
+
+\newcommand\textahref[2]{%
+ \begin{textblock*}{\paperwidth}(0pt,0.025\textheight)
+ \raggedleft \small{\emph{\href{#1}{#2} }}\hspace{1.5em}
+ \end{textblock*}}
+
+
+\author{ {Marcin Chrzaszcz} (IFJ PAN)}
+\institute{UZH, IFJ PAN}
+\title[Rare Decays at LHCb]{Rare Decays at LHCb}
+\date{25 September 2014}
+
+
+\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}{0.75\textwidth}
+ \flushright\bfseries \LARGE {Rare decays at LHCb\\ including LFU test and LFV searches}
+ \end{column}
+ \begin{column}{0.02\textwidth}
+ {~}
+ \end{column}
+ \begin{column}{0.23\textwidth}
+ % \hspace*{-1.cm}
+ \vspace*{-3mm}
+ \includegraphics[width=0.6\textwidth]{lhcb-logo}
+ \end{column}
+
+ \end{columns}
+\end{center}
+ \quad
+ \vspace{3em}
+\begin{columns}
+\begin{column}{0.44\textwidth}
+\flushright \vspace{-1.8em} { \Large Marcin Chrzaszcz\\\vspace{-0.1em}\small \href{mailto:mchrzasz@cern.ch}{mchrzasz@cern.ch}}
+
+\end{column}
+\begin{column}{0.53\textwidth}
+\includegraphics[height=1.1cm]{ifj.png}
+\end{column}
+\end{columns}
+
+\vspace{1em}
+ \footnotesize\textcolor{gray}{on behalf of the LHCb collaboration,\\ Institute of Nuclear Physics, Polish Academy of Science}\normalsize\\
+\vspace{0.5em}
+
+ \textcolor{normal text.fg!50!Comment}{BEACH, Krakow, 6 June 2022}
+\end{center}
+\end{frame}
+}
+
+
+
+
+\begin{frame}{Rare Decays at LHCb}
+
+ \begin{minipage}{\textwidth}
+\begin{center}
+
+\begin{columns}
+\column{0.45\textwidth}
+\begin{exampleblock}{Muonic $\PB$ decays}
+\ARROWR Br $\PBs/\PBd \to \mu \mu / \tau \tau$.\\
+\ARROWR Br + Ang. $\PB \to \PKstar \mu \mu$.\\
+\ARROWR Br + Ang. $\PBs \to \Pphi \mu \mu$.\\
+\ARROWR Br + Ang. $\Lambda_b \to p \pi \mu \mu$.\\
+\ARROWR Isospin $\PB \to \PK \mu \mu$.\\
+
+\end{exampleblock}
+
+\begin{alertblock}{Charm decays}
+\ARROWR $\PD\to h h\Pmu \Pmu$\\
+\ARROWR $\PD\to e \mu$.
+\end{alertblock}
+
+
+\ARROW Enormous Physics program which is constantly expanding.\\
+\ARROW Will cover only part of the results.
+\column{0.45\textwidth}
+\begin{alertblock}{LFU test}
+\ARROW $\PBplus \to \PKplus \ell \ell$\\
+\ARROW $\PBd \to \PKstar \ell \ell$\\
+\ARROW $\Lambda_b \to p \pi \ell \ell$\\
+\end{alertblock}
+
+
+
+\begin{exampleblock}{Strange decays}
+\ARROW $\PKshort \to \mu \mu$.
+\end{exampleblock}
+\begin{alertblock}{Radiative decays}
+\ARROWR $\PB \to \PKstar \gamma$, $\PBs \to \Pphi \gamma$\\
+\ARROWR $\Xi_b \to \Xi \gamma$\\
+\ARROWR $\PBs/\PBd \to \PJpsi \gamma$
+\end{alertblock}
+
+\begin{exampleblock}{$\tau$ decays}
+\ARROW $\tau \to \mu \mu \mu$.
+\ARROW $\tau \to p \mu \mu$.
+\end{exampleblock}
+
+\end{columns}
+
+\end{center}
+
+\end{minipage}
+ \vspace*{2.cm}
+\end{frame}
+
+
+
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{frame}\frametitle{Why rare decays?}
+\begin{columns}
+\column{4in}
+\begin{itemize}
+\item In SM allows only the charged interactions to change flavour.
+\begin{itemize}
+\item Other interactions are flavour conserving.
+\end{itemize}
+\item One can escape this constrain and produce $\Pbottom \to \Pstrange$ and $\Pbottom \to \Pdown$ at loop level.
+\begin{itemize}
+\item This kind of processes are suppressed in SM $\to$~Rare decays.
+\item New Physics can enter in the loops.
+\end{itemize}
+\end{itemize}
+\begin{center}
+\includegraphics[scale=0.3]{images/lupa.png}
+\includegraphics[scale=0.3]{images/example.png}
+\end{center}
+\column{1.5in}
+\includegraphics[width=0.61\textwidth]{images/couplings.png}
+\end{columns}
+
+\end{frame}
+
+
+\begin{frame}\frametitle{Tools}
+\begin{itemize}
+\item \textbf{Operator Product Expansion and Effective Field Theory}
+\end{itemize}
+\begin{columns}
+\column{0.1in}{~}
+\column{1.2in}
+\begin{small}
+\begin{align*}
+H_{eff} = - \dfrac{4G_f}{\sqrt{2}} V V^{\prime \ast}\ \sum_i \left[\underbrace{C_i(\mu)O_i(\mu)}_\text{left-handed} +\underbrace{C'_i(\mu)O'_i(\mu)}_\text{right-handed}\right],
+\end{align*}
+\end{small}
+\column{1.8in}
+\begin{tiny}
+\begin{description}
+ \item[i=1,2] Tree
+ \item[i=3-6,8] Gluon penguin
+ \item[i=7] Photon penguin
+ \item[i=9.10] EW penguin
+ \item[i=S] Scalar penguin
+ \item[i=P] Pseudoscalar penguin
+ \end{description}
+
+\end{tiny}
+\end{columns}
+where $C_i$ are the Wilson coefficients and $O_i$ are the corresponding effective operators.
+\begin{center}
+\includegraphics[width=0.85\textwidth,height=3cm]{images/all.png}
+
+\end{center}
+
+
+\end{frame}
+
+
+
+\iffalse
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+
+\begin{frame}
+\only<1>{\frametitle{LHCb detector - tracking}
+
+\begin{columns}
+\column{3in}
+\includegraphics[width=0.9\textwidth]{images/1050px-Lhcbview.jpg}
+
+\column{2in}
+\includegraphics[width=0.95\textwidth]{images/sketch.png}
+\end{columns}
+\begin{itemize}
+\item Excellent Impact Parameter (IP) resolution ($20~\rm \mu m$).\\
+$\Rightarrow$ Identify secondary vertices from heavy flavour decays
+\item Proper time resolution $\sim~40~\rm fs$.\\
+$\Rightarrow$ Good separation of primary and secondary vertices.
+\item Excellent momentum ($\delta p/p \sim 0.5 - 1.0\%$) and inv. mass resolution.\\
+$\Rightarrow$ Low combinatorial background.
+
+\end{itemize}
+
+}
+
+\only<2>{\frametitle{LHCb detector - PID}
+
+\begin{columns}
+\column{3in}
+\includegraphics[width=0.9\textwidth]{images/1050px-Lhcbview.jpg}
+
+\column{2in}
+\includegraphics[width=0.95\textwidth]{images/cher.png}
+\end{columns}
+\begin{itemize}
+\item Excellent Muon identification $\epsilon_{\mu \to \mu} \sim 97\%$, $\epsilon_{\pi \to \mu} \sim 1-3\%$
+\item Good $\PK-\Ppi$ separation via RICH detectors, $\epsilon_{\PK \to \PK} \sim 95\%$, $\epsilon_{\Ppi \to \PK} \sim 5\%$.\\
+$\Rightarrow$ Reject peaking backgrounds.
+\item High trigger efficiencies, low momentum thresholds.
+Muons: $p_T > 1.76 \GeV$ at L0, $p_T > 1.0 \GeV$ at HLT1,\\
+$B \to \PJpsi X $: Trigger $\sim 90\%$.
