\documentclass[showdate=true]{beamer} \usetheme{Antibes} \usepackage{pgfpages} \setbeameroption{show notes on second screen=left} %\setbeameroption{hide notes} %\setbeameroption{show only notes} %%%%% Remove Subsection bar from header \makeatletter \setbeamertemplate{headline} {% \begin{beamercolorbox}[wd=\paperwidth,colsep=1.5pt]{upper separation line head} \end{beamercolorbox} \begin{beamercolorbox}[wd=\paperwidth,ht=2.5ex,dp=1.125ex,% leftskip=.3cm,rightskip=.3cm plus1fil]{title in head/foot} \usebeamerfont{title in head/foot}\insertshorttitle \end{beamercolorbox} \begin{beamercolorbox}[wd=\paperwidth,ht=2.5ex,dp=1.125ex,% leftskip=.3cm,rightskip=.3cm plus1fil]{section in head/foot} \usebeamerfont{section in head/foot}% \ifbeamer@tree@showhooks \setbox\beamer@tempbox=\hbox{\insertsectionhead}% \ifdim\wd\beamer@tempbox>1pt% \hskip2pt\raise1.9pt\hbox{\vrule width0.4pt height1.875ex\vrule width 5pt height0.4pt}% \hskip1pt% \fi% \else% \hskip6pt% \fi% \insertsectionhead \end{beamercolorbox} % Code for subsections removed here } \makeatother \usepackage{amsmath} %%%%% Add Frame Number \addtobeamertemplate{navigation symbols}{}{% \usebeamerfont{footline}% \usebeamercolor[fg]{footline}% \hspace{1em}% \insertframenumber } \title{ The KM3NeT project \\ ARCA + ORCA } \date{April 21st, 2020} \author{E.T. de Boone} \begin{document} \frame{\titlepage} \begin{frame} \frametitle{Outline} \tableofcontents \end{frame} \begin{frame} \frametitle{Papers} \begin{figure} \centering \includegraphics[width=\textwidth]{images/paper-prototype.png} \end{figure} \begin{figure} \centering \includegraphics[width=\textwidth]{images/paper-letter-of-intent.png} \end{figure} \end{frame} \begin{frame} \frametitle{Astrophysical vs Atmospheric Neutrino} \begin{figure} \centering \includegraphics[width=0.9\textwidth]{images/neutrino_sources.png} %{\tiny \href{https://doi.org/10.1140/epjh/e2012-30014-2}{10.1140/epjh/e2012-30014-2}} \end{figure} \end{frame} \note[itemize]{ \item Distinction Atmospheric vs Astrophysical \begin{itemize} \item steep decline for > TeV \item lower energies \end{itemize} \item Observatories: IceCube, ANTARES \begin{itemize} \item IceCube: 100 GeV - several PeV \item ANTARES: 10 GeV - 100 TeV \end{itemize} \item Types of events \begin{itemize} \item Tracklike (through-going) \item Showerlike \end{itemize} } %%%%%%%%%%%%%%%%%% %% General Info %% %%%%%%%%%%%%%%%%%% \section{General Info} \subsection{KM3NeT} \begin{frame} \frametitle{KM3NeT} Cubic Kilometer Neutrino Telescope \begin{itemize} \item Deep-sea neutrino telescope \note[item]{ Observation Principle IceCube } \item Three locations in the Mediterranean Sea \note[item]{ Locations: Toulon (FR), Sicily (It), Pylos (Gr) } \note[item]{ Properties Water } \bigskip \pause \item 2 Main objectives \begin{itemize} \item Determine the Neutrino Mass Hierarchy \item Observe the Universe using Neutrino’s \end{itemize} \end{itemize} \end{frame} \note[itemize] { \item Neutrino Mass Hierarchy \begin{itemize} \item Neutrino's have mass \end{itemize} \item Universe \begin{itemize} \item Counterpart to IceCube \item Objectives to confirm icecube findings \end{itemize} } \begin{frame} \begin{figure} \centering \includegraphics[width=1\textwidth]{images/km3net-infrastructure.jpg} \end{figure} \end{frame} \note[itemize] { \item Spread over large part of mediterranean sea \item Reason for locations: deep water \item Succesor to: \begin{itemize} \item ANTARES (Fr): only ten km from \item NEMO (It) \item NESTOR (Gr) \end{itemize} \item Greece is pending future funding } \begin{frame} \frametitle{KM3NeT} \begin{itemize} \item 2 main objectives \begin{itemize} \item Determine the Neutrino Mass Hierarchy \item Observe the Universe using Neutrino’s \end{itemize} \bigskip \pause \item 2 main