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Moved old dir to subdirectory 2018-19

This commit is contained in:
Eric-Teunis de Boone 2020-04-16 10:38:52 +02:00
parent 18ca312dcd
commit e7003ee061
22 changed files with 30 additions and 12 deletions

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@ -0,0 +1,707 @@
%% This file implements the beamer template for the 2014 Radboud
%% University corporate style. It also contains the template for
%% the Centre for Language and Speech Technology department.
%%
%% For comments, questions, and suggestions contact me at
%% l.onrust@let.ru.nl or visit the github repository on
%% https://github.com/naiaden/presentations/tree/master/ruhuisstijl
%% (this single-file version can be found in the distributed dir)
%%
%% You can distribute and edit the files as you wish, but I'd
%% love to hear of any changes. Also, if you let me know that
%% you are using the template, I can keep you up-to-date on
%% future changes.
\NeedsTeXFormat{LaTeX2e}
\ProvidesClass{beamerruhuisstijl}[2014/10/07 Beamer template for Radboud University corporate style]
\LoadClass[xcolor=table,10pt,t]{beamer}
\RequirePackage[utf8]{inputenc}
\RequirePackage[T1]{fontenc}
\RequirePackage{pgfpages}
\RequirePackage{calc}
\RequirePackage{ifthen}
\RequirePackage{tikz}
\newif\ifbeamer@official
\beamer@officialfalse
\DeclareOptionBeamer{official}[false]{\csname beamer@official#1\endcsname}
\DeclareOptionBeamer{handout}{\gdef\beamer@currentmode{handout}}
\newcommand{\notes}{hide notes}
\DeclareOptionBeamer{notes}{\renewcommand{\notes}{#1}}
\newcommand{\dept}{none}
\DeclareOptionBeamer{department}{\renewcommand{\dept}{#1}}
\newcommand{\grouplogo}{none}
\DeclareOptionBeamer{grouplogo}{\renewcommand{\grouplogo}{#1}}
\newcommand{\spp}{1}
\DeclareOptionBeamer{slidesperpage}{\renewcommand{\spp}{#1}}
\newcommand{\tablecolours}{false}
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\newcommand{\alwaysshowdate}{false}
\DeclareOptionBeamer{alwaysshowdate}{\renewcommand{\alwaysshowdate}{#1}}
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\newcommand{\tocatsectionstarttitle}{Overview}
\DeclareOptionBeamer{tocatsectionstarttitle}{\renewcommand{\tocatsectionstarttitle}{#1}}
\newcommand{\showinstitute}{false}
\DeclareOptionBeamer{showinstitute}{\renewcommand{\showinstitute}{#1}}
\newcommand{\showdate}{false}
\DeclareOptionBeamer{showdate}{\renewcommand{\showdate}{#1}}
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% stack on top of one another
\pgfpageslogicalpageoptions{1}
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\mode<presentation>
\setbeamerfont{page number in head/foot}{size=\footnotesize}
\setbeamercolor*{page number in head/foot}{fg=ruhuisstijlzwart}
\setbeamerfont{author in head/foot}{size=\footnotesize}
\setbeamercolor*{author in head/foot}{fg=ruhuisstijlzwart}
%%% Footnote stuff
% Cannot get it working to skip the title page when extra information
% is displayed in the footline. In the next version hopefully...
