phy-4660/feedback/report/report.tex

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\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}


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\section{Introduction}
    \label{sec:intro}

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\section{Cosmology}
    \label{sec:cosmology}

    \subsection{Millenium Simulation}
    The Millenium Run and its following iterations are N-body simulations that predict the evolution of the matter in the universe. It is considered a (successful) test of the \LCDM cosmology.


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\section{Quasar Feedback Simulations}
\label{sec:feedbacksims}

    It is strongly believed by cosmologists that 

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\section{Conclusion}
    \label{sec:conclusion}


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