+
+\end{itemize}
+
+
+}
+
+\textref{Int. J. Mod. Phys. A30 (2015) 1530022}
+\vspace*{2.1cm}
+\end{frame}
+
+
+\fi
+\iffalse
+
+\begin{frame}{Observables in $\PB \to \PKstar \Pmu \Pmu$}
+{~}
+\begin{minipage}{\textwidth}
+
+\ARROW The kinematics of $\PBzero \to \PKstar \Pmuon \APmuon$ decay is described by three angles $\thetal$, $\thetak$, $\phi$ and invariant mass of the dimuon system ($q^2)$.\\
+\ARROW The angular distribution can be written as:
+
+\begin{tiny}
+\begin{align*}
+\left.\frac{1}{{\rm d}(\Gamma+\bar{\Gamma})/{\rm d}q^2}\frac{{\rm d}(\Gamma+\bar{\Gamma})}{{\rm dcos}\thetal\,{\rm dcos}\thetak\,{\rm d}\phi}\right|_{\rm P} =
+\tfrac{9}{32\pi}\bigl[
+&\tfrac{3}{4} (1-{F_{\rm L}})\sin^2\thetak \label{eq:pdfpwave}\\[-0.75em]
+&+ {F_{\rm L}}\cos^2\thetak + \tfrac{1}{4}(1-{F_{\rm L}})\sin^2\thetak\cos 2\thetal\nonumber\\
+&- {F_{\rm L}} \cos^2\thetak\cos 2\thetal + {S_3}\sin^2\thetak \sin^2\thetal \cos 2\phi\nonumber\\
+&+ {S_4} \sin 2\thetak \sin 2\thetal \cos\phi + {S_5}\sin 2\thetak \sin \thetal \cos \phi\nonumber\\
+&+ \tfrac{4}{3} {A_{\rm FB}} \sin^2\thetak \cos\thetal + {S_7} \sin 2\thetak \sin\thetal \sin\phi\nonumber\\
+&+ {S_8} \sin 2\thetak \sin 2\thetal \sin\phi + {S_9}\sin^2\thetak \sin^2\thetal \sin 2\phi \nonumber
+\bigr].
+%\end{split}
+%\bigr],\
+\end{align*}
+\end{tiny}
+
+
+
+\end{minipage}
+\vspace*{2.1cm}
+\end{frame}
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{frame}{Link to effective operators}
+{~}
+\begin{minipage}{\textwidth}
+$\color{JungleGreen}{\Rrightarrow}$ The observables ${\color{red}{S_i}}$ are bilinear combinations of transversity amplitudes: $\apeLR,~\apaLR,~\azeLR $. \\
+$\color{JungleGreen}{\Rrightarrow}$ So here is where the magic happens. At leading order the amplitudes can be written as:
+{\tiny{
+\eqa{
+\apeLR &=&\sqrt{2} N m_B(1- \hat s)\bigg[ (\Ceff9 + \Cpeff9) \mp (\C{10} + \Cp{10})
++\frac{2\hat{m}_b}{\hat s} (\Ceff7 + \Cpeff7) \bigg]\xi_{\bot}(E_{K^*}) \nn \\[2mm]
+\apaLR &=& -\sqrt{2} N m_B (1-\hat s)\bigg[(\Ceff9 - \Cpeff9) \mp (\C{10} - \Cp{10})
++\frac{2\hat{m}_b}{\hat s}(\Ceff7 - \Cpeff7) \bigg] \xi_{\bot}(E_{K^*}) \nn \\[2mm]
+\azeLR &=& -\frac{N m_B (1-\hat s)^2}{2 \hat{m}_{K^*} \sqrt{\hat s}} \bigg[ (\Ceff9 - \Cpeff9) \mp (\C{10} - \Cp{10}) + 2\hat{m}_b (\Ceff7 - \Cpeff7) \bigg]\xi_{\|}(E_{K^*}),
+\label{LargeRecoilAs}\nonumber}
+}}
+where $\hat s = q^2 /m_B^2$, $\hat{m}_i = m_i/m_B$. The $\xi_{\|,\bot }$ are the soft form factors. \\
+\pause
+$\color{JungleGreen}{\Rrightarrow}$ Now we can construct observables that cancel the $\xi$ soft form factors at leading order:
+\eq{P_5^{\prime} = \dfrac{J_5+\bar{J}_5}{2\sqrt{-(J_2^c+\bar{J}_2^c)(J_2^s+\bar{J}_2^s)} }\nonumber
+}
+
+
+\end{minipage}
+\vspace*{2.1cm}
+\end{frame}
+
+% symmetries
+
+\fi
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{frame}{$\PB_{s/d} \to \mu \mu$}
+{~}
+\begin{minipage}{\textwidth}
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{center}
+
+\begin{columns}
+\column{0.52\textwidth}
+\only<1>
+{
+\ARROW Golden channel for LHCb.\\
+\ARROW Normalized to the $\PB \to \PK \Ppi$ and $\PB \to \PK \PJpsi$.\\
+\ARROW The selection is achived by BDT trained on MC and calibrated on data. \\
+%\ARROW $\Br(\PBs \to \mu \mu) = 3.0 \pm 0.6^{+0.3}_{-0.2}$,\\
+\begin{exampleblock}{\begin{small}\ARROWR $\Br(\PBs \to \mu \mu) =( 3.09^{+0.46+0.15}_{-0.43-0.11} )10^{-9}$\end{small}
+}
+$>10~\sigma$ significant!
+\end{exampleblock}
+\begin{alertblock}{}
+\begin{small}\ARROWR $\Br(\PBd \to \mu \mu) < 2.3 \times 10^{-10}$, $90\%\rm CL$\end{small}
+\begin{small}\ARROWR $\Br(\PBs \to \mu \mu \gamma ) < 1.5 \times 10^{-9}$, $90\%\rm CL$\end{small}
+
+\end{alertblock}
+}
+
+\only<2>
+{
+
+\begin{exampleblock}{Effective lifetime}
+\ARROWR Sensitivity to non-scalar NP.\\
+$\tau(\PBs \to \mu\mu)=2.07\pm0.29\pm0.03 \rm~ps$
+\end{exampleblock}
+
+\includegraphics[width=0.9\textwidth]{images/Fig11_bottom_left.pdf}
+}
+
+\column{0.50\textwidth}
+\only<1>{
+\includegraphics[width=0.90\textwidth]{images/Fig10_right_e.pdf}\\
+
+\includegraphics[width=0.90\textwidth]{images/Fig11_top.pdf}\\
+}
+\only<2>{
+\includegraphics[width=0.9\textwidth]{images/Fig17_right.pdf}\\
+
+\includegraphics[width=0.9\textwidth]{images/life.png}\\
+}
+
+\end{columns}
+\end{center}
+
+\end{minipage}
+\textref{PHYS. REV. LETT. 128, (2022) 041801}
+\vspace*{2.1cm}
+\end{frame}
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{frame}{$\PB_{s/d} \to \mu \mu \mu \mu$}
+{~}
+\begin{minipage}{\textwidth}
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{center}
+
+\begin{columns}
+\column{0.52\textwidth}
+\only<1>
+{
+\ARROW \sout{Golden} Platinum channel for LHCb.\\
+\ARROW Normalized to the $\PBs \to \PJpsi(\mu\mu) \phi (\mu\mu)$.\\
+%\ARROW $\Br(\PBs \to \mu \mu) = 3.0 \pm 0.6^{+0.3}_{-0.2}$,\\
+\begin{exampleblock}{UL at $95~\%$ CL:}
+\begin{small}
+\ARROWR $\Br(\PBs \to \mu \mu \mu \mu) < 8.6 \times 10^{-10}$\\
+\ARROWR $\Br(\PBd \to \mu \mu \mu \mu) < 1.8 \times 10^{-10}$\\
+\end{small}
+}
+\end{exampleblock}
+
+\includegraphics[width=0.9\textwidth]{images/Fig4a_4m.pdf}
+
+
+\column{0.50\textwidth}
+\only<1>{
+\includegraphics[width=0.9\textwidth]{images/Fig1_4m.pdf}
+
+\includegraphics[width=0.90\textwidth]{images/Fig3.pdf}\\
+}
+
+
+\end{columns}
+\end{center}
+
+\end{minipage}
+\textref{JHEP 03 (2022) 109}
+\vspace*{2.1cm}
+\end{frame}
+
+
+
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{frame}{$\PB_{s/d} \to \tau \tau$}
+{~}
+\begin{minipage}{\textwidth}
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{center}
+
+\begin{columns}
+\column{0.50\textwidth}
+
+\ARROW NP sensitivity enhanced due to the high $\tau$ mass.\\
+\ARROW More challenging: at least 2$\nu$ are escaping.\\
+\ARROW Selecting $\tau \to 3\pi \nu$, $\rightarrow~9.31~\%$\\
+\ARROW Normalization channel: $\PB \to \PD(\PK \pi \pi) \PDs(\PK \PK \pi)$.\\
+\ARROW No peak in the $\PB$ mass window $\rightarrow$ fit the NN output.
