diff --git a/SUSY_2015/RD/Makefile b/SUSY_2015/RD/Makefile new file mode 100644 index 0000000..e4cf8e8 --- /dev/null +++ b/SUSY_2015/RD/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/SUSY_2015/RD/beamercolorthemeFlip.sty b/SUSY_2015/RD/beamercolorthemeFlip.sty new file mode 100755 index 0000000..d6b9c50 --- /dev/null +++ b/SUSY_2015/RD/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/SUSY_2015/RD/beamerinnerthemeFlip.sty b/SUSY_2015/RD/beamerinnerthemeFlip.sty new file mode 100755 index 0000000..9910f4d --- /dev/null +++ b/SUSY_2015/RD/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/SUSY_2015/RD/beamerouterthemeFlip.sty b/SUSY_2015/RD/beamerouterthemeFlip.sty new file mode 100755 index 0000000..d12f6d6 --- /dev/null +++ b/SUSY_2015/RD/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/SUSY_2015/RD/beamerouterthemedecolines.sty b/SUSY_2015/RD/beamerouterthemedecolines.sty new file mode 100755 index 0000000..669e493 --- /dev/null +++ b/SUSY_2015/RD/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/SUSY_2015/RD/beamerthemeFlip.sty b/SUSY_2015/RD/beamerthemeFlip.sty new file mode 100755 index 0000000..a615ff5 --- /dev/null +++ b/SUSY_2015/RD/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 diff --git a/SUSY_2015/RD/images/.DS_Store b/SUSY_2015/RD/images/.DS_Store new file mode 100644 index 0000000..5008ddf --- /dev/null +++ b/SUSY_2015/RD/images/.DS_Store Binary files differ diff --git a/SUSY_2015/RD/images/A3Pad.pdf b/SUSY_2015/RD/images/A3Pad.pdf new file mode 100644 index 0000000..a70e975 --- /dev/null +++ b/SUSY_2015/RD/images/A3Pad.pdf Binary files differ diff 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when boldfaced +%% This is a hack to use Helvetica instead +%% Usage: \textbf{\forbold some stuff} +%\newcommand{\forbold}{\fontspec{Arial}} + +\usepackage{graphicx} +\usepackage[export]{adjustbox} + +\usepackage{amsmath} +\usepackage{amsfonts} +\usepackage{amssymb} +\usepackage{bm} +\usepackage{colortbl} +\usepackage{mathrsfs} % For Weinberg-esque letters +\usepackage{cancel} % For "SUSY-breaking" symbol +\usepackage{slashed} % for slashed characters in math mode +\usepackage{bbm} % for \mathbbm{1} (unit matrix) +\usepackage{amsthm} % For theorem environment +\usepackage{multirow} % For multi row cells in table +\usepackage{arydshln} % For dashed lines in arrays and tables +\usepackage{siunitx} +\usepackage{xhfill} +\usepackage{grffile} +\usepackage{textpos} +\usepackage{subfigure} +\usepackage{tikz} + +%\usepackage{hepparticles} +\usepackage[italic]{hepparticles} + +\usepackage{hepnicenames} + +% Drawing a line +\tikzstyle{lw} = [line width=20pt] +\newcommand{\topline}{% + \tikz[remember picture,overlay] {% + \draw[crimsonred] ([yshift=-23.5pt]current page.north west) + -- ([yshift=-23.5pt,xshift=\paperwidth]current page.north west);}} + + + +% % % % % % % % % % % % % % % % % % % % % % % % % % % % % % % % % % % +\usepackage{tikzfeynman} % For Feynman diagrams +\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 +% 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}{$#2$}}% +\newcommand{\thetal}{\theta_l} +\newcommand{\thetak}{\theta_k} + +\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{\im}{\rm{Im}} +\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{{\rm Br}} + + + +\author{ {\fontspec{Trebuchet MS}Marcin Chrz\k{a}szcz} (Universit\"{a}t Z\"{u}rich)} +\institute{UZH} +\title[Electroweak penguin decays to leptons and Radiative decays at LHCb]{Electroweak penguin decays to leptons and Radiative 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\fontspec{Trebuchet MS}\bfseries \LARGE {Electroweak penguin decays to leptons and Radiative decays at LHCb} + \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} {\fontspec{Trebuchet MS} \Large Marcin Chrząszcz\\\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}{Zurich meeting, CERN\\September 24, 2014} +\end{center} +\end{frame} +} + + +\section[Outline]{} +\begin{frame} +%\tableofcontents +%FIXME! +\begin{enumerate} +\item Rare $\PB$ decays: +\begin{itemize} +\item $\PB^+ \to \PK^+ \Ppi^- \Ppi^+ \Pphoton$ +\item $\PBs/\PBzero \to \mu^- \mu^+$. +\item $\PBzero \to \PKstar \Pmuon \APmuon$. +\end{itemize} + +\end{enumerate} + +\end{frame} + +%------------------------------------------------------------------- +% Introduction +%------------------------------------------------------------------- +% +% Set the background for the rest of the slides. +% Insert infoline +%\setbeamertemplate{background} +% {\includegraphics[width=\paperwidth,height=\paperheight]{slide_bg}} +%\setbeamertemplate{footline}[bunsentheme] + + + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% + +%\setbeamertemplate{background} +% {\includegraphics[width=\paperwidth,height=\paperheight]{slide_bg}} +%\setbeamertemplate{footline}[bunsentheme] +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%\section{LHCb detector} + +%\begin{frame}\frametitle{LHCb detector} +%\begin{columns} +%\column{3.in} +%\begin{center} +%\includegraphics[width=0.98\textwidth]{det.jpg} +%\end{center} + +%\column{2.0in} +%\begin{footnotesize} + + + % LHCb is a forward spectrometer: + % \begin{itemize} + % \item Excellent vertex resolution. + % \item Efficient trigger. + % \item High acceptance for $\Ptau$ and $\PB$. + % \item Great Particle ID + % \end{itemize} + + + +%\end{footnotesize} +%\end{columns} + +%\end{frame} + +\section{Introduction} + +\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]{susy/lupa.png} +\includegraphics[scale=0.3]{susy/example.png} +\end{center} +\column{1.5in} +\includegraphics[width=0.61\textwidth]{susy/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{3.2in} +\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*} + +\column{2in} +\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]{susy/all.png} + +\end{center} + + +\end{frame} + + + +\begin{frame}\frametitle{Radiative