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