+
+
+\includegraphics[width=0.85\textwidth]{images/hidef_Fig7.png}
+
+
+
+\column{0.50\textwidth}
+
+\includegraphics[width=0.85\textwidth]{images/hidef_Fig11.png}\\
+\includegraphics[width=0.85\textwidth]{images/hidef_Fig2a.png}\\
+\end{columns}
+\end{center}
+
+\end{minipage}
+\textref{Phys. Rev. Lett. 118, 251802 (2017)}
+\vspace*{2.1cm}
+\end{frame}
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{frame}{$\PB_{s/d} \to e e$}
+{~}
+\begin{minipage}{\textwidth}
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{center}
+
+\begin{columns}
+\column{0.52\textwidth}
+
+\ARROW Extreamly rare decays!: $\Br(\PBs \to e e)=(8.60 \pm 0.36) \times 10^{-14}$\\
+$\Br(\PBd \to e e)=(2.41 \pm 0.13) \times 10^{-15}$.\\
+\ARROW Analysed $5~\invfb$ of data.\\
+\ARROW Set UL ($90\%$ CL):\\
+$\Br(\PBs \to e e) <9.4 \times 10^{-9}$\\
+$\Br(\PBd \to e e) <2.5 \times 10^{-9}$
+
+
+
+\includegraphics[width=0.85\textwidth]{images/Fig2a1.pdf}
+
+
+
+\column{0.48\textwidth}
+
+\includegraphics[width=0.85\textwidth]{images/Fig1a.pdf}\\
+\includegraphics[width=0.85\textwidth]{images/Fig9a1.pdf}\\
+\end{columns}
+\end{center}
+
+\end{minipage}
+\textref{PHYS. REV. LETT. 124 (2020) 211802}
+\vspace*{2.1cm}
+\end{frame}
+
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+% B2sll
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{frame}{$\PBzero \to \PKstar \Pmuon \APmuon$ decay }
+{~}
+\begin{minipage}{\textwidth}
+\begin{columns}
+
+\column{0.55\textwidth}
+
+\ARROW $\PBzero \to \PKstar \Pmuon \APmuon$ is a smoking gun for NP hunting!\\
+\ARROW Rich angular observables makes is sensitive to different NP models\\
+\ARROW In addition one can construct less form factor dependent observables:
+\begin{equation}
+P_5^{\prime}=\frac{S_5}{\sqrt{F_L(1-F_L)}}\nonumber
+\end{equation}
+\ARROW Analysed $4.7~\invfb$ of data.\\
+\ARROW Results correspond to $3.3~\sigma$ deviation in $\Re(C_9)$ WC wrt. SM.
+
+\column{0.45\textwidth}
+\includegraphics[width=0.9\textwidth]{images/Fig2d1.pdf} \\
+\includegraphics[width=0.9\textwidth]{images/AFBNEW.pdf}
+
+
+\end{columns}
+
+
+
+\end{minipage}
+ \textref{PHYS. REV. LETT. 125 (2020) 011802}
+
+\vspace*{2.1cm}
+\end{frame}
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{frame}{$\PBu \to \PKstar^+ (\PKshort \pi^+) \Pmuon \APmuon$ decay }
+{~}
+\begin{minipage}{\textwidth}
+\begin{columns}
+
+\column{0.55\textwidth}
+
+\ARROW Isospin partner of previous decay.\\
+\ARROW Experimentally more chalanging due to the $\PKshort$ presents.\\
+\ARROW Analysed $9~\invfb$ of data.\\
+
+\includegraphics[width=0.9\textwidth]{images/Fig1Bu.pdf}
+
+\column{0.45\textwidth}
+\includegraphics[width=0.9\textwidth]{images/Fig2bBu.pdf} \\
+\includegraphics[width=0.9\textwidth]{images/Fig3eBu.pdf}
+
+
+\end{columns}
+
+
+
+\end{minipage}
+ \textref{PHYS. REV. LETT.126 (2021) 161802}
+
+\vspace*{2.1cm}
+\end{frame}
+
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{frame}{$\PBs \to \phi/f^{\prime}_2 (1525) \Pmuon \APmuon$ decays }
+{~}
+\begin{minipage}{\textwidth}
+\begin{columns}
+
+\column{0.6\textwidth}
+
+\ARROW No self-tagging $\rightarrow$ not all angular observables accessible.
+\includegraphics[width=0.46\textwidth]{images/Fig3aBs.pdf}
+\includegraphics[width=0.46\textwidth]{images/Fig2.pdf} \\
+
+\ARROW Tension wrt. the current SM prediction remains.
+
+\includegraphics[width=0.75\textwidth]{images/WC_2_3_like2D.pdf}
+
+\column{0.4\textwidth}
+\includegraphics[width=0.86\textwidth]{images/Fig1bBs.pdf} \\
+\includegraphics[width=0.86\textwidth]{images/Fig3aBs2.pdf}
+\includegraphics[width=0.86\textwidth]{images/Fig3bBs2.pdf}
+
+\end{columns}
+
+
+
+\end{minipage}
+ \textref{PHYS. REV. LETT.127 (2021) 151801,\\JHEP 11 (2021) 043 }
+
+\vspace*{2.1cm}
+\end{frame}
+
+
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{frame}{$\Lambda_b \to p \pi \mu \mu$}
+{~}
+\begin{minipage}{\textwidth}
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{center}
+
+\begin{columns}
+\column{0.60\textwidth}
+
+\ARROW First observation of $b \to d$ in baryon system!\\
+\ARROW BDT selection trained on MC\\
+\ARROW Normalized to $\Lambda_b \to p \pi \PJpsi$\\
+\ARROW With futher QCD improvements we will be able to to measure $\frac{\vert V_{ts}\vert }{\vert V_{td}\vert}$.
+
+\begin{exampleblock}{\begin{small}\ARROWR $\frac{\Br(\Lambda_b \to p \pi \mu \mu)}{\Br(\Lambda_b \to p \pi \PJpsi)} =0.044 \pm 0.012 \pm 0.007$\end{small}
+}
+\ARROWR $5.5~\sigma$ significance! \ARROWR First observation.\\
+\end{exampleblock}
+
+
+\includegraphics[width=0.71\textwidth]{images/hidef_Fig3.png}
+
+
+\column{0.50\textwidth}
+
+\includegraphics[width=0.95\textwidth]{images/dupa.png}\\
+\includegraphics[width=0.95\textwidth]{images/hidef_Fig2.png}\\
+\begin{alertblock}{}\begin{small}
+$\Br(\Lambda_b \to p \pi \mu \mu) = (6.9 \pm 1.9 \pm 1.1^{+1.3}_{-1.0} ) \times 10^{-8}$
+\end{small}
+\end{alertblock}
+\end{columns}
+\end{center}
+
+\end{minipage}
+\textref{J. High Energy Phys. 04 (2017) 029}
+\vspace*{2.1cm}
+\end{frame}
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{frame}{Search for light scalars}
+{~}
+\begin{minipage}{\textwidth}
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{center}
+
+\begin{columns}
+\column{0.55\textwidth}
+\ARROW Hidden sector models are gathering more and more attention.\\
+\ARROW Inflaton model: new scalar then mixes with the Higgs.\\
+\ARROW $\PB$ decays are sensitive as the inflaton might be light.\\
+\ARROW Searched for long living particle $\chi$ produced in: $\PB \to \chi(\mu\mu) \PK$.\\
+\ARROW Analysis performed blindly as a peak search.\\
+\ARROW Light inflaton essentially ruled out:\\
+
+\includegraphics[width=0.75\textwidth]{{images/hidef_Inflaton_parameter_space_log_PAPER}.png}\\
+
+
+
+
+\column{0.45\textwidth}
+
+\includegraphics[width=0.95\textwidth]{images/hidef_diagram.png}\\
+\includegraphics[width=0.95\textwidth]{images/hidef_excluded_limit2D.png}
+
+
+
+\end{columns}
+\end{center}
+
+\end{minipage}
+\textref{Phys. Rev. D 95, 071101 (2017)}
+\vspace*{2.1cm}
+\end{frame}
+
+
+
+
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+
+\begin{frame}\frametitle{$\PBu \to \PK^+ \Pelectron \APelectron$}
+
+\ARROW Most precise measurements performed at LHCb.\\
+\ARROW Main challenge is due to electron Bremsstrahlung.\\
+\begin{center}
+\includegraphics[width=0.45\textwidth]{images/Fig2a_Rk.pdf}
+\includegraphics[width=0.45\textwidth]{images/Fig2b_Rk.pdf}
+
+\end{center}
+\ARROW To protect ourself from electron reconstruction issue we use double ratio:
+\begin{align*}
+R_K = \frac{ \Br(\PB \to \PK \mu \mu ) \times \Br(\PB \to \PK \PJpsi(\to e e)) }{ \Br(\PB \to \PK e e ) \times \Br(\PB \to \PK \PJpsi(\to \mu \mu)) }
+\end{align*}
+
+\textref{NATURE PHYSICS 18, (2022) 277-282}
+\end{frame}
+
+
+
+\begin{frame}\frametitle{$\PBu \to \PK^+ \Pelectron \APelectron$}
+
+\begin{columns}
+
+\column{0.5\textwidth}
+\ARROW The efficiency correction was calculated using $\PB \to \PJpsi \PK$.\\
+\ARROW Cross-checked with $\PB \to \Ppsi(2S) \PK$.\\
+\ARROW The result:\\
+\begin{small}
+$R_{\PK}(1.1 < q^2 < 6.0~\GeV^2/c^4) = 0.846^{+0.042+0.013}_{-0.039-0.012}$
+\end{small}
+
+
+\includegraphics[width=0.95\textwidth]{images/Fig8.pdf}
+\column{0.5\textwidth}
+\includegraphics[width=0.95\textwidth]{images/Fig3b_Rk.pdf}
+\ARROW Disagrees with SM at $3.1~\sigma$ level.