decays} + +\begin{columns} +\column{5in} + +\begin{itemize} +\item $\PBzero \to \PKstar \Pphoton$ - first observed penguin! +\begin{itemize} +\item CLEO, [\href{http://journals.aps.org/prl/abstract/10.1103/PhysRevLett.71.674}{\color{blue}PRL, 71 (1993) 674}] +\end{itemize} +\item B-factories probed NP measuring, inclusively/ semi-inclusively $\mathcal{B}(\Pbeauty \to \Pstrange \Pphoton)$ +\end{itemize} +\column{0.1in}{~} + +\end{columns} + + + +\begin{columns} +\column{3in} +\begin{itemize} +\item Is there any way LHCb can contribute? +\begin{itemize} +\item Measurements of $\mathcal{B}(\Pbeauty \to \Pstrange \Pphoton)$ very difficult. +\item Can probe the photon polarization! +\end{itemize} +\end{itemize} +\column{2in} +\includegraphics[width=0.85\textwidth]{susy/btosgamma.png} +\end{columns} +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%5 + + +\begin{columns} +\column{5in} + +\begin{itemize} +\item In SM, photons form $\Pbeauty \to \Pstrange \Pphoton$ decays are left handed. +\begin{itemize} +\item Charged current interactions: $C_7/C'_7\sim m_{\Pbeauty}/m_{\Pstrange}$ +\end{itemize} +\item Can test $C_7/C'_7$ using: +\begin{itemize} +\item Mixing induced CP violation: \href{http://arxiv.org/abs/hep-ph/9704272}{\color{blue}Atwood et. al. PRL 79 (1997) 185-188} +\item $\PLambdab$ baryons: \href{http://arxiv.org/abs/hep-ph/0108074}{\color{blue}Hiller \& kagan PRD 65 (2002) 074038} +\end{itemize} +\end{itemize} +\column{0.1in}{~} + +\end{columns} + +\end{frame} +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%5 + +\begin{frame}\frametitle{Photon polarization from $\PB^+ \to \PK^{+} \Ppi^- \Ppi^+ \Pphoton$} + + +\begin{columns} +\column{3.5in} + +\begin{itemize} +\item OR: Study $\PB \to \PK^{\ast \ast} \Pphoton$ decays like $\PBplus \to \PK_1(1270) \Pphoton$ +\begin{itemize} +\item \href{http://arxiv.org/abs/hep-ph/0205065}{\color{blue}Gronau \& Pirjol PRD 66 (2002) 054008} +\end{itemize} +\item The trick is to get the photon polarization from the up-down asymmetry of photon direction in the $\PK \Ppi \Ppi$ rest frame. +\begin{itemize} +\item No asymmetry $\rightarrow$ Unpolarised photons. +\end{itemize} +\item Conceptionally this measurement is similar to the Wu experiment, which first observed parity violation. + + +\end{itemize} +\column{1.5in} + +\includegraphics[width=0.95\textwidth]{susy/polarization.png} + +\end{columns} +\end{frame} +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}\frametitle{$\PB^+ \to \PK^{+} \Ppi^- \Ppi^+ \Pphoton$ at LHCb} + + +\begin{columns} +\column{3.in} + +\begin{itemize} +\item LHCb looked at $\PBplus \to \PKplus \Ppiminus \Ppiplus \Pphoton$, using un-converted photons. +\item Got over 13.000 candidates in $3~fb^{-1}$! +\item \href{http://journals.aps.org/prl/abstract/10.1103/PhysRevLett.112.161801}{\color{blue} Phys. Rev. Lett. 112, 161801 } +\item $\PKplus \Ppiminus \Ppiplus$ system has variety of resonances. +\begin{itemize} +\item $\PK \Ppi \Ppi$ system studied inclusively. +\item Bin the $m_{K\pi\pi}$ mass and look for polarization there. +\end{itemize} +\end{itemize} +\column{2in} +{~} +\includegraphics[width=0.95\textwidth]{susy/plotspolarization.png} + +\end{columns} +\end{frame} + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}%\frametitle{$\color{white} B^+ \to K^{+} \pi^- \pi^+ \gamma$ at LHCb} +\begin{center} +{\color{red} Fit with $\color{red}(C_7'-C_7)/(C_7'+C_7)=0$}, {\color{blue} Best fit} +\includegraphics[width=0.93\textwidth]{susy/photonfit.png} +\end{center} + + +\end{frame} + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}\frametitle{Up-down asymmetry} + +\begin{columns} +\column{3.in} + +\begin{itemize} +\item Combining the 4 bins, the hypothesis of non photon polarisation can be excluded with $5.2~\sigma$ significance. +\item Unfortunately without understanding the hadron system it is impossible to tell if the photon is left or right -handed. + +\end{itemize} + +\column{2in} +{~} +\includegraphics[width=0.95\textwidth]{susy/aud.png} + +\end{columns} +\begin{center} +$\rightarrow$~ First observation of photon polarization in $\Pbeauty \to \Pstrange \Pphoton$! +\begin{itemize} +\item Ideal solution would be to leave photon polarization free in the fit. +\item No general description exist $\rightarrow$ input from theory community needed. +\end{itemize} + + +\end{center} + + + +\end{frame} + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}\frametitle{$\PB_{(s)} \rightarrow \Pmu^+ \Pmu^-$} +\begin{columns} +\column{3.2in} + +\begin{itemize} +\item Clean theoretical prediction, GIM and helicity suppressed in the SM: +\begin{itemize} +\item $\mathcal{B}(\PBs \to \Pmuon \APmuon) = (3.66 \pm 0.23)\times 10^{-9}$ +\item $\mathcal{B}(\PBzero \to \Pmuon \APmuon) = (1.06 \pm 0.09)\times 10^{-10}$ +\end{itemize} +\item $50\%$ of the error comes from lattice. +\item SM predictions from \href{http://journals.aps.org/prl/abstract/10.1103/PhysRevLett.112.101801}{\color{blue}{Phys. Rev. Lett. 112, 101801 (2014)}}. +\item Sensitive to contributions from scalar and pesudoscalar couplings. +\item Probing: MSSM, higgs sector, etc. +\item In MSSM: $\mathcal{B}(\PBs \to \Pmuon \APmuon) \sim \tan^6 \beta /m_A^4$ +\end{itemize} + +\column{1.5in} +{~} +\includegraphics[width=0.95\textwidth]{susy/bs2mumu1.png}\\ +\includegraphics[width=0.95\textwidth]{susy/bs2mumu2.png}\\ +\includegraphics[width=0.6\textwidth]{susy/higgspen.png} +\end{columns} + + +\end{frame} +\iffalse +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}\frametitle{$\PB_{(s)} \rightarrow \Pmu^+ \Pmu^-$ searches} + + +\begin{columns} +\column{5in} + +\begin{itemize} +\item Background rejection power is a key feature of rare decays $\rightarrow$ use multivariate classifiers (BDT) and strong PID. +\end{itemize} +\column{0.1in}{~} + +\end{columns} +\begin{columns} +\column{2.5in} +\includegraphics[width=0.95\textwidth]{susy/BDT.png} + +\column{2.5in} + +\includegraphics[width=0.95\textwidth]{susy/mass.png} + +\end{columns} + +\begin{itemize} +\item Normalize the BF to $\PBplus \to \PJpsi(\mu\mu) \PKplus$ and $\PBzero \to \PK \Ppi$. +\end{itemize} +\end{frame} + +\fi +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}\frametitle{$\PB_{(s)} \rightarrow \Pmu^+ \Pmu^-$ Results} + + + +\begin{columns} +\column{2.in} +\begin{itemize} +\item Nov. 2012: +\begin{itemize} +\item First evidence $3.5\sigma$ for $\PB_s \rightarrow \mu^+ \mu^-$. with $2.1~fb^{-1}$. +\end{itemize} +\item Summer 2013: +\begin{itemize} +\item Full data sample: $3~fb^{-1}$. +\end{itemize} +\end{itemize} +\column{3.0in} + +\includegraphics[width=0.95\textwidth]{susy/mass2.png} + +\end{columns} +\begin{itemize} +\item Measured BF:\\ $\mathcal{B}(\PBs \to \Pmuon \APmuon) =(2.9^{+1.1}_{-1.0}(stat.)^{+0.3}_{-0.1}(syst.))\times 10^{-9}$ +\item $4.0 \sigma$ significance! +\item $\mathcal{B}(\PBzero \to \Pmuon \APmuon) < 7 \times 10^{-10}$ at $95\%$ CL +\item \href{http://journals.aps.org/prl/abstract/10.1103/PhysRevLett.110.021801}{\color{blue} PRL 110 (2013) 021801 } +\item \href{http://journals.aps.org/prl/abstract/10.1103/PhysRevLett.111.101805}{\color{blue} CMS result: PRL 111 (2013) 101805} +\end{itemize} + + +\end{frame} + + + + + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}\frametitle{LHCb+CMS combined analysis} +\begin{Large} + + +\begin{center} +$\mathcal{B}(\PBs \to \Pmuon \APmuon) =(2.8^{+0.7}_{-0.6} )\times 10^{-9}$\\ +$\mathcal{B}(\PBzero \to \Pmuon \APmuon) =(3.9^{+1.6}_{-1.4} )\times 10^{-10}$ +\end{center} +\end{Large} + +\includegraphics[width=0.95\textwidth]{susy/bs2mumu_comb.png} + +\begin{itemize} +\item \href{http://arxiv.org/pdf/1411.4413v1.pdf}{\color{blue}Nature 522, 7554} +%\item See Daniele Fasanella talk for CMS side. +\end{itemize} + +\end{frame} + + + + + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}\frametitle{$\PBzero \rightarrow \PK^{\ast} \Pmu \Pmu$ angular distributions} +\begin{columns} +\column{2.5in}{~} +\begin{itemize} +\item $\Pbeauty \to \Pstrange \Plepton \Plepton$ decays poses large spectrum of observables. +\item LHCb favourite: $\PBzero \to \PKstar \Pmuon \APmuon$. +\item Sensitive to lot of new physics models. +\item Decay described by three angles $\theta_l, \theta_K, \phi$ and dimuon invariant mass $q^2$. +\item Analysis is performed in bins of $q^2$. +\end{itemize} +\column{2.5in} +\includegraphics[width=0.95\textwidth]{susy/angles.png} + +\end{columns} +\end{frame} +\begin{frame}\frametitle{$\PBzero \rightarrow \PK^{\ast} \Pmu \Pmu$ selection} +\begin{center} +\includegraphics[width=0.65\textwidth]{images/Fig1.pdf} +\end{center} +\begin{itemize} +\item BDT to suppress combinatorial background.\\ Input variables: PID, kinematics and geometric quantities, isolations. +\item Veto the $\PJpsi$ and $\Psi(2S)$ resonances. +\item \href{http://lhcb.web.cern.ch/lhcb/Physics-Results/LHCb-CONF-2015-002.pdf}{\color{blue}{CONF-2015-002}} +\end{itemize} + + +\end{frame} +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}\frametitle{$\PBzero \rightarrow \PK^{\ast} \Pmu \Pmu$ mass modeling} +\only<1>{ +\begin{columns} +\column{0.05in} +{~} +\column{2.5in} +Control Channel: $\PBzero \to \PJpsi \PKstar$ +\includegraphics[angle=-90,width=0.85\textwidth]{images/Fig3a.pdf} +\column{2.5in} +Signal Channel: $\PBzero \to \Pmuon \APmuon \PKstar$ +\includegraphics[angle=-90,width=0.85\textwidth]{images/Fig3b.pdf} +\end{columns} +\begin{itemize} +\item Signal mass model from high statistics $\PBzero \to \PJpsi \PKstar$. +\item Correction factor from simulation to account for $q^2$ dep. resolution. +\end{itemize} +} +\only<2>{ +\begin{center} +\includegraphics[angle=-90,width=0.25\textwidth]{susy/m0.pdf} +\includegraphics[angle=-90,width=0.25\textwidth]{susy/m1.pdf} +\includegraphics[angle=-90,width=0.25\textwidth]{susy/m2.pdf} +\includegraphics[angle=-90,width=0.25\textwidth]{susy/m3.pdf}\\ +\includegraphics[angle=-90,width=0.25\textwidth]{susy/m4.pdf} +\includegraphics[angle=-90,width=0.25\textwidth]{susy/m5.pdf} +\includegraphics[angle=-90,width=0.25\textwidth]{susy/m6.pdf} +\includegraphics[angle=-90,width=0.25\textwidth]{susy/m7.pdf} +\end{center} +} +\begin{itemize} +\item Finer $q^2$ binning allow more flexible usage for theoriets. +\item Significant signal yield in all bins! +\item Integrated over all bins we have $2398\pm57$ candidates. +\end{itemize} + +\end{frame} + + + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}\frametitle{$\PBzero \rightarrow \PK^{\ast} \Pmu \Pmu$ angular distributions} +\begin{itemize} +\item Angular distributions depends on 11 angular terms: +%\includegraphics[width=0.95\textwidth]{susy/eq.png} +\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 \\[-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{itemize} +where the $S_i$ are bilinear combinations of helicity amplitudes. +\begin{itemize} +\item We assume no scalar and tensor contribution and massless leptons. +\end{itemize} + +\end{frame} +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}\frametitle{S-wave pollution} +\begin{itemize} +\item S-wave: $\PK^+ \Ppi^-$ in spin $0$ configuration +\item Introduced by additional two decay amplitudes $\rightarrow$ six observables. +\end{itemize} +{\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 S}+{\rm P}} = +(1-F_S)&\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}\label{eq:pdfswave}\\ ++\tfrac{3}{16\pi} &\bigl[F_S \sin^2\thetal + S-P~\rm{interefence} \bigr].