diff --git a/2019-20/presentation/images/Neutrino-candidate-in-KM3NeT-ORCA6.jpg b/2019-20/presentation/images/Neutrino-candidate-in-KM3NeT-ORCA6.jpg new file mode 100644 index 0000000..91b41f1 Binary files /dev/null and b/2019-20/presentation/images/Neutrino-candidate-in-KM3NeT-ORCA6.jpg differ diff --git a/2019-20/presentation/images/km3net-orca-significance-nmh.jpg b/2019-20/presentation/images/km3net-orca-significance-nmh.jpg new file mode 100644 index 0000000..68a5480 Binary files /dev/null and b/2019-20/presentation/images/km3net-orca-significance-nmh.jpg differ diff --git a/2019-20/presentation/images/neutrino-oscillation.jpg b/2019-20/presentation/images/neutrino-oscillation.jpg new file mode 100644 index 0000000..e660962 Binary files /dev/null and b/2019-20/presentation/images/neutrino-oscillation.jpg differ diff --git a/2019-20/presentation/presentation.tex b/2019-20/presentation/presentation.tex index e5c8ae5..fb572a2 100644 --- a/2019-20/presentation/presentation.tex +++ b/2019-20/presentation/presentation.tex @@ -191,14 +191,14 @@ \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 @@ -267,6 +267,7 @@ \note[itemize] { \item PMT: gain $10^6$ + \item PMT: compare amount with IceCube: 1:31 \item Acoustics: resolution to 20 cm $\mapsto$ 1 ns } @@ -292,6 +293,10 @@ \end{figure} \end{columns} \end{frame} + \note[itemize] + { + \item DOM uplink 1Gbps + } % Calibration %%%%%%%%%%%%%%%%%%%%%%%%%% @@ -305,6 +310,11 @@ \end{itemize} \end{itemize} \end{frame} + \note[itemize] + { + \item 8ns data + \item $1\mathrm{ns} \times c = 30\mathrm{cm}$ $\mapsto$ $\Delta x \approx 2.40\mathrm{m}$ + } %% \begin{frame} @@ -352,6 +362,7 @@ \item comparison of timings on the same string \item Acoustics: position calibration } + %% \begin{frame} \frametitle{Background Effects} @@ -367,16 +378,24 @@ \item bioluminescence: marine sciences, effect of upto 10\% \item } + % Events %%%%%%%%%%%%%%%%%%%%%%%% \begin{frame} \frametitle{Event Triggers} + \begin{columns} + \column{0.6\textwidth} Multiple Triggers \begin{itemize} \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 \end{itemize} + \column{0.4\textwidth} + \begin{figure} + \includegraphics[width=\textwidth]{images/Neutrino-candidate-in-KM3NeT-ORCA6.jpg} + \end{figure} + \end{columns} \end{frame} \note[itemize] { @@ -386,6 +405,23 @@ \item study gives relative time offset mostly 10 ns. \end{itemize} \item L2: halves the remaining hits + + \item Causality: $25\mathrm{ns} \mapsto 7.5\mathrm{m}$ + } + + %% + \begin{frame} + \frametitle{Event Triggers: Muon Tracks and Showers} + \begin{figure} + \includegraphics[width=\textwidth]{images/km3net-track-length-estimation.png} + \end{figure} + \end{frame} + \note[itemize] + { + \item Various Trigger Algorithms + \item Muon track + \item directional filter $\sim 10^\circ$ $\mapsto$ 200 directions cover $4\pi$ + \item shower events } %%%%%%%%%%%%%%%%%% @@ -406,7 +442,8 @@ \begin{columns} \column{.4\textwidth} \begin{itemize} - \item + \item 1 Building Block + \item dense packing $\mapsto$ sensitivity GeV to TeV \end{itemize} \column{.6\textwidth} \begin{figure} @@ -416,6 +453,10 @@ \end{frame} \note[itemize] { + \item depth: 2500m + \item height: 150m + \item width: \textit{see frame} + \item instrumented volume: 8 Million tonnes of water \item horizontal distance 20m \item vertical distance 6m } @@ -425,27 +466,34 @@ \end{figure} \end{frame} -\subsection{Neutrino Mass Hierarchy} +%\subsection{Neutrino Mass Hierarchy} + %% + \begin{frame} + \frametitle{Neutrino Oscillations} + \begin{center} + \begin{itemize} + \item Pontecorvo - Maki - Nakagawa - Sakata matrix + \item 3 angles, 1 phase + \end{itemize} + \begin{figure} + \includegraphics[width=.8\textwidth]{images/neutrino-oscillation.jpg} + \end{figure} + \end{center} + \end{frame} + \note[itemize] + { + \item solar neutrino puzzle + \item + \item mass eigenstates $\neq$ flavour eigenstates, mass squared diff + } + + %% \begin{frame} \frametitle{Neutrino Mass Hierarchy} \begin{figure} \includegraphics[width=\textwidth]{images/neutrino-mass-hierarchies.png} \end{figure} \end{frame} - - %% - \begin{frame} - \frametitle{Neutrino Oscillations} - \end{frame} - \note[itemize] - { - \item mass eigenstates $\neq$ flavour eigenstates, mass squared diff - } - - %% - \begin{frame} - \frametitle{Neutrino Oscillations in Matter} - \end{frame} \note[itemize] { \item vaccum oscillations insensitive to sign of mass sq. diff. @@ -455,6 +503,11 @@ \item $\sigma(\nu N) \approx 2\sigma(\bar{\nu} N)$ } + %% + \begin{frame} + \includegraphics[width=\textwidth]{images/km3net-orca-significance-nmh.jpg} + \end{frame} + %%%%%%%%%%%%%%% %% ARCA @@ -493,7 +546,7 @@ \frametitle{IceCube and Expected Signal} \begin{itemize} \item Signals from 10 TeV to above 1 PeV - \item 54 events with reconstructed energy above 30TeV (2016) + \item 54 events with reconstructed energy above 30TeV (2016, IceCube) \end{itemize} \pause \begin{figure}