+\includegraphics[width=0.95\textwidth]{images/FigS1.pdf}
+
+\end{columns}
+
+\textref{NATURE PHYSICS 18, (2022) 277-282}
+\end{frame}
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%5
+% RKstar
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+
+
+\begin{frame}\frametitle{$\PBd \to \PKstar \Pelectron \APelectron$}
+\ARROW The neutral continuation of the $R_K$ measurement is to measure its partner:
+\begin{center}
+\begin{align*}
+R_{\PKstar} = \frac{\Br(\PB \to \PKstar \mu \mu)}{\Br(\PB \to \PKstar e e)}
+\end{align*}
+\end{center}
+
+
+\begin{columns}
+
+\column{0.4\textwidth}
+\ARROW Measurement performed in two $q^2$ bins. \\
+
+\ARROW Normalized in double ratio to $\PB \to \PKstar \PJpsi$.\\
+\includegraphics[width=0.95\textwidth]{images/plot.png}
+\column{0.6\textwidth}
+
+\begin{center}
+
+\includegraphics[width=0.92\textwidth]{images/Fig10akstar.pdf}\\
+\ARROW Over $2~\sigma$ deviation in each bin.
+
+\end{center}
+
+
+\end{columns}
+
+
+\textref{JHEP 08 (2017) 055}
+
+\end{frame}
+
+
+
+\begin{frame}\frametitle{$\PBd/\PBu \to \PKshort/\PKstar^+ \Pelectron \APelectron$}
+
+\begin{columns}
+
+\column{0.6\textwidth}
+
+
+\includegraphics[width=0.48\textwidth]{images/for_publication_bd_rare_ee.pdf}
+\includegraphics[width=0.48\textwidth]{images/for_publication_bd_rare_mm.pdf}\\
+
+\includegraphics[width=0.48\textwidth]{images/for_publication_bu_rare_ee.pdf}
+\includegraphics[width=0.48\textwidth]{images/for_publication_bu_rare_mm.pdf}
+
+\ARROW Measurement performed in the low $q^2$ regions.\\
+\ARROW The electron decays have been observed with significance $> 5~\sigma$.
+\column{0.4\textwidth}
+\ARROW Same strategy as previous measurements.\\
+\begin{exampleblock}{Results:}
+$R_{\PKshort} = 0.66^{+0.20+0.02}_{-0.14-0.04}$\\
+$R_{\PKstar^+} = 0.70^{+0.18+0.03}_{-0.13-0.04}$\\
+
+\end{exampleblock}
+\ARROW Consistent with SM at $2\sigma$ level.
+
+\includegraphics[width=0.92\textwidth]{images/R_Comparisons.pdf}
+
+\end{columns}
+
+
+\textref{Phys. Rev. Lett. 128 (2022) 191802}
+
+\end{frame}
+
+
+
+
+\begin{frame}\frametitle{$\PBd \to \PKstar \Pelectron \APelectron$ at low $q^2$}
+
+\begin{columns}
+
+\column{0.6\textwidth}
+\ARROW Use the electrons to measure the radiative penguing.\\
+\ARROW Accessign the kinematic range: $\left[0.0008,0.257\right]~\GeV^2/c^4$.
+
+\begin{alertblock}{}
+$F_L=0.044 \pm 0.026 \pm 0.014$\\
+$A^{Re}_T= −0.06 \pm 0.08 \pm 0.02$\\
+$A^{2}_T= 0.11 \pm 0.10 \pm 0.02$\\
+$A^{Im}_T= 0.02 \pm 0.10 \pm 0.01$\\
+
+\end{alertblock}
+
+\includegraphics[width=0.92\textwidth]{images/Fig4.pdf}
+
+
+
+\column{0.4\textwidth}
+\includegraphics[width=0.95\textwidth]{images/plot.png}
+
+\includegraphics[width=0.92\textwidth]{images/rad_penguin2.jpg}
+
+
+
+\end{columns}
+
+
+
+\textref{JHEP 12 (2020) 081}
+
+\end{frame}
+
+
+\begin{frame}\frametitle{$\PD \to h h \mu \mu$}
+
+\begin{columns}
+
+\column{0.5\textwidth}
+
+\ARROW Extreamly suppressed by GIM mechanism. \\
+\ARROW Dominated by long-range iteractions.\\
+\includegraphics[width=0.45\textwidth]{images/fig1a.pdf}
+\includegraphics[width=0.45\textwidth]{images/fig1b.pdf}\\
+\ARROW Because of tagging $(\PDstar \to \PD \pi_{\rm slow})$ one can measure angular observables.
+
+
+\column{0.5\textwidth}
+\only<1>{
+\includegraphics[width=0.95\textwidth]{images/fig1.pdf}
+}
+\only<2>
+{
+\includegraphics[width=0.95\textwidth]{images/fig2a.pdf}
+
+}
+
+
+
+\end{columns}
+
+
+
+
+
+
+
+\textref{LHCB-PAPER-2021-035, accepted by PRL}
+
+\end{frame}
+
+
+\begin{frame}\frametitle{$\Lambda_c \to \Pproton \mu \mu$}
+
+\vspace{0.5em}
+ \begin{minipage}{\textwidth}
+
+
+\begin{columns}
+\column{0.1in}
+{~}\\
+\column{3in}
+\vspace{0.5em}
+
+\ARROW SM predictions:\\
+~~~~~~$\mathcal{O}(10^{-8})$\\
+\ARROW Long distance effects:\\
+~~~~~~$\mathcal{O}(10^{-6})$\\
+~~~~\\
+\ARROW Previous measurement done by Babar:\\
+~~${\rm Br}(\Lambda_c^{+} \to p \mu^+ \mu^-) < 4.4\cdot 10^{-5}$ at 90\% CL\\
+\begin{center}
+\includegraphics[width=0.65\textwidth]{images/babar.png}\\
+
+\end{center}
+
+
+\column{2in}
+\includegraphics[width=0.95\textwidth]{images/indeks1.jpg}\\
+\includegraphics[width=0.95\textwidth]{images/indeks2.jpg}\\
+\begin{exampleblock}{}
+LHCb analysis with $3~\invfb$
+\end{exampleblock}
+
+
+\end{columns}
+
+ \end{minipage}
+ \vspace*{2.cm}
+
+
+
+\textref{Phys. Rev D 84 072006}
+\end{frame}
+
+
+
+\begin{frame}\frametitle{$\Lambda_c \to \Pproton \mu \mu$}
+
+\begin{columns}
+
+\column{0.02\textwidth}
+
+\column{0.5\textwidth}
+\ARROW It's the first observation of $\Lambda_c \to \Pproton \mu \mu$ in the $\omega$ region, with $5.0~\sigma$ significance.\\
+\ARROW The corresponding branching fraction reads:
+\begin{align*}
+\mathcal{B}(\Lambda_c \to \Pproton \omega) = \left( 9.4 \pm 3.2 \pm 1.0 \pm 2.0 \right) \cdot 10^{-4}
+\end{align*}
+\ARROW No significant excess observed in the nonresonant region:
+\begin{align*}
+\mathcal{B}(\Lambda_c \to \Pproton \mu \mu) < 7.7(9.6) \times 10^{-8}
+\end{align*}
+\ARROW Improving BaBar result by 3 orders of magnitude!
+\column{0.5\textwidth}
+\includegraphics[width=0.92\textwidth]{{images/Lc_mumu_mass_fit_sel}.pdf}\\
+\includegraphics[width=0.92\textwidth]{{images/Lc2pmumu_bf90}.pdf}
+
+
+\end{columns}
+
+\textref{Phys. Rev D , 091101 (2018]}
+\end{frame}
+
+
+
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{frame}{$\PKshort \to \mu \mu$}
+{~}
+\begin{minipage}{\textwidth}
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{center}
+
+\begin{columns}
+\column{0.60\textwidth}
+\ARROW $\Pproton \Pproton$ collisions create enormous amount of strange mesons.\\
+\ARROW Can be used to search for $\PKshort \to \mu \mu$.\\
+\ARROW SM prediction: $\Br(\PKshort \to \mu \mu)= (5.0 \pm 1.5) \times 10^{-12}$\\
+\ARROW Dominated by the long distance effects.\\
+%\ARROW We used two types of triggers: TIS and TOS.\\
+\ARROW Bkg dominated by $\PKshort \to \pi \pi$.
