phy-4660/feedback/report/report.tex

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2017-04-24 06:37:51 +00:00
\documentclass[11pt,letterpaper]{article}
%\usepackage{aas_macros}
\usepackage{biblatex}
\usepackage{graphicx}
\usepackage[margin=1.in,centering]{geometry}
\usepackage{hyperref}
\usepackage{caption}
\usepackage[export]{adjustbox}
\usepackage{float}
\usepackage{gensymb}
\bibliography{/home/caes/wmu/phy-4660/adv_lab.bib}
\begin{document}
%\newcommand{}$^7\textrm{Li(p,}\alpha)^4\textrm{He}$ reaction.\\
\newcommand{\LCDM}{$\Lambda$CDM}
\title{Active Galactic Nuclei in Cosmology}
\author{Otho Ulrich}
\maketitle
\begin{abstract}
Active Galactic Nuclei (AGN) play a role in cosmology as both component and probe.
They are used to contrain cosmological parameters, to characterize the intergalactic medium, and as a .
AGN interact with their host galaxies, influencing its evolution through a process called AGN feedback.
Modeling AGN feedback presents significant challenges, but has improved upon the \LCDM model as tested by the Millenium Simulation. \cite{2005Natur.435..629S}
\end{abstract}
%─────────────
\section{Introduction}
\label{sec:intro}
%─────────────
\section{Cosmology}
\label{sec:cosmology}
\subsection{Millenium Simulation}
The Millenium Simulation tests the \LCDM cosmology
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%─────────────
\section{Quasar Feedback Simulations}
\label{sec:feedbacksims}
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%─────────────
\section{Conclusion}
\label{sec:conclusion}
\printbibliography
\end{document}