201 lines
4.9 KiB
TeX
201 lines
4.9 KiB
TeX
\documentclass{beamer}
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\usepackage[utf8]{inputenc}
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\usepackage{amsmath}
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\usepackage{unicode-math}
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\usetheme{Madrid}
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\usecolortheme{default}
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%------------------------------------------------------------
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%This block of code defines the information to appear in the
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%Title page
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\title{Observational Astronomy}
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\subtitle{How we make the EM spectrum our bitch}
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\author{Lauren Thomas (ljaytee)}
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\date{Newline 2023}
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%End of title page configuration block
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%------------------------------------------------------------
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%------------------------------------------------------------
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%The next block of commands puts the table of contents at the
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%beginning of each section and highlights the current section:
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%------------------------------------------------------------
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\begin{document}
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%The next statement creates the title page.
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\frame{\titlepage}
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\section{First section}
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%---------------------------------------------------------
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%Changing visivility of the text
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\begin{frame}{Light spectra}{Electromagnetic spectrum}
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\centering
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\includegraphics[width=10cm]{Encyclopaedia Brittanica EM spectrum.jpg}
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\end{frame}
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%---------------------------------------------------------
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%---------------------------------------------------------
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%Example of the \pause command
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\begin{frame}{How is electromagnetic radiation created}
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\begin{figure}
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\centering
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\includegraphics{Bohr_atom_model.pdf}
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\caption{Bohr model of a hydrogen atom}
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\end{figure}
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\end{frame}
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\begin{frame}{How is electromagnetic radiation created}
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\begin{figure}
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\centering
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\includegraphics{Bohr_atom_model_absorb.pdf}
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\caption{Absorption}
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\end{figure}
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\end{frame}
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\begin{frame}{How is electromagnetic radiation created}
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\begin{figure}
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\centering
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\includegraphics{Bohr_atom_model_emit.pdf}
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\caption{Emission}
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\end{figure}
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\end{frame}
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\begin{frame}{Photon energy}
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\begin{align*}
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\action<+->{
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&E_3 - E_2 = {\sf Energy~ of~ the~ photon} = hf \\
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&{\sf where~} h =6.626\cdot 10^{-34} J\cdot Hz^{-1} \\
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}
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\action<+->{
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&E = {hc \over \lambda} \\
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&c =3\cdot 10^8 m\cdot s^{-1}
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}
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\end{align*}
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\end{frame}
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\begin{frame}{Let's do an example}
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\begin{align*}
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E_n &= {-hc R_\infty \over n^2} \\
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R_\infty &= {m_e e^4 \over 8\epsilon_0 ^2 h^3 c}
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\end{align*}
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\begin{alignat*}{3}
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R_\infty &= 10\:973\:781.568160\; m^{-1} &\hspace{1em}& {\sf Rydberg~ constant} \\
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n_e &= 9.11 \cdot 10^{-31}\; kg && {\sf Electron~ mass} \\
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e &= 1.602 \cdot 10^{-19}\; C && {\sf Elementary~ charge} \\
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\epsilon_0 &= 8.854 \cdot 10^{-12}\; F \cdot m^{-1} && {\sf Permitivity~ of~ free~ space}
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\end{alignat*}
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\end{frame}
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\begin{frame}{Lets's do an example (continued)}
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The Rydberg constant for hydrogen can be calculated using the reduced mass of the electron.
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\begin{align*}
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R_H &= R_\infty {m_p \over m_e + m_p} \\
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R_H &= 0.999\ldots R_\infty
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\end{align*}
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\end{frame}
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\begin{frame}{Lets's do an example (continued)}
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\begin{align*}
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E_3 - E_2 &= 3.027 \cdot 10^{-19} \\
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E &= {hc \over \lambda} \\
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\lambda &= {hc \over E} \\
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& = 6.5611 \cdot 10^{-7} m \\
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& ~\therefore \\
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\lambda &= 656\; nm~ (3\; s.f.)
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\end{align*}
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\end{frame}
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\begin{frame}{Emission and absorption spectra}
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\begin{figure}
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\centering
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\includegraphics[width=12cm]{emission-and-absorption-spectra.jpeg}
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\end{figure}
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\end{frame}
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\begin{frame}{A real emission spectrum}
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\begin{figure}
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\centering
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\includegraphics[width=7cm]{qso.jpg}
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\end{figure}
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\end{frame}
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\begin{frame}{Redshift and the expanding universe}
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\begin{eqnarray*}
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z &= \sqrt\dfrac{c+v}{ c-v} - 1 \\
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&= \dfrac{\lambda_{obs} - \lambda_{emit}}{\lambda_{emit}}
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\end{eqnarray*}
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\end{frame}
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%---------------------------------------------------------
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\end{document}
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\section{Second section}
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%---------------------------------------------------------
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%Highlighting text
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\begin{frame}
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\frametitle{Sample frame title}
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In this slide, some important text will be
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\alert{highlighted} because it's important.
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Please, don't abuse it.
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\begin{block}{Remark}
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Sample text
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\end{block}
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\begin{alertblock}{Important theorem}
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Sample text in red box
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\end{alertblock}
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\begin{examples}
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Sample text in green box. The title of the block is ``Examples".
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\end{examples}
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\end{frame}
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%---------------------------------------------------------
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%---------------------------------------------------------
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%Two columns
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\begin{frame}
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\frametitle{Two-column slide}
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\begin{columns}
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\column{0.5\textwidth}
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This is a text in first column.
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$$E=mc^2$$
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\begin{itemize}
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\item First item
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\item Second item
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\end{itemize}
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\column{0.5\textwidth}
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This text will be in the second column
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and on a second tought this is a nice looking
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layout in some cases.
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\end{columns}
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\end{frame}
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%---------------------------------------------------------
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%%% Local Variables:
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%%% mode: latex
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%%% TeX-master: t
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%%% End:
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