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/\inserttotalframenumber
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{}
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\usebeamerfont{author in head/foot}\insertshortauthor
\end{beamercolorbox}
}{}
\ifthenelse{\equal{\alwaysshowdate}{true}}{%
\begin{beamercolorbox}[wd=.15\paperwidth,ht=2.25ex,dp=1ex]{author in head/foot}%
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\end{beamercolorbox}
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}
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\setbeamertemplate{footnote}{%
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%%% Table of content stuff
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\defbeamertemplate{description item}{align left}{\hspace*{1em}\insertdescriptionitem\hfill}
\setbeamertemplate{description item}[align left]
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\setbeamertemplate{description item}[align left]
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%%% Itemisation stuff
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{%
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% The original style requires 2.5cm margin, whatever that means. Our frames
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\documentclass{standalone}
\usepackage{tikz}
\usetikzlibrary{decorations.pathmorphing}
\usetikzlibrary{decorations.markings}
\usetikzlibrary{patterns}
\begin{document}
\begin{tikzpicture}[decoration={
markings,
mark=at position 0.5 with {\arrow{>}}}
]
\draw[thick,postaction={decorate}] (-2,3) node[left] {$\nu_\mu$} -- (0,2) ; % incoming top
\draw[thick,postaction={decorate}] (0,2) -- (2,3) node[right] {$\mu^-$} ; % outgoing top
\draw[draw=white,double=black, very thick, decorate, decoration=snake] (0,2) -- (0,1) node[right,pos=0.5] {$W^{+}$};
\draw[thick,postaction={decorate}] (-2,0) node[left] {$e^{-}$} -- (0,1); % ingoing bottom
\draw[thick,postaction={decorate}] (0,1) -- (2,0) node[right] {$\nu_e$} ; % ingoing bottom
\end{tikzpicture}
\end{document}

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\documentclass{standalone}
\usepackage{tikz}
\usetikzlibrary{decorations.pathmorphing}
\usetikzlibrary{decorations.markings}
\usetikzlibrary{patterns}
\begin{document}
\begin{tikzpicture}[decoration={
markings,
mark=at position 0.5 with {\arrow{>}}}
]
\draw[thick,postaction={decorate}] (-2,3) node[left] {$\nu_\mu$} -- (0,2) ; % incoming top
\draw[thick,postaction={decorate}] (0,2) -- (2,3) node[right] {$\nu_\mu$} ; % outgoing top
\draw[draw=white,double=black, very thick, decorate, decoration=snake] (0,2) -- (0,1) node[right,pos=0.5] {$Z$};
\draw[thick,postaction={decorate}] (-2,0) node[left] {$e^{-}$} -- (0,1); % ingoing bottom
\draw[thick,postaction={decorate}] (0,1) -- (2,0) node[right] {$e^{-}$} ; % ingoing bottom
\end{tikzpicture}
\end{document}

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%\documentclass[alwaysshowauthor=true,spp=2,showdate=true,slidenumbers=relative]{beamerruhuisstijl}
\documentclass{beamer}
\usepackage{amsmath}
\usepackage{amssymb}
\usepackage{tikz}
\usepackage[english]{babel}
%\title{Evidence for High-Energy Extraterrestrial Neutrinos at the IceCube Detector}
\title{ IceCube Neutrino Astronomy }
\author{Eric Teunis de Boone}
\addtobeamertemplate{navigation symbols}{}{%
\usebeamerfont{footline}%
\usebeamercolor[fg]{footline}%
\hspace{1em}%
\insertframenumber
}
\begin{document}
\begin{frame}[noframenumbering]
\titlepage
\end{frame}
\note{}
%%%%%%% Outline
% History of Neutrino Astronomy - (Instruments)
% Introduction into Neutrino Astronomy
% + Cherenkov
% IceCube, IceTop, DeepCore
% + IceTop
% + IceCube
% + DeepCore
%
%
%
%
%
%%%%%%%%%%%%%%%%%%%%%
\begin{frame}[noframenumbering]{Overview}
\tableofcontents
\end{frame}
\section{ Neutrino Astronomy }
\begin{frame}{ Why Neutrino Astronomy }
\includegraphics[width=\textwidth]{images/icecube-3-fig9-multimessenger-spectrum.png}
\end{frame}
\begin{frame}{ Neutrino Astronomy: History }
\begin{itemize}
\item First observation of neutrino in 1956
\item Deep Underwater Muon and Neutrino Detector, Hawaii (1990)
failed, but proof of concept for ANTARES, KM3NeT
\item Antarctic Muon and Neutrino Detector Array (, now part of IceCube)
\end{itemize}
\end{frame}
\begin{frame}{ Neutrino Astronomy: Basics }
\begin{itemize}
\item Neutrino interacts in atmosphere, ice or water
\item Charged particle gets into the ice or water and emit Cherenkov photons
\item Cherenkov photons detected by DOMs in the matter
\end{itemize}
\begin{columns}[t]
\begin{column}{0.9\textwidth}
\begin{figure}[hbtp]
\centering
\includegraphics[width=\textwidth]{images/icecube-3-fig1-initial-outline.png}
\includegraphics[width=0.3\textwidth]{images/prinicipal_idea_neutrino_telescope.png}
\caption{\small Cherenkov cone propagating through the IceCube Detector}
\end{figure}
\end{column}
\end{columns}
\end{frame}
\begin{frame}{ Neutrino Astronomy: Production }
Neutrinos produced in sources and CR interactions
\begin{itemize}
\item Main CR interactions:
\begin{itemize}
\item $ p + \gamma_{bg} \to p + \pi^0 \to p + \gamma + \gamma $
\item $ p + \gamma_{bg} \to n + \pi^+ \to n + \mu^ + \nu_\mu \to n + \nu_\mu + e^ + \bar{\nu_\mu} + \nu_e $
\end{itemize}
\end{itemize}
\end{frame}
\section{IceCube observatory}
\begin{frame}{IceCube observatory}
\includegraphics[width=0.9\textwidth]{images/icecube-array-fancy.png}
\end{frame}
\begin{frame}{IceCube observatory}
Divided into three parts:
\begin{itemize}
\item IceTop: detects CR airshower above IceCube
\item IceCube: the main detector for $E_\nu > 100$ GeV
\item DeepCore: sensitive for $E_\nu \raise.17ex\hbox{$\scriptstyle\sim$} 10$ GeV due to tight spacing
\end{itemize}
\includegraphics[width=\textwidth]{images/icecube-3-fig2-architecture-and-dom.png}
\end{frame}
%\begin{frame}{IceCube observatory: Digital Optical Module}
% \includegraphics[width=\textwidth]{images/icecube-4-Aartsen_2017_DOM.pdf}
%\end{frame}
\subsection{Event Detection and Background}
\begin{frame}{Event Detection}
Event selection and simulation needed to identify particles.\\
IceTop and outer region of IceCube are veto regions.