experiments \begin{itemize} \item ORCA: Oscillation Research with Cosmics in the Abyss \item ARCA: Astroparticle Research with Cosmics in the Abyss \end{itemize} \end{itemize} \end{frame} \note[itemize] { \item ORCA in Fr, ARCA in Italy \item Combined sensitivity from GeV to above PeV \item ORCA: \begin{itemize} \item Focus on atmospheric neutrinos \item densely packed \item GeV to TeV $\nu$'s \end{itemize} \item ARCA: \begin{itemize} \item Focus on (extra)galactic neutrinos \item sparsely packed \item TeV to PeV $\nu$'s \end{itemize} } %% Technology %% \begin{frame} \frametitle{Detector Design} \pause \begin{figure} \includegraphics[width=0.8\textwidth]{images/principal-idea-neutrino-telescope-icecube-with-text.png} \end{figure} \end{frame} \note[itemize]{ \item Old design => Markov 1960 multiple predecessors \item compare with IceCube, ANTARES, DUMAND \bigskip \item Cherenkov light \item Digital-Optical Module } \begin{frame} \frametitle{Detector Prototypes} \begin{columns} \column{0.6\textwidth} \begin{figure} \includegraphics[width=\textwidth]{images/km3net-ppm-du-schematic.png} \end{figure} \column{0.4\textwidth} \begin{itemize} \item Digital Optical Module (April 2013) \item Detection Unit (May 2014) \end{itemize} \end{columns} \end{frame} \begin{frame} \begin{columns} \column{0.6\textwidth} \begin{figure} \includegraphics[width=\textwidth]{images/km3net-building-block-du.png} \end{figure} \column{0.4\textwidth} Building Block \begin{itemize} \item 115 strings \item 18 Digital Optical Modules per string \item 31 Photo Multiplier Tubes per DOM \end{itemize} \end{columns} \end{frame} % Digital Optical Modules %%%%%%%%%%%%%%%%%%%%%%%%%%% \begin{frame} \frametitle{ Digital Optical Modules } \begin{figure} \includegraphics[width=0.6\textwidth]{images/km3net-build-dom.png} \end{figure} \end{frame} \begin{frame} \frametitle{Calibration} \begin{itemize} \item Acoustic Sensor \item $^{40}$K decay in seawater \end{itemize} \begin{figure} \includegraphics[width=0.4\textwidth]{images/km3net-build-dom-with-piezo.png} \end{figure} \end{frame} \note[itemize] { \item $^{40}$K \begin{itemize} \item $\lambda_{1/2}$ Gyr \end{itemize} } \subsection{Event Trigger} \begin{frame} \frametitle{Event Triggers} \end{frame} %%%%%%%%%%%%%%%%%% %% Physics %% %%%%%%%%%%%%%%%%%% %% ORCA \section{ORCA - Particle Physics} \begin{frame} \frametitle{ORCA - Particle Physics} \begin{figure} \includegraphics[width=\textwidth]{images/km3net-orca-locations-france.png} \end{figure} \end{frame} \subsection{Neutrino Mass Hierarchy} \begin{frame} \frametitle{Neutrino Mass Hierarchy} \end{frame} %% ARCA \section{ARCA - Astroparticle Physics} \begin{frame} \frametitle{ARCA - Astroparticle Physics} \begin{columns} \column{.5\textwidth} \begin{figure} \includegraphics[width=\textwidth]{images/km3net-arca-locations-italy.png} \end{figure} \column{.5\textwidth} \begin{figure} \includegraphics[width=\textwidth]{images/km3net-arca-block-division.png} \end{figure} \end{columns} \end{frame} \begin{frame} \frametitle{Differences between ARCA and ORCA} \begin{figure} \includegraphics[width=\textwidth]{images/KM3NeT-ARCA-and-ORCA-comparison-area.png} \end{figure} \end{frame} \subsection{Glashow Resonance} \begin{frame} \frametitle{Glashow Resonance} \end{frame} %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% \begin{frame} \frametitle{Recap} \begin{itemize} \item Deep-sea Cubic Kilometer Neutrino Telescope in the Mediterranean Sea \item 2 objectives $\mapsto$ 2 experiments \begin{itemize} \item ARCA: Astrophysics Research with Cosmics in the Abyss \item ORCA: Oscillation Research with Cosmics in the Abyss \end{itemize} \item Field of View contains Galactic Plane \end{itemize} \pause \begin{center} \vspace{1em} Question Time \end{center} \end{frame} \end{document}