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Wrap up for tonight

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Eric Teunis de Boone 2020-04-19 22:43:51 +02:00
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2019-20/presentation/presentation.tex
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@ -2,10 +2,10 @@
\usetheme{Antibes}
%\usepackage{pgfpages}
%\setbeameroption{show notes on second screen=left}
\usepackage{pgfpages}
\setbeameroption{show notes on second screen=left}
%\setbeameroption{show notes}
\setbeameroption{hide notes}
%\setbeameroption{hide notes}
%\setbeameroption{show only notes}
%%%%% Remove Subsection bar from header
@ -45,7 +45,7 @@
\hspace{1em}%
\insertframenumber
}
\title{ The KM3NeT project \\ ARCA + ORCA }
\title{The KM3NeT project\\ ARCA + ORCA}
\date{April 21st, 2020}
\author{E.T. de Boone}
@ -119,7 +119,7 @@
\item 2 Main objectives
\begin{itemize}
\item Determine the Neutrino Mass Hierarchy
\item Observe the Universe using Neutrino’s
\item Observe the Universe with highly energetic Neutrino’s
\end{itemize}
\end{itemize}
\end{frame}
@ -127,12 +127,13 @@
\item Neutrino Mass Hierarchy
\begin{itemize}
\item Neutrino's have mass
\item flavour eigenstates $neq$ mass eigenstates
\end{itemize}
\item Universe
\begin{itemize}
\item Counterpart to IceCube
\item Objectives to confirm icecube findings
\item Counterpart to IceCube - Galactic Plane in FoV
\end{itemize}
}
@ -145,10 +146,10 @@
\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)
\item Succesor to and experience from: \begin{itemize}
\item ANTARES (Fr)
\item NEMO (It) - Pilot
\item NESTOR (Gr) - Pilot
\end{itemize}
\item Greece is pending future funding
}
@ -172,7 +173,7 @@
\end{frame}
\note[itemize] {
\item ORCA in Fr, ARCA in Italy
\item Combined sensitivity from GeV to above PeV
\item Combined sensitivity from GeV to above PeV: 6 orders of magnitude
\item ORCA:
\begin{itemize}
\item Focus on atmospheric neutrinos
@ -183,20 +184,21 @@
\item Focus on (extra)galactic neutrinos
\item sparsely packed $\mapsto$ TeV to PeV $\nu$'s
\end{itemize}
\item shared technology
}
%% Technology %%
\section{Detector Design}
\begin{frame}
\frametitle{Detector Design}
\note[item]{ Old design => Markov 1960 multiple predecessors }
\note[item]{ compare with IceCube, ANTARES, DUMAND }
\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
@ -212,8 +214,9 @@
\end{figure}
\column{0.5\textwidth}
\begin{itemize}
\item Digital Optical Module \\(April 2013)
\item Detection Unit \\(May 2014)
\item Digital Optical Module \\(Apr 2013)
\item Detection Unit (3 DOMs)\\(May 2014)
\item Detection Unit (18 DOMs)\\(Dec 2015)
\end{itemize}
\end{columns}
\end{frame}
@ -234,6 +237,13 @@
\end{itemize}
\end{columns}
\end{frame}
\note[itemize]
{
\item lattice structure (also on prev slides)
\item data transmission fibre-optics (1 Gbps per DOM)
\item $31 \times 18 = 558$ PMTs per string
\item $558 \times 115 = 64 170$ PMTs per block
}
% Digital Optical Modules
%%%%%%%%%%%%%%%%%%%%%%%%%%%
@ -256,7 +266,9 @@
\end{frame}
\note[itemize]
{
\item PMT: gain $10^6$
\item Acoustics: resolution to 20 cm $\mapsto$ 1 ns
}
%%
@ -336,7 +348,9 @@
\end{frame}
\note[itemize]
{
\item
\item LED: 470nm, fully controlled from shore ($I$, $f$)
\item comparison of timings on the same string
\item Acoustics: position calibration
}
%%
\begin{frame}
@ -349,7 +363,7 @@
\end{frame}
\note[itemize]
{
\item LED: 470nm, fully controlled from shore ($I$, $f$)
\item $^{40}$K is background but also calibrator
\item bioluminescence: marine sciences, effect of upto 10\%
\item
}
@ -362,7 +376,6 @@
\item L0: 0.3 photo-electrons in PMT (in DOM)
\item L1: 2 hits in separate PMTs within 25ns
\item L2: use orientation of PMTs
\note { L2 halves the remaining hits }
\end{itemize}
\end{frame}
\note[itemize]
@ -475,7 +488,7 @@
\end{figure}
\end{frame}
%%
%% Diffuse
\begin{frame}
\frametitle{IceCube and Expected Signal}
\begin{itemize}
@ -509,14 +522,23 @@
\end{figure}
\end{frame}
\subsection{Glashow Resonance}
%% Point like
\begin{frame}
\frametitle{Glashow Resonance}
\begin{figure}
\includegraphics[width=0.9\textwidth]{images/km3net-arca-eff-area-glashow-resonance.png}
\end{figure}
\frametitle{Expected Signals: Point like sources}
\begin{itemize}
\item Good Angular Resolution
\item Galactic Sources can be probed
\end{itemize}
\end{frame}
%\subsection{Glashow Resonance}
% \begin{frame}
% \frametitle{Glashow Resonance}
% \begin{figure}
% \includegraphics[width=0.9\textwidth]{images/km3net-arca-eff-area-glashow-resonance.png}
% \end{figure}
% \end{frame}
@ -538,4 +560,12 @@
Question Time
\end{center}
\end{frame}
\begin{frame}
\frametitle{}
\end{frame}
\begin{frame}
\frametitle{Deployment of Strings}
\url{https://www.youtube.com/watch?v=7HKHW0hLxt4&list=PLL9OR_-tW5qOtfZigqVpzMmTSwkMjCT1s&index=8}
\end{frame}
\end{document}