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1\section[Photoabsorption cross section at low energies]
2{Photoabsorption Cross Section at Low Energies} \label{secsandia}
3
4\subsection{Method}
5
6The photoabsorption cross section, $\sigma_{\gamma}(\omega)$, where $\omega$ 
7is the photon energy, is used in Geant4 for the description of the
8photo-electric effect, X-ray transportation and ionization effects in very
9thin absorbers.  As mentioned in the discussion of photoabsorption
10ionization (see section \ref{secpai}), it is convenient to represent the
11cross section as a polynomial in $\omega^{-1}$ 
12\cite{sandia.bigg} :
13\begin{equation}
14\sigma_{\gamma}(\omega) = \sum_{k=1}^{4}a_{k}^{(i)}\omega^{-k} .
15\end{equation} \\
16
17\noindent
18Using cross sections from the original Sandia data tables, calculations of
19primary ionization and energy loss distributions produced by relativistic
20charged particles in gaseous detectors show clear disagreement with
21experimental data, especially for gas mixtures which include xenon. \\
22
23\noindent
24Therefore a special investigation was performed \cite{sandia.grich} by
25fitting the coefficients $a_{k}^{(i)}$ to modern data from synchrotron
26radiation experiments in the energy range of $ 10 - 50 \ eV$.  The fits
27were performed for elements typically used in detector gas mixtures:
28hydrogen, fluorine, carbon, nitrogen and oxygen.  Parameters for these
29elements were extracted from data on molecular gases such as $N_2$, $O_2$,
30$CO_2$, $CH_4$, and $CF_4$ \cite{sandia.lee73, sandia.lee77}.  Parameters
31for the noble gases were found using data given in the tables
32\cite{sandia.marr, sandia.west}.
33
34\subsection{Status of  this document}
3518.11.98 created by V. Grichine \\
3610.05.02 re-written by D.H. Wright \\
37
38\begin{latexonly}
39
40\begin{thebibliography}{99}
41\bibitem{sandia.bigg} Biggs F., and Lighthill R.,
42{Preprint Sandia Laboratory, SAND 87-0070} (1990)
43\bibitem{sandia.grich} Grichine V.M., Kostin A.P., Kotelnikov S.K. et al.,
44{Bulletin of the Lebedev Institute no. 2-3, 34} (1994).
45\bibitem{sandia.lee73} Lee L.C. et al.,
46{J.Q.S.R.T., v. 13, p. 1023} (1973).
47\bibitem{sandia.lee77} Lee L.C. et al.,
48{Journ. of Chem. Phys., v. 67, p. 1237} (1977).
49\bibitem{sandia.marr} G.V. Marr and J.B. West,
50{Atom. Data Nucl. Data Tabl., v. 18, p. 497} (1976).
51\bibitem{sandia.west} J.B. West and J. Morton,
52{Atom. Data Nucl. Data Tabl., v. 30, p. 253} (1980).
53\end{thebibliography}
54
55\end{latexonly}
56
57\begin{htmlonly}
58
59\subsection{Bibliography}
60
61\begin{enumerate}
62\item Biggs F., and Lighthill R.,
63{Preprint Sandia Laboratory, SAND 87-0070} (1990)
64\item Grichine V.M., Kostin A.P., Kotelnikov S.K. et al.,
65{Bulletin of the Lebedev Institute no. 2-3, 34} (1994).
66\item Lee L.C. et al.,
67{J.Q.S.R.T., v. 13, p. 1023} (1973).
68\item Lee L.C. et al.,
69{Journ. of Chem. Phys., v. 67, p. 1237} (1977).
70\item G.V. Marr and J.B. West,
71{Atom. Data Nucl. Data Tabl., v. 18, p. 497} (1976).
72\item J.B. West and J. Morton,
73{Atom. Data Nucl. Data Tabl., v. 30, p. 253} (1980).
74\end{enumerate}
75
76\end{htmlonly}
77
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