\nonumber +\end{align*} +}} +\begin{columns} +\column{2.5in} +\begin{itemize} +\item $F_S$ dilutes the P-wave observables by a factor $1-F_S$. +\item Needs to be taken into account \\ $\rightarrow$ fit the $m_{K\pi}$. +\item Rel. BW for P-wave. +\item LASS model for S-wave\\{~}\\{~}\\{~} +\end{itemize} +\column{2in} +\includegraphics[angle=-90,width=0.85\textwidth]{images/mkpi4sig.pdf} + +\end{columns} + + +\end{frame} + + + + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%5 +\begin{frame}\frametitle{$\PBzero \rightarrow \PK^{\ast} \Pmu \Pmu$ results} +\begin{columns} +\column{2.5in} +\includegraphics[angle=-90,width=0.95\textwidth]{images/Fig5a.pdf}\\ +\includegraphics[angle=-90,width=0.95\textwidth]{images/Fig5c.pdf} +\column{2.5in} +\includegraphics[angle=-90,width=0.95\textwidth]{images/Fig5b.pdf}\\ +\includegraphics[angle=-90,width=0.95\textwidth]{images/Fig5d.pdf} +\end{columns} +\end{frame} + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%5 +\begin{frame}\frametitle{$\PBzero \rightarrow \PK^{\ast} \Pmu \Pmu$ results} +\begin{center} +\includegraphics[angle=-90,width=0.65\textwidth]{images/Fig17.pdf}\\ +\end{center} +\begin{itemize} +\item Tension in $P_5^{\prime}$ confirmed! +\item $[4.0,6.0]$ and $[6.0, 8.0]~\GeV^2/c^4$ show $2.9 \sigma$ deviation each. +\item Naive combination shows $3.7\sigma$ discrepancy. +\item Result compatible with previous result. +\end{itemize} + + +\end{frame} + + + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}\frametitle{Understanding the $\PBzero \rightarrow \PK^{\ast} \Pmu \Pmu$ anomaly} +\begin{columns} +\column{3.in} +\begin{itemize} +\item Matias, Decotes-Genon \& Virto performed a fit to our preliminary result.s +\item Found $\sim 4 \sigma$ discrepancy from SM. +\item Fit favours $C_9^{NP}=-1.1$ +\item \href{https://indico.in2p3.fr/event/10819/session/10/contribution/14/material/slides/0.pdf}{\color{Blue}{Moriond 2015 slides}} +\end{itemize} +\begin{itemize} +\item Straub performed the same analysis as Matias et. al. +\item Found the same solution:\\ $\rightarrow$ $C_9$ modification. +\item Data can be explained by introducing a flavour changing $\PZprime$ boson, with mass $\mathcal{O}(10~TeV)$ +\item \href{https://indico.in2p3.fr/event/10819/session/10/contribution/87/material/slides/0.pdf}{\color{blue}{Moriond 2015 slides}} +\end{itemize} + +\column{2.in} +\includegraphics[width=0.95\textwidth]{images/quim.png}\\ +\includegraphics[width=0.95\textwidth]{images/straub.png} +\end{columns} +\end{frame} +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%\begin{frame}\frametitle{Understanding the $\color{white}B^{0} \rightarrow K^{\ast} \mu \mu$ anomaly 2/2} +%\begin{columns} +%\column{3in} + +%\includegraphics[width=0.99\textwidth]{susy/c9.png} +%\column{2in} +%\begin{itemize} +%\item High $q^2$ differential BF suggests are all below SM. +%\item Better consistency with $C_9^{NP}=-1.5$ +%\end{itemize} + +%\end{columns} + + +%\end{frame} + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}\frametitle{Lepton universality} +\begin{columns} +\column{3.0in} +\begin{itemize} +\item If $\PZprime$ is responsible for the $P'_5$ anomaly, does it couple equally to all flavours? +\includegraphics[width=0.9\textwidth]{susy/uni2.png} +\item Challenging analysis due to bremsstrahlung. +\item Migration of events modeled by MC. +\item Correct bremsstrahlung. +\item Take double ratio with $\PBplus \to \PJpsi \PKplus$ to cancel systematics. +\item In $3fb^{-1}$, LHCb measures $R_K=0.745^{+0.090}_{-0.074}(stat.)^{+0.036}_{-0.036}(syst.)$ +\item Consistent with SM at $2.6\sigma$. + +\end{itemize} +\column{2.0in} +\includegraphics[width=0.99\textwidth]{images/RK.png}\\ +\begin{itemize} +\item \href{http://arxiv.org/abs/1406.6482}{Phys. Rev. Lett. 113, 151601 (2014)} +\end{itemize} +\end{columns} +\end{frame} +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}\frametitle{Lepton universality with $\PBzero \rightarrow \PK^{\ast} \Pmu \Pmu$ anomaly} +\begin{columns} +\column{3in} +\begin{itemize} +\item Lepton flavour universality cannot be explained by any QCD effect! +\item This effect is consistent with anomaly (non universal $\PZ'$) +\item Global fit to $\Pbeauty \rightarrow \Pstrange \Pmuon \APmuon$ and $\Pbeauty \rightarrow \Pstrange \Pelectron \APelectron$ seems to favour $\PZ'$ with non lepton universal couplings. +\end{itemize} + + +\column{2in} +\includegraphics[width=0.9\textwidth]{images/LU.png} +\end{columns} +\href{http://arxiv.org/pdf/1408.4097v3.pdf}{\color{blue}{JHEP (2014) 131}} +\end{frame} + + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}\frametitle{Conclusions} +\begin{columns} +\column{3.3in} +\begin{itemize} +\item Rare decays play important role in hutting NP. +\item Can access NP scales beyond reach of GPD. +\item Tension in $\Pbeauty \to \Pstrange \Plepton \Plepton$, theory correct? +\item List of decays presented in this talk is just a tip of iceberg: +\begin{itemize} +\item Please look at ours: isospin, $A_{CP}$. +\item More results are on their way. +\end{itemize} +\item Many results really on SM prediction, QCD improved calculations would be highly appreciated. + +\end{itemize} +\column{2in} +\includegraphics[width=0.9\textwidth]{susy/higgs_boring.png} +\end{columns} + +\end{frame} + + + +\backupbegin + +\begin{frame}\frametitle{Backup} +\topline + +\end{frame} + +\backupend + +\end{document} diff --git a/SUSY_2015/RD/mchrzasz.tex~ b/SUSY_2015/RD/mchrzasz.tex~ new file mode 100644 index 0000000..0a59116 --- /dev/null +++ b/SUSY_2015/RD/mchrzasz.tex~ @@ -0,0 +1,889 @@ +\documentclass[11 pt,xcolor={dvipsnames,svgnames,x11names,table}]{beamer} + +\usepackage[english]{babel} +\usepackage{polski} + + +\usetheme[ + bullet=circle, % Other option: square + bigpagenumber, % circled page number on lower right + topline=true, % colored bar at the top of the frame + shadow=false, % Shading for beamer blocks + watermark=BG_lower, % png file for the watermark + ]{Flip} + +%\logo{\kern+1.em\includegraphics[height=1cm]{SHiP-3_LightCharcoal}} + + +\usepackage[lf]{berenis} +\usepackage[LY1]{fontenc} +\usepackage[utf8]{inputenc} + +\usepackage{emerald} +\usefonttheme{professionalfonts} +\usepackage[no-math]{fontspec} +\defaultfontfeatures{Mapping=tex-text} % This seems to be important for mapping glyphs properly + +\setmainfont{Gillius ADF} % Beamer ignores "main font" in favor of sans font +\setsansfont{Gillius ADF} % This is the font that beamer will use by default +% \setmainfont{Gill Sans Light} % Prettier, but harder to read + +\setbeamerfont{title}{family=\fontspec{Gillius ADF}} + +\input t1augie.fd + +%\newcommand{\handwriting}{\fontspec{augie}} % From Emerald City, free font +%\newcommand{\handwriting}{\usefont{T1}{fau}{m}{n}} % From Emerald City, free font +% \newcommand{\handwriting}{} % If you prefer no special handwriting font or don't have augie + +%% Gill Sans doesn't look very nice when boldfaced +%% This is a hack to use Helvetica instead +%% Usage: \textbf{\forbold some stuff} +%\newcommand{\forbold}{\fontspec{Arial}} + +\usepackage{graphicx} +\usepackage[export]{adjustbox} + +\usepackage{amsmath} +\usepackage{amsfonts} +\usepackage{amssymb} +\usepackage{bm} +\usepackage{colortbl} +\usepackage{mathrsfs} % For Weinberg-esque letters +\usepackage{cancel} % For "SUSY-breaking" symbol +\usepackage{slashed} % for slashed characters in math mode +\usepackage{bbm} % for \mathbbm{1} (unit matrix) +\usepackage{amsthm} % For theorem environment +\usepackage{multirow} % For multi row cells in table +\usepackage{arydshln} % For dashed lines in arrays and tables +\usepackage{siunitx} +\usepackage{xhfill} +\usepackage{grffile} +\usepackage{textpos} +\usepackage{subfigure} +\usepackage{tikz} + +%\usepackage{hepparticles} +\usepackage[italic]{hepparticles} + +\usepackage{hepnicenames} + +% Drawing a line +\tikzstyle{lw} = [line width=20pt] +\newcommand{\topline}{% + \tikz[remember picture,overlay] {% + \draw[crimsonred] ([yshift=-23.5pt]current page.north west) + -- ([yshift=-23.5pt,xshift=\paperwidth]current page.north west);}} + + + +% % % % % % % % % % % % % % % % % % % % % % % % % % % % % % % % % % % +\usepackage{tikzfeynman} % For Feynman diagrams +\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 +% 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]{<}}}}, + 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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}{$#2$}}% +\newcommand{\thetal}{\theta_l} +\newcommand{\thetak}{\theta_k} + +\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{\im}{\rm{Im}} +\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{{\rm Br}} + + + +\author{ {\fontspec{Trebuchet MS}Marcin Chrz\k{a}szcz} (Universit\"{a}t Z\"{u}rich)} +\institute{UZH} +\title[Electroweak penguin decays to leptons and Radiative decays at LHCb]{Electroweak penguin decays to leptons and Radiative 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\fontspec{Trebuchet MS}\bfseries \LARGE {Electroweak penguin decays to leptons and Radiative decays at LHCb} + \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} {\fontspec{Trebuchet MS} \Large Marcin Chrząszcz\\\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}{Zurich meeting, CERN\\September 24, 2014} +\end{center} +\end{frame} +} + + +\section[Outline]{} +\begin{frame} +%\tableofcontents +%FIXME! +\begin{enumerate} +\item Rare $\PB$ decays: +\begin{itemize} +\item $\PB^+ \to \PK^+ \Ppi^- \Ppi^+ \Pphoton$ +\item $\PBs/\PBzero \to \mu^- \mu^+$. +\item $\PBzero \to \PKstar \Pmuon \APmuon$. +\end{itemize} + +\end{enumerate} + +\end{frame} + +%------------------------------------------------------------------- +% Introduction +%------------------------------------------------------------------- +% +% Set the background for the rest of the slides. +% Insert infoline +%\setbeamertemplate{background} +% {\includegraphics[width=\paperwidth,height=\paperheight]{slide_bg}} +%\setbeamertemplate{footline}[bunsentheme] + + + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% + +%\setbeamertemplate{background} +% {\includegraphics[width=\paperwidth,height=\paperheight]{slide_bg}} +%\setbeamertemplate{footline}[bunsentheme] +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%\section{LHCb detector} + +%\begin{frame}\frametitle{LHCb detector} +%\begin{columns} +%\column{3.in} +%\begin{center} +%\includegraphics[width=0.98\textwidth]{det.jpg} +%\end{center} + +%\column{2.0in} +%\begin{footnotesize} + + + % LHCb is a forward spectrometer: + % \begin{itemize} + % \item Excellent vertex resolution. + % \item Efficient trigger. + % \item High acceptance for $\Ptau$ and $\PB$. + % \item Great Particle ID + % \end{itemize} + + + +%\end{footnotesize} +%\end{columns} + +%\end{frame} + +\section{Introduction} + +\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]{susy/lupa.png} +\includegraphics[scale=0.3]{susy/example.png} +\end{center} +\column{1.5in} +\includegraphics[width=0.61\textwidth]{susy/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{3.2in} +\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*} + +\column{2in} +\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]{susy/all.png} + +\end{center} + + +\end{frame} + + + +\begin{frame}\frametitle{Radiative decays} + +\begin{columns} +\column{5in} + +\begin{itemize} +\item $\PBzero \to \PKstar \Pphoton$ - first observed penguin! +\begin{itemize} +\item CLEO, [\href{http://journals.aps.org/prl/abstract/10.1103/PhysRevLett.71.674}{\color{blue}PRL, 71 (1993) 674}] +\end{itemize} +\item B-factories probed NP measuring, inclusively/ semi-inclusively $\mathcal{B}(\Pbeauty \to \Pstrange \Pphoton)$ +\end{itemize} +\column{0.1in}{~} + +\end{columns} + + + +\begin{columns} +\column{3in} +\begin{itemize} +\item Is there any way LHCb can contribute? +\begin{itemize} +\item Measurements of $\mathcal{B}(\Pbeauty \to \Pstrange \Pphoton)$ very difficult. +\item Can probe the photon polarization! +\end{itemize} +\end{itemize} +\column{2in} +\includegraphics[width=0.85\textwidth]{susy/btosgamma.png} +\end{columns} +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%5 + + +\begin{columns} +\column{5in} + +\begin{itemize} +\item In SM, photons form $\Pbeauty \to \Pstrange \Pphoton$ decays are left handed. +\begin{itemize} +\item Charged current interactions: $C_7/C'_7\sim m_{\Pbeauty}/m_{\Pstrange}$ +\end{itemize} +\item Can test $C_7/C'_7$ using: +\begin{itemize} +\item Mixing induced CP violation: \href{http://arxiv.org/abs/hep-ph/9704272}{\color{blue}Atwood et. al. PRL 79 (1997) 185-188} +\item $\PLambdab$ baryons: \href{http://arxiv.org/abs/hep-ph/0108074}{\color{blue}Hiller \& kagan PRD 65 (2002) 074038} +\end{itemize} +\end{itemize} +\column{0.1in}{~} + +\end{columns} + +\end{frame} +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%5 + +\begin{frame}\frametitle{Photon polarization from $\PB^+ \to \PK^{+} \Ppi^- \Ppi^+ \Pphoton$} + + +\begin{columns} +\column{3.5in} + +\begin{itemize} +\item OR: Study $\PB \to \PK^{\ast \ast} \Pphoton$ decays like $\PBplus \to \PK_1(1270) \Pphoton$ +\begin{itemize} +\item \href{http://arxiv.org/abs/hep-ph/0205065}{\color{blue}Gronau \& Pirjol PRD 66 (2002) 054008} +\end{itemize} +\item The trick is to get the photon polarization from the up-down asymmetry of photon direction in the $\PK \Ppi \Ppi$ rest frame. +\begin{itemize} +\item No asymmetry $\rightarrow$ Unpolarised photons. +\end{itemize} +\item Conceptionally this measurement is similar to the Wu experiment, which first observed parity violation. + + +\end{itemize} +\column{1.5in} + +\includegraphics[width=0.95\textwidth]{susy/polarization.png} + +\end{columns} +\end{frame} +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}\frametitle{$\PB^+ \to \PK^{+} \Ppi^- \Ppi^+ \Pphoton$ at LHCb} + + +\begin{columns} +\column{3.in} + +\begin{itemize} +\item LHCb looked at $\PBplus \to \PKplus \Ppiminus \Ppiplus \Pphoton$, using un-converted photons. +\item Got over 13.000 candidates in $3~fb^{-1}$! +\item \href{http://journals.aps.org/prl/abstract/10.1103/PhysRevLett.112.161801}{\color{blue} Phys. Rev. Lett. 112, 161801 } +\item $\PKplus \Ppiminus \Ppiplus$ system has variety of resonances. +\begin{itemize} +\item $\PK \Ppi \Ppi$ system studied inclusively. +\item Bin the $m_{K\pi\pi}$ mass and look for polarization there. +\end{itemize} +\end{itemize} +\column{2in} +{~} +\includegraphics[width=0.95\textwidth]{susy/plotspolarization.png} + +\end{columns} +\end{frame} + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}%\frametitle{$\color{white} B^+ \to K^{+} \pi^- \pi^+ \gamma$ at LHCb} +\begin{center} +{\color{red} Fit with $\color{red}(C_7'-C_7)/(C_7'+C_7)=0$}, {\color{blue} Best fit} +\includegraphics[width=0.93\textwidth]{susy/photonfit.png} +\end{center} + + +\end{frame} + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}\frametitle{Up-down asymmetry} + +\begin{columns} +\column{3.in} + +\begin{itemize} +\item Combining the 4 bins, the hypothesis of non photon polarisation can be excluded with $5.2~\sigma$ significance. +\item Unfortunately without understanding the hadron system it is impossible to tell if the photon is left or right -handed. + +\end{itemize} + +\column{2in} +{~} +\includegraphics[width=0.95\textwidth]{susy/aud.png} + +\end{columns} +\begin{center} +$\rightarrow$~ First observation of photon polarization in $\Pbeauty \to \Pstrange \Pphoton$! +\begin{itemize} +\item Ideal solution would be to leave photon polarization free in the fit. +\item No general description exist $\rightarrow$ input from theory community needed. +\end{itemize} + + +\end{center} + + + +\end{frame} + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}\frametitle{$\PB_{(s)} \rightarrow \Pmu^+ \Pmu^-$} +\begin{columns} +\column{3.2in} + +\begin{itemize} +\item Clean theoretical prediction, GIM and helicity suppressed in the SM: +\begin{itemize} +\item $\mathcal{B}(\PBs \to \Pmuon \APmuon) = (3.66 \pm 0.23)\times 10^{-9}$ +\item $\mathcal{B}(\PBzero \to \Pmuon \APmuon) = (1.06 \pm 0.09)\times 10^{-10}$ +\end{itemize} +\item $50\%$ of the error comes from lattice. +\item SM predictions from \href{http://journals.aps.org/prl/abstract/10.1103/PhysRevLett.112.101801}{\color{blue}{Phys. Rev. Lett. 112, 101801 (2014)}}. +\item Sensitive to contributions from scalar and pesudoscalar couplings. +\item Probing: MSSM, higgs sector, etc. +\item In MSSM: $\mathcal{B}(\PBs \to \Pmuon \APmuon) \sim \tan^6 \beta /m_A^4$ +\end{itemize} + +\column{1.5in} +{~} +\includegraphics[width=0.95\textwidth]{susy/bs2mumu1.png}\\ +\includegraphics[width=0.95\textwidth]{susy/bs2mumu2.png}\\ +\includegraphics[width=0.6\textwidth]{susy/higgspen.png} +\end{columns} + + +\end{frame} +\iffalse +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}\frametitle{$\PB_{(s)} \rightarrow \Pmu^+ \Pmu^-$ searches} + + +\begin{columns} +\column{5in} + +\begin{itemize} +\item Background rejection power is a key feature of rare decays $\rightarrow$ use multivariate classifiers (BDT) and strong PID. +\end{itemize} +\column{0.1in}{~} + +\end{columns} +\begin{columns} +\column{2.5in} +\includegraphics[width=0.95\textwidth]{susy/BDT.png} + +\column{2.5in} + +\includegraphics[width=0.95\textwidth]{susy/mass.png} + +\end{columns} + +\begin{itemize} +\item Normalize the BF to $\PBplus \to \PJpsi(\mu\mu) \PKplus$ and $\PBzero \to \PK \Ppi$. +\end{itemize} +\end{frame} + +\fi +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}\frametitle{$\PB_{(s)} \rightarrow \Pmu^+ \Pmu^-$ Results} + + + +\begin{columns} +\column{2.in} +\begin{itemize} +\item Nov. 2012: +\begin{itemize} +\item First evidence $3.5\sigma$ for $\PB_s \rightarrow \mu^+ \mu^-$. with $2.1~fb^{-1}$. +\end{itemize} +\item Summer 2013: +\begin{itemize} +\item Full data sample: $3~fb^{-1}$. +\end{itemize} +\end{itemize} +\column{3.0in} + +\includegraphics[width=0.95\textwidth]{susy/mass2.png} + +\end{columns} +\begin{itemize} +\item Measured BF:\\ $\mathcal{B}(\PBs \to \Pmuon \APmuon) =(2.9^{+1.1}_{-1.0}(stat.)^{+0.3}_{-0.1}(syst.))\times 10^{-9}$ +\item $4.0 \sigma$ significance! +\item $\mathcal{B}(\PBzero \to \Pmuon \APmuon) < 7 \times 10^{-10}$ at $95\%$ CL +\item \href{http://journals.aps.org/prl/abstract/10.1103/PhysRevLett.110.021801}{\color{blue} PRL 110 (2013) 021801 } +\item \href{http://journals.aps.org/prl/abstract/10.1103/PhysRevLett.111.101805}{\color{blue} CMS result: PRL 111 (2013) 101805} +\end{itemize} + + +\end{frame} + + + + + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}\frametitle{LHCb+CMS combined analysis} +\begin{Large} + + +\begin{center} +$\mathcal{B}(\PBs \to \Pmuon \APmuon) =(2.8^{+0.7}_{-0.6} )\times 10^{-9}$\\ +$\mathcal{B}(\PBzero \to \Pmuon \APmuon) =(3.9^{+1.6}_{-1.4} )\times 10^{-10}$ +\end{center} +\end{Large} + +\includegraphics[width=0.95\textwidth]{susy/bs2mumu_comb.png} + +\begin{itemize} +\item \href{http://arxiv.org/pdf/1411.4413v1.pdf}{\color{blue}Nature 522, 7554} +%\item See Daniele Fasanella talk for CMS side. +\end{itemize} + +\end{frame} + + + + + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}\frametitle{$\PBzero \rightarrow \PK^{\ast} \Pmu \Pmu$ angular distributions} +\begin{columns} +\column{2.5in}{~} +\begin{itemize} +\item $\Pbeauty \to \Pstrange \Plepton \Plepton$ decays poses large spectrum of observables. +\item LHCb favourite: $\PBzero \to \PKstar \Pmuon \APmuon$. +\item Sensitive to lot of new physics models. +\item Decay described by three angles $\theta_l, \theta_K, \phi$ and dimuon invariant mass $q^2$. +\item Analysis is performed in bins of $q^2$. +\end{itemize} +\column{2.5in} +\includegraphics[width=0.95\textwidth]{susy/angles.png} + +\end{columns} +\end{frame} +\begin{frame}\frametitle{$\PBzero \rightarrow \PK^{\ast} \Pmu \Pmu$ selection} +\begin{center} +\includegraphics[width=0.65\textwidth]{images/Fig1.pdf} +\end{center} +\begin{itemize} +\item BDT to suppress combinatorial background.\\ Input variables: PID, kinematics and geometric quantities, isolations. +\item Veto the $\PJpsi$ and $\Psi(2S)$ resonances. +\item \href{http://lhcb.web.cern.ch/lhcb/Physics-Results/LHCb-CONF-2015-002.pdf}{\color{blue}{CONF-2015-002}} +\end{itemize} + + +\end{frame} +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}\frametitle{$\PBzero \rightarrow \PK^{\ast} \Pmu \Pmu$ mass modeling} +\begin{columns} +\column{0.05in} +{~} +\column{2.5in} + +\column{2.5in} + +\end{columns} + + + +\end{frame} + + + + + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}\frametitle{$\PBzero \rightarrow \PK^{\ast} \Pmu \Pmu$ angular distributions} +\begin{itemize} +\item Angular distributions depends on 11 angular terms: +%\includegraphics[width=0.95\textwidth]{susy/eq.png} +\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 \\[-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{itemize} +where the $S_i$ are bilinear combinations of helicity amplitudes. +\begin{itemize} +\item We assume no scalar and tensor contribution and massless leptons. +\end{itemize} + +\end{frame} +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}\frametitle{S-wave pollution} +\begin{itemize} +\item S-wave: $\PK^+ \Ppi^-$ in spin $0$ configuration +\item Introduced by additional two decay amplitudes $\rightarrow$ six observables. +\end{itemize} +{\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 S}+{\rm P}} = +(1-F_S)&\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}\label{eq:pdfswave}\\ ++\tfrac{3}{16\pi} &\bigl[F_S \sin^2\thetal + S-P~\rm{interefence} \bigr].