+
+\includegraphics[width=0.75\textwidth]{{images/ks2mumu2}.png}\\
+
+
+
+
+\column{0.4\textwidth}
+
+\includegraphics[width=0.95\textwidth]{images/ks2mumu.png}\\
+\ARROWR No significant enhanced of signal has been observed and UL was set:
+\begin{alertblock}{}\begin{small}
+$\Br(\PKshort \to \mu \mu) <0.8 (1.0) \times 10^{-9}$ at $90 (95)\%$ CL
+\end{small}
+\end{alertblock}
+
+
+\end{columns}
+\end{center}
+
+\end{minipage}
+\textref{Eur. Phys. J. C 77 (2017) 678}
+\vspace*{2.1cm}
+\end{frame}
+
+%%%%%%%%%%%%%%
+
+
+%LFV
+
+
+\begin{frame}\frametitle{$\PBu \to \PK^+ \mu e$}
+\begin{columns}
+
+\column{0.5\textwidth}
+\ARROW Normalized to $\PB \to \PK \PJpsi(\mu\mu)$.\\
+\ARROW Both charge sign combinations considered: $\PBu \to \PK^+ \mu^{\pm} e^{\mp}$
+
+\includegraphics[width=0.49\textwidth]{images/Fig3bLFVem.pdf}
+\includegraphics[width=0.49\textwidth]{images/Fig3bLFVem.pdf}
+\begin{alertblock}{Results at $90~\%$ CL:}
+\ARROWR $\Br(\PBu \to \PK^+ \mu^- e^+<7.0\times10^{-9}$\\
+\ARROWR $\Br(\PBu \to \PK^+ \mu^+ e^-<6.4\times10^{-9}$
+\end{alertblock}
+
+
+
+\column{0.5\textwidth}
+
+\includegraphics[width=0.95\textwidth]{images/Fig2aLFVem.pdf}
+\includegraphics[width=0.95\textwidth]{images/Fig2bLFVem.pdf}
+
+
+\end{columns}
+
+
+\textref{PHYS. REV. LETT.123 (2019) 241802}
+
+\end{frame}
+
+\begin{frame}\frametitle{$\PB \to \PK \mu \tau$}
+
+
+\begin{columns}
+
+\column{0.5\textwidth}
+
+\ARROW Very challanging due to presents of $\tau$ lepton.\\
+\ARROW Use the $\PB_{s2}^{\ast 0} \to \PB^+ \PK^-$ to reconstruct the $\tau$ momentum.\\
+\ARROW Normalized to $\PB \to \PK \PJpsi(\mu\mu)$.
+
+\includegraphics[width=0.49\textwidth]{images/Fig3aLFV.pdf}
+\includegraphics[width=0.49\textwidth]{images/Fig3bLFV.pdf}
+\includegraphics[width=0.49\textwidth]{images/Fig3cLFV.pdf}
+\includegraphics[width=0.49\textwidth]{images/Fig3dLFV.pdf}
+
+\column{0.5\textwidth}
+
+\includegraphics[width=0.95\textwidth]{images/Fig2aLFV.pdf}
+\includegraphics[width=0.95\textwidth]{images/Fig4LFV.pdf}
+
+
+\end{columns}
+
+
+
+
+\textref{JHEP 06 (2020) 129}
+
+\end{frame}
+
+
+
+
+
+
+
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{frame}{Conclusions}
+{~}
+\begin{minipage}{\textwidth}
+\begin{itemize}
+\item Lots of rare decays studied at LHCb.
+\item Observed tensions wrt. to SM in the $\Pbeauty \to \Pstrange \ell \ell$ transitions.
+\item LHCb is setting nowadays strongest limits on LFV.
+\item LUV are the cleanest (wrt. theory errors) of the anomalies.
+\end{itemize}
+
+
+\end{minipage}
+\vspace*{2.1cm}
+\end{frame}
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{frame}
+{~}
+\begin{minipage}{\textwidth}
+\begin{center}
+\begin{LARGE}
+Thank you for the attention!
+\end{LARGE}
+\includegraphics[width=0.8\textwidth]{images/Joke.jpg}
+
+\end{center}
+
+
+
+\end{minipage}
+\vspace*{2.1cm}
+\end{frame}
+
+
+
+\backupbegin
+
+\begin{frame}\frametitle{Backup}
+
+
+\end{frame}
+
+
+
+
+
+
+\begin{frame}{Theory implications}
+{~}
+ \begin{minipage}{\textwidth}
+
+\includegraphics[height=0.9\textheight]{images/table.png}
+
+
+\end{minipage}
+ \vspace*{2.1cm}
+\end{frame}
+
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{frame}{If not NP?}
+{~}
+\begin{minipage}{\textwidth}
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+
+
+\begin{itemize}
+\item How about our clean $P_i$ observables?
+\item The QCD cancel as mentioned only at leading order.
+\item Comparison to normal observables with the optimised ones.
+\end{itemize}
+\includegraphics[width=0.9\textwidth]{images/C9_S_P.png}
+
+
+\end{minipage}
+\vspace*{2.1cm}
+\end{frame}
+
+
+
+
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{frame}{Transversity amplitudes }
+{~}
+\begin{minipage}{\textwidth}
+
+$\color{JungleGreen}{\Rrightarrow}$ One can link the angular observables to transversity amplitudes
+{\tiny{
+\eqa{
+J_{1s} & = & \frac{(2+\beta_\ell^2)}{4} \left[|\apeL|^2 + |\apaL|^2 +|\apeR|^2 + |\apaR|^2 \right]
+ + \frac{4 m_\ell^2}{q^2} \re\left(\apeL\apeR^* + \apaL\apaR^*\right)\,,\nn\\[1mm]
+%
+J_{1c} & = & |\azeL|^2 +|\azeR|^2 + \frac{4m_\ell^2}{q^2} \left[|A_t|^2 + 2\re(\azeL^{}\azeR^*) \right] + \beta_\ell^2\, |A_S|^2 \,,\nn\\[1mm]
+%
+J_{2s} & = & \frac{ \beta_\ell^2}{4}\left[ |\apeL|^2+ |\apaL|^2 + |\apeR|^2+ |\apaR|^2\right],
+\hspace{0.92cm} J_{2c} = - \beta_\ell^2\left[|\azeL|^2 + |\azeR|^2 \right]\,,\nn\\[1mm]
+%
+J_3 & = & \frac{1}{2}\beta_\ell^2\left[ |\apeL|^2 - |\apaL|^2 + |\apeR|^2 - |\apaR|^2\right],
+\qquad J_4 = \frac{1}{\sqrt{2}}\beta_\ell^2\left[\re (\azeL\apaL^* + \azeR\apaR^* )\right],\nn \\[1mm]
+%
+J_5 & = & \sqrt{2}\beta_\ell\,\Big[\re(\azeL\apeL^* - \azeR\apeR^* ) - \frac{m_\ell}{\sqrt{q^2}}\,
+\re(\apaL A_S^*+ \apaR^* A_S) \Big]\,,\nn\\[1mm]
+%
+J_{6s} & = & 2\beta_\ell\left[\re (\apaL\apeL^* - \apaR\apeR^*) \right]\,,
+\hspace{2.25cm} J_{6c} = 4\beta_\ell\, \frac{m_\ell}{\sqrt{q^2}}\, \re (\azeL A_S^*+ \azeR^* A_S)\,,\nn\\[1mm]
+%
+J_7 & = & \sqrt{2} \beta_\ell\, \Big[\im (\azeL\apaL^* - \azeR\apaR^* ) +
+\frac{m_\ell}{\sqrt{q^2}}\, \im (\apeL A_S^* - \apeR^* A_S)) \Big]\,,\nn\\[1mm]
+%
+J_8 & = & \frac{1}{\sqrt{2}}\beta_\ell^2\left[\im(\azeL\apeL^* + \azeR\apeR^*)\right]\,,
+%
+\hspace{1.9cm} J_9 = \beta_\ell^2\left[\im (\apaL^{*}\apeL + \apaR^{*}\apeR)\right] \,,
+\label{Js}\nonumber}
+}}
+
+\end{minipage}
+\vspace*{2.1cm}
+\end{frame}
+
+
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{frame}{Link to effective operators}
+{~}
+\begin{minipage}{\textwidth}
+$\color{JungleGreen}{\Rrightarrow}$ So here is where the magic happens. At leading order the amplitudes can be written as (soft form factors):
+{\tiny{
+\eqa{
+\apeLR &=&\sqrt{2} N m_B(1- \hat s)\bigg[ (\Ceff9 + \Cpeff9) \mp (\C{10} + \Cp{10})
++\frac{2\hat{m}_b}{\hat s} (\Ceff7 + \Cpeff7) \bigg]\xi_{\bot}(E_{K^*}) \nn \\[2mm]
+\apaLR &=& -\sqrt{2} N m_B (1-\hat s)\bigg[(\Ceff9 - \Cpeff9) \mp (\C{10} - \Cp{10})
++\frac{2\hat{m}_b}{\hat s}(\Ceff7 - \Cpeff7) \bigg] \xi_{\bot}(E_{K^*}) \nn \\[2mm]
+\azeLR &=& -\frac{N m_B (1-\hat s)^2}{2 \hat{m}_{K^*} \sqrt{\hat s}} \bigg[ (\Ceff9 - \Cpeff9) \mp (\C{10} - \Cp{10}) + 2\hat{m}_b (\Ceff7 - \Cpeff7) \bigg]\xi_{\|}(E_{K^*}),
+\label{LargeRecoilAs}\nonumber}
+}}
+where $\hat s = q^2 /m_B^2$, $\hat{m}_i = m_i/m_B$. The $\xi_{\|,\bot }$ are the form factors. \\
+\pause
+$\color{JungleGreen}{\Rrightarrow}$ Now we can construct observables that cancel the $\xi$ form factors at leading order:
+\eq{P_5^{\prime} = \dfrac{J_5+\bar{J}_5}{2\sqrt{-(J_2^c+\bar{J}_2^c)(J_2^s+\bar{J}_2^s)} }\nonumber
+}
+
+
+\end{minipage}
+\vspace*{2.1cm}
+\end{frame}
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{frame}{$\PBzero \to \PKstar \Pmuon \APmuon$ kinematics}
+{~}
+\begin{minipage}{\textwidth}
+
+$\color{JungleGreen}{\Rrightarrow}$ 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}
+\column{0.5\textwidth}
+
+$\color{JungleGreen}{\Rrightarrow}$ $\cos \thetak$: the angle between the direction of the kaon in the $\PKstar$ ($\overline{\PK}^{\ast}$) rest frame and the direction of the $\PKstar$ ($\overline{\PK}^{\ast}$) in the $\PBzero$ ($\APBzero$) rest frame.\\
+$\color{JungleGreen}{\Rrightarrow}$ $\cos \thetal$: the angle between the direction of the $\Pmuon$ ($\APmuon$) in the dimuon rest frame and the direction of the dimuon in the $\PBzero$ ($\APBzero$) rest frame.\\
+$\color{JungleGreen}{\Rrightarrow}$ $\phi$: the angle between the plane containing the $\Pmuon$ and $\APmuon$ and the plane containing the kaon and pion from the $\PKstar$.
