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