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pcygni.tex
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\documentclass[12pt,a4paper,twoside]{article}
\usepackage[utf8]{inputenc}
\usepackage{amsmath,amsfonts,amssymb}
\usepackage{graphicx}
\usepackage{natbib}
\usepackage{siunitx}
\usepackage[top=1cm,left=2.5cm,right=2.5cm]{geometry}
\usepackage[pdfborder=0]{hyperref}
\setlength{\parindent}{0pt}
\setlength{\parskip}{15pt}
\pagestyle{empty}
\renewcommand{\baselinestretch}{1.15}
\renewcommand{\labelenumi}{{\bf \arabic{enumi}.}}
\newcommand{\abs}[1]{\ensuremath{\left \vert #1 \right \vert}}
\input{journals.tex}
\begin{document}
\hrule
\begin{enumerate}
\item \textbf{Sobolev Approximation and P-Cygni Line Profiles}
In this exercise, the Sobolev Approximation is used to calculate a P-Cygni
within a Monte Carlo radiative transfer simulation. For this purpose, we
consider a shell in homologous expansion which is illuminated by a radiative
source at its lower boundary. Within the expanding material, photons may
perform resonant line-interactions with one atomic transition only. The
emergent radiation field is recorded and thus line profile, shaped by the
interactions within the shell, calculated. Your task is to write a simple
Monte Carlo program, which solves the propagation of the radiation field. Use
the Sobolev approximation to treat the line interactions and thus determine
the P-Cygni line profile in the emergent spectrum. For this problem you may
adopt the following assumptions:
\begin{itemize}
\item the shell extends from $R_{\mathrm{min}} = \SI{1e11}{cm}$ to
$R_{\mathrm{max}} = \SI{1e13}{cm}$. In velocity space, it covers the
linear range from $0.0001\,c$ to $0.01 \,c$.
\item the shell is entirely composed of hydrogen and the only allowed atomic
transition is the Lyman-$\alpha$ line at the rest frame wavelength of
$1215.6\,\mathrm{\AA}$
\item the material within the shell has constant density and temperature.
These material properties are such that the Sobolev optical depth of the
relevant transition amounts to $\tau_{\mathrm{sob}} = 10$
\item at the lower boundary, an isotropic radiative source is located, which
emits uniformly within the wavelength range $\lambda_{\mathrm{min}} = 1100
\, \mathrm{\AA}$ and $\lambda_{\mathrm{max}} = 1300 \, \mathrm{\AA}$
\end{itemize}
In developing the Monte Carlo routine you may adhere to the following
strategy:
\begin{enumerate}
\item initialise the Monte Carlo packets at the lower boundary. Assign an
initial frequency and direction (assuming no limb darkening, i.e.\ $N(\mu)
\mathrm{d} \mu \propto \mu \mathrm{d}\mu$)
\item packets may only interact at the Sobolev point, i.e.\ at the location
where their CMF frequency is equal to the rest-frame frequency of the line
transition. Determine this point using the Doppler effect formula, $\nu_0 =
\gamma \nu (1 - \beta \mu)$\footnote{For the problem at hand, where $v \ll
c$, you may set $\gamma = 1$.}
\item at the Sobolev point, packets interact if $\tau >
\tau_{\mathrm{sob}}$. The optical depth of the packet is determined in the
usual way, i.e.\ by $\tau = - \ln z$
\item if a line interaction occurs, change the packet properties by assuming
isotropy of the resonant scatterings and by according for
energy conservation in the CMF
\item follow the propagation of each packet in the described fashion until
it leaves through either of the two boundaries. Discard the packet if it
intersects the lower boundary, but record its LF frequency if it emerges
through the outer boundary
\item construct a spectrum from the recorded frequencies
\item compare your obtained spectrum with the analytic solution according to
\citet{Jeffery1990}. For this purpose, you may use the python script,
\texttt{pcygni\_profile.py}. Change the example to match the setup at hand.
Use a large value for \texttt{ve} (e.g.\ $v_e = 10^{40}$) to enforce a uniform
Sobolev optical depth throughout the ejecta in
the analytic calculation. To simplify the comparison, normalize both the
results of both calculations to the continuum level, i.e.\ to
$F_{\nu}$ at $\nu \ll \nu_{\mathrm{line}}$ or at $\nu \gg
\nu_{\mathrm{line}}$. Following these steps, you should obtain a
comparison similar to Figure \ref{fig:profile}.
\end{enumerate}
\end{enumerate}
\begin{figure}[h]
\centering
\includegraphics[width=\textwidth]{line_profile}
\caption{P-Cygni Line profile as predicted by \citet{Jeffrey1990} and
calculated by the Monte Carlo simulation with $10^5$ packets.}
\label{fig:profile}
\end{figure}
\bibliography{astrouli.bib}
\bibliographystyle{aa}
\end{document}