+
+
+
+\column{0.5\textwidth}
+\includegraphics[width=0.99\textwidth]{images/angles.png}
+
+\end{columns}
+}
+ \only<2>{
+{\tiny{
+\eqa{\label{dist}
+\frac{d^4\Gamma}{dq^2\,d\!\cos\theta_K\,d\!\cos\theta_l\,d\phi}&=&\frac9{32\pi} \bigg[
+{\color{red}{J_{1s}}} \sin^2\theta_K + {\color{red}{J_{1c}}} \cos^2\theta_K + ({\color{red}{J_{2s} }}\sin^2\theta_K + {\color{red}{J_{2c}}} \cos^2\theta_K) \cos 2\theta_l\nn\\[1.5mm]
+&&\hspace{-2.7cm}+ {\color{red}{J_3}} \sin^2\theta_K \sin^2\theta_l \cos 2\phi + {\color{red}{J_4}} \sin 2\theta_K \sin 2\theta_l \cos\phi + {\color{red}{J_5}} \sin 2\theta_K \sin\theta_l \cos\phi \nn\\[1.5mm]
+&&\hspace{-2.7cm}+ ({\color{red}{J_{6s}}} \sin^2\theta_K + {\color{red}{{J_{6c}}}} \cos^2\theta_K) \cos\theta_l
++ {\color{red}{J_7}} \sin 2\theta_K \sin\theta_l \sin\phi + {\color{red}{J_8}} \sin 2\theta_K \sin 2\theta_l \sin\phi \nn\\[1.5mm]
+&&\hspace{-2.7cm}+ {\color{red}{J_9}} \sin^2\theta_K \sin^2\theta_l \sin 2\phi \bigg]\,,
+\nonumber}
+}}\\{~}\\
+$\color{JungleGreen}{\Rrightarrow}$ This is the most general expression of this kind of decay.\\
+$\color{JungleGreen}{\Rrightarrow}$ The $CP$ averaged angular observables are defined:\\
+\eq{
+S_i = \dfrac{J_i+ \bar{J}_i}{(d \Gamma + d \bar{\Gamma})/dq^2}\nonumber
+}
+
+}
+
+\end{minipage}
+\vspace*{2.1cm}
+\end{frame}
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{frame}{Link to effective operators}
+{~}
+\begin{minipage}{\textwidth}
+$\color{JungleGreen}{\Rrightarrow}$ The observables ${\color{red}{J_i}}$ are bilinear combinations of transversity amplitudes: $\apeLR,~\apaLR,~\azeLR $. \\
+$\color{JungleGreen}{\Rrightarrow}$ So here is where the magic happens. At leading order the amplitudes can be written as:
+{\tiny{
+\eqa{
+\apeLR &=&\sqrt{2} N m_B(1- \hat s)\bigg[ (\Ceff9 + \Cpeff9) \mp (\C{10} + \Cp{10})
++\frac{2\hat{m}_b}{\hat s} (\Ceff7 + \Cpeff7) \bigg]\xi_{\bot}(E_{K^*}) \nn \\[2mm]
+\apaLR &=& -\sqrt{2} N m_B (1-\hat s)\bigg[(\Ceff9 - \Cpeff9) \mp (\C{10} - \Cp{10})
++\frac{2\hat{m}_b}{\hat s}(\Ceff7 - \Cpeff7) \bigg] \xi_{\bot}(E_{K^*}) \nn \\[2mm]
+\azeLR &=& -\frac{N m_B (1-\hat s)^2}{2 \hat{m}_{K^*} \sqrt{\hat s}} \bigg[ (\Ceff9 - \Cpeff9) \mp (\C{10} - \Cp{10}) + 2\hat{m}_b (\Ceff7 - \Cpeff7) \bigg]\xi_{\|}(E_{K^*}),
+\label{LargeRecoilAs}\nonumber}
+}}
+where $\hat s = q^2 /m_B^2$, $\hat{m}_i = m_i/m_B$. The $\xi_{\|,\bot }$ are the soft form factors. \\
+\pause
+$\color{JungleGreen}{\Rrightarrow}$ Now we can construct observables that cancel the $\xi$ soft form factors at leading order:
+\eq{P_5^{\prime} = \dfrac{J_5+\bar{J}_5}{2\sqrt{-(J_2^c+\bar{J}_2^c)(J_2^s+\bar{J}_2^s)} }\nonumber
+}
+
+
+\end{minipage}
+\vspace*{2.1cm}
+\end{frame}
+
+% symmetries
+\begin{frame}{Symmetries in $\PB \to \PKstar \Pmu \Pmu$}
+{~}
+\begin{minipage}{\textwidth}
+$\color{JungleGreen}{\Rrightarrow}$ We have 12 angular coefficients ($S_i$).\\
+$\color{JungleGreen}{\Rrightarrow}$ There exist 4 symmetry transformations that leave the angular distributions unchanged:
+\begin{tiny}
+\eq{
+n_\|=\binom{A_\|^L}{A_\|^{R*}}\ ,\quad
+n_\bot=\binom{A_\bot^L}{-A_\bot^{R*}}\ ,\quad
+n_0=\binom{A_0^L}{A_0^{R*}}\ .\nonumber
+}
+\end{tiny}
+\begin{tiny}
+\eq{
+ n_i^{'} = U n_i=
+ \left[
+ \begin{array}{ll}
+ e^{i\phi_L} & 0 \\
+ 0 & e^{-i \phi_R}
+ \end{array}
+ \right]
+ \left[
+ \begin{array}{rr}
+ \cos \theta & -\sin \theta \\
+ \sin \theta & \cos \theta
+ \end{array}
+ \right]
+ \left[
+ \begin{array}{rr}
+ \cosh i \tilde{\theta} & -\sinh i \tilde{\theta} \\
+ - \sinh i \tilde{\theta} & \cosh i \tilde{\theta}
+ \end{array}
+ \right]
+ n_i \,.