\begin{figure}[hbtp]
\centering
\includegraphics[width=0.75\textwidth]{images/icecube_veto_regions.png}
%\caption{\ref{}}
\end{figure}
\end{frame}
\begin{frame}{Event Detection}
\begin{columns}[t]
\begin{column}{.5\textwidth}
\begin{block}{Tracklike}
\begin{itemize}
\item Distinct track -- caused by $\mu^{-}$
\item Angular resolution $\lesssim 1\deg$
\item Energy resolution not so good
\end{itemize}
\end{block}
\end{column}
\begin{column}{.5\textwidth}
\begin{block}{Showerlike}
\begin{itemize}
\item Spherical light pattern due to well-localised particle shower
\item Angular resolution $\sim 15\deg$
\item Energy resolution $\sim 15\%$
\end{itemize}
\end{block}
\end{column}
\end{columns}
\includegraphics[width=\textwidth]{images/simulation_of_cherenkov_propagation.png}
\end{frame}
\begin{frame}{Event Detection}
\begin{columns}[t]
\begin{column}{.5\textwidth}
\begin{block}{Tracklike}
\begin{itemize}
\item Mostly CC of $\nu_\mu$
\item Through-going Muons
\end{itemize}
\end{block}
\end{column}
\begin{column}{.5\textwidth}
\begin{block}{Showerlike}
\begin{itemize}
\item NC of all $\nu$ flavours
\item CC of $\nu_e$ (and $\nu_\tau$ if $E \lesssim 100 TeV$)
\end{itemize}
\end{block}
\end{column}
\end{columns}
both: Glashow resonance of $\overline{\nu_e}$ at $E \sim 6.3 PeV$ on $e^{-}$ to $W$
\begin{columns}[t]
\begin{column}{.5\textwidth}
\begin{block}{Charged Current}
\includegraphics[width=\textwidth]{feynman_diags/charged_current.pdf}
\end{block}
\end{column}
\begin{column}{.5\textwidth}
\begin{block}{Neutral Current}
\includegraphics[width=\textwidth]{feynman_diags/neutral_current.pdf}
\end{block}
\end{column}
\end{columns}
%\begin{figure}
% \includegraphics[width=0.5\textwidth]{images/charged_and_neutral_neutrino_interactions.pdf}
% \caption{From \url{http://inspirehep.net/record/1236362/files/TwoDiagrams.png}}
%\end{figure}
\end{frame}
\begin{frame}{Background vs Signals}
\begin{itemize}
\item 2500 to 2900 events per second
\item $\sim 10^{5}$ atmospheric neutrinos vs. $\lesssim 10^3$ cosmic neutrinos per year
\item $10^{-6}$ events due to neutrino interaction
\end{itemize}
\end{frame}
\section{High Energy Extraterrestrial Neutrinos}
\begin{frame}{High Energy Extraterrestrial Neutrinos}
\small{ 28 neutrino candidate events, ranging from 30 to $1200 TeV$ in a 2-year dataset }
\includegraphics[width=\textwidth]{images/icecube-3-table1-28events.png}
\end{frame}
\begin{frame}{High Energy Extraterrestrial Neutrinos}
\includegraphics[width=\textwidth]{images/icecube-3-fig3-vertical-deposition.png}
\end{frame}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
% Appendix
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\end{document}