\nonumber +\end{align*} +}} +\begin{columns} +\column{2.5in} +\begin{itemize} +\item $F_S$ dilutes the P-wave observables by a factor $1-F_S$. +\item Needs to be taken into account \\ $\rightarrow$ fit the $m_{K\pi}$. +\item Rel. BW for P-wave. +\item LASS model for S-wave\\{~}\\{~}\\{~} +\end{itemize} +\column{2in} +\includegraphics[angle=-90,width=0.85\textwidth]{images/mkpi4sig.pdf} + +\end{columns} + + +\end{frame} + + + + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%5 +\begin{frame}\frametitle{$\PBzero \rightarrow \PK^{\ast} \Pmu \Pmu$ results} +\begin{columns} +\column{2.5in} +\includegraphics[angle=-90,width=0.95\textwidth]{images/Fig5a.pdf}\\ +\includegraphics[angle=-90,width=0.95\textwidth]{images/Fig5c.pdf} +\column{2.5in} +\includegraphics[angle=-90,width=0.95\textwidth]{images/Fig5b.pdf}\\ +\includegraphics[angle=-90,width=0.95\textwidth]{images/Fig5d.pdf} +\end{columns} +\end{frame} + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%5 +\begin{frame}\frametitle{$\PBzero \rightarrow \PK^{\ast} \Pmu \Pmu$ results} +\begin{center} +\includegraphics[angle=-90,width=0.65\textwidth]{images/Fig17.pdf}\\ +\end{center} +\begin{itemize} +\item Tension in $P_5^{\prime}$ confirmed! +\item $[4.0,6.0]$ and $[6.0, 8.0]~\GeV^2/c^4$ show $2.9 \sigma$ deviation each. +\item Naive combination shows $3.7\sigma$ discrepancy. +\item Result compatible with previous result. +\end{itemize} + + +\end{frame} + + + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}\frametitle{Understanding the $\PBzero \rightarrow \PK^{\ast} \Pmu \Pmu$ anomaly} +\begin{columns} +\column{3.in} +\begin{itemize} +\item Matias, Decotes-Genon \& Virto performed a fit to our preliminary result.s +\item Found $\sim 4 \sigma$ discrepancy from SM. +\item Fit favours $C_9^{NP}=-1.1$ +\item \href{https://indico.in2p3.fr/event/10819/session/10/contribution/14/material/slides/0.pdf}{\color{Blue}{Moriond 2015 slides}} +\end{itemize} +\begin{itemize} +\item Straub performed the same analysis as Matias et. al. +\item Found the same solution:\\ $\rightarrow$ $C_9$ modification. +\item Data can be explained by introducing a flavour changing $\PZprime$ boson, with mass $\mathcal{O}(10~TeV)$ +\item \href{https://indico.in2p3.fr/event/10819/session/10/contribution/87/material/slides/0.pdf}{\color{blue}{Moriond 2015 slides}} +\end{itemize} + +\column{2.in} +\includegraphics[width=0.95\textwidth]{images/quim.png}\\ +\includegraphics[width=0.95\textwidth]{images/straub.png} +\end{columns} +\end{frame} +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%\begin{frame}\frametitle{Understanding the $\color{white}B^{0} \rightarrow K^{\ast} \mu \mu$ anomaly 2/2} +%\begin{columns} +%\column{3in} + +%\includegraphics[width=0.99\textwidth]{susy/c9.png} +%\column{2in} +%\begin{itemize} +%\item High $q^2$ differential BF suggests are all below SM. +%\item Better consistency with $C_9^{NP}=-1.5$ +%\end{itemize} + +%\end{columns} + + +%\end{frame} + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}\frametitle{Lepton universality} +\begin{columns} +\column{3.0in} +\begin{itemize} +\item If $\PZprime$ is responsible for the $P'_5$ anomaly, does it couple equally to all flavours? +\includegraphics[width=0.9\textwidth]{susy/uni2.png} +\item Challenging analysis due to bremsstrahlung. +\item Migration of events modeled by MC. +\item Correct bremsstrahlung. +\item Take double ratio with $\PBplus \to \PJpsi \PKplus$ to cancel systematics. +\item In $3fb^{-1}$, LHCb measures $R_K=0.745^{+0.090}_{-0.074}(stat.)^{+0.036}_{-0.036}(syst.)$ +\item Consistent with SM at $2.6\sigma$. + +\end{itemize} +\column{2.0in} +\includegraphics[width=0.99\textwidth]{images/RK.png}\\ +\begin{itemize} +\item \href{http://arxiv.org/abs/1406.6482}{Phys. Rev. Lett. 113, 151601 (2014)} +\end{itemize} +\end{columns} +\end{frame} +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}\frametitle{Lepton universality with $\PBzero \rightarrow \PK^{\ast} \Pmu \Pmu$ anomaly} +\begin{columns} +\column{3in} +\begin{itemize} +\item Lepton flavour universality cannot be explained by any QCD effect! +\item This effect is consistent with anomaly (non universal $\PZ'$) +\item Global fit to $\Pbeauty \rightarrow \Pstrange \Pmuon \APmuon$ and $\Pbeauty \rightarrow \Pstrange \Pelectron \APelectron$ seems to favour $\PZ'$ with non lepton universal couplings. +\end{itemize} + + +\column{2in} +\includegraphics[width=0.9\textwidth]{images/LU.png} +\end{columns} +\href{http://arxiv.org/pdf/1408.4097v3.pdf}{\color{blue}{JHEP (2014) 131}} +\end{frame} + + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\begin{frame}\frametitle{Conclusions} +\begin{columns} +\column{3.3in} +\begin{itemize} +\item Rare decays play important role in hutting NP. +\item Can access NP scales beyond reach of GPD. +\item Tension in $\Pbeauty \to \Pstrange \Plepton \Plepton$, theory correct? +\item List of decays presented in this talk is just a tip of iceberg: +\begin{itemize} +\item Please look at ours: isospin, $A_{CP}$. +\item More results are on their way. +\end{itemize} +\item Many results really on SM prediction, QCD improved calculations would be highly appreciated. + +\end{itemize} +\column{2in} +\includegraphics[width=0.9\textwidth]{susy/higgs_boring.png} +\end{columns} + +\end{frame} + + + +\backupbegin + +\begin{frame}\frametitle{Backup} +\topline + +\end{frame} + +\backupend + +\end{document} diff --git a/SUSY_2015/RD/mchrzasz.toc b/SUSY_2015/RD/mchrzasz.toc new file mode 100644 index 0000000..3f1749c --- /dev/null +++ b/SUSY_2015/RD/mchrzasz.toc @@ -0,0 +1,6 @@ +\boolfalse {citerequest}\boolfalse {citetracker}\boolfalse {pagetracker}\boolfalse {backtracker}\relax +\defcounter {refsection}{0}\relax 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%%%% +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% + +\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}, + decoration={markings,mark=at position .55 with {\arrow{>}}}}, + scalarbar/.style={dashed, postaction={decorate}, + decoration={markings,mark=at position .55 with {\arrow{<}}}}, + scalarnoarrow/.style={dashed,draw}, +% +%% Special vectors (when you need to fine-tune wiggles) + provector/.style={decorate, decoration={snake,amplitude=2.5pt}, draw}, + antivector/.style={decorate, decoration={snake,amplitude=-2.5pt}, draw}, +} +