+ \label{symmassless}\nonumber}
+\end{tiny}
+$\color{JungleGreen}{\Rrightarrow}$ Using this symmetries one can show that there are 8 independent observables. The pdf can be written as:
+\begin{tiny}
+\begin{align*}
+\left.\frac{1}{{\rm d}(\Gamma+\bar{\Gamma})/{\rm d}q^2}\frac{{\rm d}(\Gamma+\bar{\Gamma})}{{\rm dcos}\thetal\,{\rm dcos}\thetak\,{\rm d}\phi}\right|_{\rm P} =
+\tfrac{9}{32\pi}\bigl[
+&\tfrac{3}{4} (1-{F_{\rm L}})\sin^2\thetak \label{eq:pdfpwave}\\[-0.75em]
+&+ {F_{\rm L}}\cos^2\thetak + \tfrac{1}{4}(1-{F_{\rm L}})\sin^2\thetak\cos 2\thetal\nonumber\\
+&- {F_{\rm L}} \cos^2\thetak\cos 2\thetal + {S_3}\sin^2\thetak \sin^2\thetal \cos 2\phi\nonumber\\
+&+ {S_4} \sin 2\thetak \sin 2\thetal \cos\phi + {S_5}\sin 2\thetak \sin \thetal \cos \phi\nonumber\\
+&+ \tfrac{4}{3} {A_{\rm FB}} \sin^2\thetak \cos\thetal + {S_7} \sin 2\thetak \sin\thetal \sin\phi\nonumber\\
+&+ {S_8} \sin 2\thetak \sin 2\thetal \sin\phi + {S_9}\sin^2\thetak \sin^2\thetal \sin 2\phi \nonumber
+\bigr].
+%\end{split}
+%\bigr],\
+\end{align*}
+\end{tiny}
+
+\end{minipage}
+\vspace*{2.1cm}
+\end{frame}
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+
+
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{frame}{$\Lambda_b \to p \pi \mu \mu$}
+{~}
+\begin{minipage}{\textwidth}
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{center}
+
+\begin{columns}
+\column{0.60\textwidth}
+
+\ARROW First observation of $b \to d$ in baryon system!\\
+\ARROW BDT selection trained on MC\\
+\ARROW Normalized to $\Lambda_b \to p \pi \PJpsi$\\
+\ARROW With futher QCD improvements we will be able to to measure $\frac{\vert V_{ts}\vert }{\vert V_{td}\vert}$.
+
+\begin{exampleblock}{\begin{small}\ARROWR $\frac{\Br(\Lambda_b \to p \pi \mu \mu)}{\Br(\Lambda_b \to p \pi \PJpsi)} =0.044 \pm 0.012 \pm 0.007$\end{small}
+}
+\ARROWR $5.5~\sigma$ significance! \ARROWR First observation.\\
+\end{exampleblock}
+
+
+\includegraphics[width=0.71\textwidth]{images/hidef_Fig3.png}
+
+
+\column{0.50\textwidth}
+
+\includegraphics[width=0.95\textwidth]{images/dupa.png}\\
+\includegraphics[width=0.95\textwidth]{images/hidef_Fig2.png}\\
+\begin{alertblock}{}\begin{small}
+$\Br(\Lambda_b \to p \pi \mu \mu) = (6.9 \pm 1.9 \pm 1.1^{+1.3}_{-1.0} ) \times 10^{-8}$
+\end{small}
+\end{alertblock}
+\end{columns}
+\end{center}
+
+\end{minipage}
+\textref{J. High Energy Phys. 04 (2017) 029}
+\vspace*{2.1cm}
+\end{frame}
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{frame}{Search for light scalars}
+{~}
+\begin{minipage}{\textwidth}
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{center}
+
+\begin{columns}
+\column{0.55\textwidth}
+\ARROW Hidden sector models are gathering more and more attention.\\
+\ARROW Inflaton model: new scalar then mixes with the Higgs.\\
+\ARROW $\PB$ decays are sensitive as the inflaton might be light.\\
+\ARROW Searched for long living particle $\chi$ produced in: $\PB \to \chi(\mu\mu) \PK$.\\
+\ARROW Analysis performed blindly as a peak search.\\
+\ARROW Light inflaton essentially ruled out:\\
+
+\includegraphics[width=0.75\textwidth]{{images/hidef_Inflaton_parameter_space_log_PAPER}.png}\\
+
+
+
+
+\column{0.45\textwidth}
+
+\includegraphics[width=0.95\textwidth]{images/hidef_diagram.png}\\
+\includegraphics[width=0.95\textwidth]{images/hidef_excluded_limit2D.png}
+
+
+
+\end{columns}
+\end{center}
+
+\end{minipage}
+\textref{Phys. Rev. D 95, 071101 (2017)}
+\vspace*{2.1cm}
+\end{frame}
+
+
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{frame}{$\PBzero \to \PKstar \Pmuon \APmuon$ decay }
+{~}
+\begin{minipage}{\textwidth}
+\begin{columns}
+
+\column{0.55\textwidth}
+
+\ARROW $\PBzero \to \PKstar \Pmuon \APmuon$ is a smoking gun for NP hunting!\\
+\ARROW Reach angular observables makes is sensitive to different NP models\\
+\ARROW In addition one can construct less form factor dependent observables:
+\begin{equation}
+P_5^{\prime}=\frac{S_5}{\sqrt{F_L(1-F_L)}}\nonumber
+\end{equation}
+\ARROW In single analysis observed $3.4~\sigma$ discrepancy in the $C_9$ WC.
+
+
+
+\column{0.45\textwidth}
+\includegraphics[width=0.9\textwidth]{images/P5p.pdf} \\
+\includegraphics[width=0.9\textwidth]{images/AFBPad.pdf}
+
+
+\end{columns}
+
+
+
+\end{minipage}
+ \textref{JHEP 02 (2016) 104, CMS-PAS-BPH-15-008,\\ ATLAS-CONF-2017-023, Phys. Rev. Lett. 118 (2017)}
+
+\vspace*{2.1cm}
+\end{frame}
+
+
+
+
+
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{frame}{$\PBzero \to \PKstar \Pmuon \APmuon$ decay }
+{~}
+\begin{minipage}{\textwidth}
+\begin{columns}
+
+\column{0.55\textwidth}
+
+\ARROW $\PBzero \to \PKstar \Pmuon \APmuon$ is a smoking gun for NP hunting!\\
+\ARROW Reach angular observables makes is sensitive to different NP models\\
+\ARROW In addition one can construct less form factor dependent observables:
+\begin{equation}
+P_5^{\prime}=\frac{S_5}{\sqrt{F_L(1-F_L)}}\nonumber
+\end{equation}
+\ARROW In single analysis observed $3.4~\sigma$ discrepancy in the $C_9$ WC.
+
+
+
+\column{0.45\textwidth}
+\includegraphics[angle=-90,width=0.9\textwidth]{images/P5p.pdf} \\
+\includegraphics[angle=-90,width=0.9\textwidth]{images/AFBPad.pdf}
+
+
+\end{columns}
+
+
+
+\end{minipage}
+ \textref{JHEP 02 (2016) 104, CMS-PAS-BPH-15-008,\\ ATLAS-CONF-2017-023, Phys. Rev. Lett. 118 (2017)}
+
+\vspace*{2.1cm}
+\end{frame}
+
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{frame}{Branching fraction measurements of $\PBs \to \Pphi \Pmu \Pmu$}
+{~}
+\begin{minipage}{\textwidth}
+ \begin{center}
+ \includegraphics[height=4cm]{images/bs2phipi.png}
+ \includegraphics[height=4cm]{images/BsSel.png}
+ \end{center}
+
+\begin{itemize}
+\item Recent LHCb measurement, \href{https://cds.cern.ch/record/2029820/files/JHEP09-179.pdf}{{\color{blue}{JHEP09 (2015) 179}}}.
+\item Suppressed by $\frac{f_s}{f_d}$.
+\item Cleaner because of narrow $\Pphi$ resonance.
+\item $3.3~\sigma$ deviation in SM in the $1-6\GeV^2$ bin.
+\item Angular part in agreement with SM ($S_5$ is not accessible).
+\end{itemize}
+
+
+\end{minipage}
+\vspace*{2.1cm}
+\end{frame}
+
+
+
+
+
+
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{frame}{Theory implications of $b \to s \ell \ell$}
+{~}
+\begin{minipage}{\textwidth}
+
+\begin{itemize}
+\item A fit prepared by \texttt{S. Descotes-Genon, L. Hofer, J. Matias, J. Virto}.
+\item The data can be explained by modifying the $C_9$ Wilson coefficient.
+\item Overall there is $>4~\sigma$ discrepancy wrt. the SM prediction.
