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writing accelerator report

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caes 2017-03-21 05:15:13 -04:00
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accelerator/report/report.tex
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\usepackage{caption}
\usepackage[export]{adjustbox}
\usepackage{float}
\usepackage{gensymb}
\bibliography{/home/caes/wmu/phy-4660/adv_lab.bib}
@ -44,17 +44,19 @@
\begin{figure}
\center
\includegraphics[width=6in]{../abundances.png}
\includegraphics[width=4.5in]{../abundances.png}
\caption{Relative elemental abundances in the sun's photosphere. Lithium and fluorine are much less abundant than their neighbour elements. It is thought this is due to large probability cross-sections for a proton collision with these nuclei. \cite{Carroll&Ostlie}}
\end{figure}
\section{Nuclear Reactions and Detection Plan}
\label{sec:beamreactions}
We expect three reactions to occur
\begin{figure}
\center
\includegraphics[width=4.5in]{../collision.png}
\caption{In general, an incident particle collides with a target nucleus, resulting in an emitted particle and a residual nucleus. The backscattering experiments in this study have $\theta = 149\pm0.05\degree$ \cite{ADVLABACCEL}}
\caption{In general, an incident particle collides with a target nucleus, resulting in an emitted particle and a residual nucleus. The backscattering experiments in this study have $\theta = 149\pm0.05\degree$ \cite{ADVLABACCEL}.}
\end{figure}