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