+\end{itemize}
+\includegraphics[width=0.9\textwidth]{images/FIT.png}
+
+
+
+
+\end{minipage}
+\textref{JHEP 06 (2016) 092}
+\vspace*{2.1cm}
+\end{frame}
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{frame}{Observables in $\PB \to \PKstar \Pmu \Pmu$}
+{~}
+\begin{minipage}{\textwidth}
+
+\ARROW The kinematics of $\PBzero \to \PKstar \Pmuon \APmuon$ decay is described by three angles $\thetal$, $\thetak$, $\phi$ and invariant mass of the dimuon system ($q^2)$.\\
+\ARROW The angular distribution can be written as:
+
+\begin{tiny}
+\begin{align*}
+\left.\frac{1}{{\rm d}(\Gamma+\bar{\Gamma})/{\rm d}q^2}\frac{{\rm d}(\Gamma+\bar{\Gamma})}{{\rm dcos}\thetal\,{\rm dcos}\thetak\,{\rm d}\phi}\right|_{\rm P} =
+\tfrac{9}{32\pi}\bigl[
+&\tfrac{3}{4} (1-{F_{\rm L}})\sin^2\thetak \label{eq:pdfpwave}\\[-0.75em]
+&+ {F_{\rm L}}\cos^2\thetak + \tfrac{1}{4}(1-{F_{\rm L}})\sin^2\thetak\cos 2\thetal\nonumber\\
+&- {F_{\rm L}} \cos^2\thetak\cos 2\thetal + {S_3}\sin^2\thetak \sin^2\thetal \cos 2\phi\nonumber\\
+&+ {S_4} \sin 2\thetak \sin 2\thetal \cos\phi + {S_5}\sin 2\thetak \sin \thetal \cos \phi\nonumber\\
+&+ \tfrac{4}{3} {A_{\rm FB}} \sin^2\thetak \cos\thetal + {S_7} \sin 2\thetak \sin\thetal \sin\phi\nonumber\\
+&+ {S_8} \sin 2\thetak \sin 2\thetal \sin\phi + {S_9}\sin^2\thetak \sin^2\thetal \sin 2\phi \nonumber
+\bigr].
+%\end{split}
+%\bigr],\
+\end{align*}
+\end{tiny}
+
+
+
+\end{minipage}
+\vspace*{2.1cm}
+\end{frame}
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{frame}{Link to effective operators}
+{~}
+\begin{minipage}{\textwidth}
+$\color{JungleGreen}{\Rrightarrow}$ The observables ${\color{red}{S_i}}$ are bilinear combinations of transversity amplitudes: $\apeLR,~\apaLR,~\azeLR $. \\
+$\color{JungleGreen}{\Rrightarrow}$ So here is where the magic happens. At leading order the amplitudes can be written as:
+{\tiny{
+\eqa{
+\apeLR &=&\sqrt{2} N m_B(1- \hat s)\bigg[ (\Ceff9 + \Cpeff9) \mp (\C{10} + \Cp{10})
++\frac{2\hat{m}_b}{\hat s} (\Ceff7 + \Cpeff7) \bigg]\xi_{\bot}(E_{K^*}) \nn \\[2mm]
+\apaLR &=& -\sqrt{2} N m_B (1-\hat s)\bigg[(\Ceff9 - \Cpeff9) \mp (\C{10} - \Cp{10})
++\frac{2\hat{m}_b}{\hat s}(\Ceff7 - \Cpeff7) \bigg] \xi_{\bot}(E_{K^*}) \nn \\[2mm]
+\azeLR &=& -\frac{N m_B (1-\hat s)^2}{2 \hat{m}_{K^*} \sqrt{\hat s}} \bigg[ (\Ceff9 - \Cpeff9) \mp (\C{10} - \Cp{10}) + 2\hat{m}_b (\Ceff7 - \Cpeff7) \bigg]\xi_{\|}(E_{K^*}),
+\label{LargeRecoilAs}\nonumber}
+}}
+where $\hat s = q^2 /m_B^2$, $\hat{m}_i = m_i/m_B$. The $\xi_{\|,\bot }$ are the soft form factors. \\
+\pause
+$\color{JungleGreen}{\Rrightarrow}$ Now we can construct observables that cancel the $\xi$ soft form factors at leading order:
+\eq{P_5^{\prime} = \dfrac{J_5+\bar{J}_5}{2\sqrt{-(J_2^c+\bar{J}_2^c)(J_2^s+\bar{J}_2^s)} }\nonumber
+}
+
+
+\end{minipage}
+\vspace*{2.1cm}
+\end{frame}
+
+\iffalse
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{frame}{Theory implications 2}
+\begin{minipage}{\textwidth}
+
+{~}
+\ARROW If one includes recent measurements of $R_k$ and $R_{\PKstar}$:
+\begin{center}
+\includegraphics[width=0.99\textwidth]{images/quim1.png}
+\end{center}
+\begin{columns}
+\column{0.5\textwidth}
+\includegraphics[width=0.75\textwidth]{images/quim2.png}
+ \column{0.5\textwidth}
+\includegraphics[width=0.75\textwidth]{images/quim3.png}
+
+
+\end{columns}
+\ARROW Strong indications of NP!
+\end{minipage}
+\textref{arxiv::1704.05340}
+
+\vspace*{2.1cm}
+\end{frame}
+
+
+\fi
+
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\begin{frame}{Measurement of phase difference}
+\begin{minipage}{\textwidth}
+{~}
+\begin{columns}
+\column{0.6\textwidth}
+\ARROW One could try to measure the phase difference between the resonances and the nonresonant amplitudes to see if the interference is large enough to explain the effects.\\
+\ARROW Measured firstly done for the decay $\PB \to \PK \mu \mu$.\\
+\ARROW The analysis based:
+\begin{equation}
+C_9^{\rm eff} = C_9 +Y(q^2) = C_9 +\sum_j \eta_j e^{i \delta_i} A_j^{\rm res}(q^2)\nonumber
+\end{equation}
+\ARROW The amplitudes are modelled Briet-Wigner and Flatte functions.\\
+\ARROW Interference cannot explain the observed anomalies.
+
+
+
+
+
+\column{0.4\textwidth}
+\includegraphics[width=0.65\textwidth]{images/charm.png}\\
+\includegraphics[width=0.75\textwidth]{{images/hidef_finalplot_pos_neg}.png}\\\includegraphics[width=0.7\textwidth]{images/hidef_WilsonProfile.png}
+
+\end{columns}
+
+\end{minipage}
+
+\textref{Phys. Rev. D 95, 071101 (2017)}
+\vspace*{2.1cm}
+\end{frame}
+
+
+
+
+
+
+
+
+
+
+\backupend
+\end{document}
+
+
+
+
+
+
+
diff --git a/UK_VD/26.12.2022/mchrzasz2-blx.bib b/UK_VD/26.12.2022/mchrzasz2-blx.bib
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+++ b/UK_VD/26.12.2022/mchrzasz2-blx.bib
@@ -0,0 +1,11 @@
+@Comment{$ biblatex control file $}
+@Comment{$ biblatex version 2.3 $}
+Do not modify this file!
+
+This is an auxiliary file used by the 'biblatex' package.
+This file may safely be deleted. It will be recreated as
+required.
+
+@Control{biblatex-control,
+ options = {2.3:0:0:1:0:0:1:1:0:0:0:0:1:1:3:1:79:+},
+}
diff --git a/UK_VD/26.12.2022/mchrzasz2.synctex.gz b/UK_VD/26.12.2022/mchrzasz2.synctex.gz
new file mode 100644
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+++ b/UK_VD/26.12.2022/mchrzasz2.synctex.gz
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diff --git a/UK_VD/26.12.2022/tikzfeynman.sty b/UK_VD/26.12.2022/tikzfeynman.sty
new file mode 100755
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--- /dev/null
+++ b/UK_VD/26.12.2022/tikzfeynman.sty
@@ -0,0 +1,43 @@
+% Tikz Feynman Diagrams
+% by Flip Tanedo
+% 4 January 2011, work in progress
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+%%% TIKZ - for drawing Feynman diagrams %%%%
+%%% ... use with pdflatex %%%%
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+
+\usepackage{tikz}
+\usetikzlibrary{arrows,shapes}
+\usetikzlibrary{trees}
+\usetikzlibrary{matrix,arrows} % For commutative diagram
+ % http://www.felixl.de/commu.pdf
+\usetikzlibrary{positioning} % For "above of=" commands
+\usetikzlibrary{calc,through} % For coordinates
+\usetikzlibrary{decorations.pathreplacing} % For curly braces
+\usepackage[tikz]{bclogo} % For cute logo boxes
+\usepackage{pgffor} % For repeating patterns
+
+\usetikzlibrary{decorations.pathmorphing} % For Feynman Diagrams
+\usetikzlibrary{decorations.markings}
+\tikzset{
+ % >=stealth', %% Different kind of arrows
+ vector/.style={decorate, decoration={snake}, draw},
+ fermion/.style={postaction={decorate},
+ decoration={markings,mark=at position .55 with {\arrow{>}}}},
+ fermionbar/.style={draw, postaction={decorate},
+ decoration={markings,mark=at position .55 with {\arrow{<}}}},
+ fermionnoarrow/.style={},
+ gluon/.style={decorate,
+ decoration={coil,amplitude=4pt, segment length=5pt}},
+ scalar/.style={dashed, postaction={decorate},
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