| 1 | \section{Compton Scattering}
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| 2 |
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| 3 | \subsection{Total Cross Section}
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| 4 |
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| 5 | The total cross section for the Compton scattering process
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| 6 | %(also called incoherent
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| 7 | %scattering~\footnote{Incoherent scattering is usually described as an interaction
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| 8 | %between a photon and the outer most, most loosely bound electrons.})
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| 9 | is determined from the data as described in section \ref{subsubsigmatot}.
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| 10 |
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| 11 | \subsection{Sampling of the Final State}
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| 12 |
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| 13 | For low energy incident photons, the simulation of the Compton scattering
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| 14 | process is performed according to the same procedure used for the
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| 15 | ``standard" Compton scattering simulation, with the addition that
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| 16 | Hubbel's atomic form factor~\cite{ce-hubbel} or scattering function, $SF$,
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| 17 | is taken into account. The angular and energy distribution of the
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| 18 | incoherently scattered photon is then given by the product of the
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| 19 | Klein-Nishina formula $\Phi(\epsilon)$ and the scattering function,
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| 20 | $SF(q)$~\cite{ce-reda}
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| 21 | \begin{equation}
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| 22 | P(\epsilon, q ) = \Phi( \epsilon ) \times SF(q) .
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| 23 | \end{equation}
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| 24 | $\epsilon$ is the ratio of the scattered photon energy $E'$, and the
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| 25 | incident photon energy $E$. The momentum transfer is given by
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| 26 | $q = E \times \sin^2(\theta/2)$, where $\theta$ is the polar angle of the
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| 27 | scattered photon with respect to the direction of the parent photon.
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| 28 | $\Phi(\epsilon)$ is given by
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| 29 | \begin{equation}
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| 30 | \Phi(\epsilon) \cong {[{1\over\epsilon} + \epsilon] [1-{\epsilon \over{1+\epsilon^2}} sin^2\theta]} .
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| 31 | \end{equation}
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| 32 |
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| 33 | The effect of the scattering function becomes significant at low energies,
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| 34 | especially in suppressing forward scattering~\cite{ce-reda}.
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| 35 |
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| 36 | The sampling method of the final state is
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| 37 | based on composition and rejection Monte Carlo methods \cite{ce-butch,ce-messel,ce-egs4},
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| 38 | with the $SF$ function included in the rejection function
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| 39 | \begin{equation}\label{en-samp-comp}
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| 40 | g(\epsilon) = \left[1-\frac{\epsilon}{1+\epsilon^2} \sin^2\theta \right] \times SF(q) ,
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| 41 | \end{equation}
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| 42 | with $0<g(\epsilon)<Z$.
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| 43 | Values of the scattering functions at each momentum transfer, $q$, are
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| 44 | obtained by interpolating the evaluated data for the corresponding atomic
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| 45 | number, $Z$.
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| 46 |
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| 47 | The polar angle $\theta$ is deduced from the sampled $\epsilon$ value.
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| 48 | In the azimuthal direction, the angular distributions of both the scattered
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| 49 | photon and the recoil electron are considered to be
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| 50 | isotropic~\cite{ce-stepanek}.
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| 51 |
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| 52 | Since the incoherent scattering occurs mainly on the outermost electronic
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| 53 | subshells, the binding energies can be neglected, as stated in
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| 54 | reference~\cite{ce-stepanek}. The momentum vector of the scattered photon,
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| 55 | $\overrightarrow{P'_{\gamma}}$,
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| 56 | is transformed into the {\tt World} coordinate system.
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| 57 | The kinetic energy and momentum of the recoil electron are then
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| 58 | \begin{eqnarray*}
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| 59 | T_{el} & = & E - E' \\
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| 60 | \overrightarrow{P_{el}} & = &
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| 61 | \overrightarrow{P_{\gamma}} - \overrightarrow{P'_{\gamma}} .
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| 62 | \end{eqnarray*}
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| 63 |
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| 64 |
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| 65 | \subsection{Status of the document}
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| 66 |
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| 67 | \noindent
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| 68 | 30.09.1999 created by Alessandra Forti\\
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| 69 | 07.02.2000 modified by V\'eronique Lef\'ebure\\
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| 70 | 08.03.2000 reviewed by Petteri Nieminen and Maria Grazia Pia\\
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| 71 | 26.01.2003 minor re-write by D.H. Wright
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| 72 |
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| 73 | \begin{latexonly}
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| 74 |
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| 75 | \begin{thebibliography}{99}
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| 76 | \bibitem{ce-hubbel}
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| 77 | ``Summary of Existing Information on the Incoherent Scattering of Photons
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| 78 | particularly on the Validity of the Use of the Incoherent Scattering
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| 79 | Function",
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| 80 | Radiat. Phys. Chem. Vol. 50, No 1, pp 113-124 (1997)
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| 81 | \bibitem{ce-reda}
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| 82 | ``A simple model of photon transport",
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| 83 | D.E. Cullen, Nucl. Instr. Meth. in Phys. Res. B 101(1995)499-510
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| 84 | \bibitem{ce-butch} J.C. Butcher and H. Messel.
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| 85 | {\em Nucl. Phys. 20} 15 (1960)
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| 86 | \bibitem{ce-messel} H. Messel and D. Crawford.
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| 87 | {\em Electron-Photon shower distribution, Pergamon Press} (1970)
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| 88 | \bibitem{ce-egs4} R. Ford and W. Nelson.
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| 89 | {\em SLAC-265, UC-32} (1985)
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| 90 | \bibitem{ce-stepanek}
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| 91 | ``New Photon, Positron and Electron Interaction Data for Geant in Energy
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| 92 | Range from 1 eV to 10 TeV",
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| 93 | J. Stepanek, Draft to be submitted for publication
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| 94 |
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| 95 | \end{thebibliography}
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| 96 |
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| 97 | \end{latexonly}
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| 98 |
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| 99 | \begin{htmlonly}
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| 100 |
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| 101 | \subsection{Bibliography}
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| 102 |
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| 103 | \begin{enumerate}
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| 104 | \item
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| 105 | ``Summary of Existing Information on the Incoherent Scattering of Photons
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| 106 | particularly on the Validity of the Use of the Incoherent Scattering
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| 107 | Function",
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| 108 | Radiat. Phys. Chem. Vol. 50, No 1, pp 113-124 (1997)
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| 109 | \item
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| 110 | ``A simple model of photon transport",
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| 111 | D.E. Cullen, Nucl. Instr. Meth. in Phys. Res. B 101(1995)499-510
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| 112 | \item J.C. Butcher and H. Messel.
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| 113 | {\em Nucl. Phys. 20} 15 (1960)
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| 114 | \item H. Messel and D. Crawford.
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| 115 | {\em Electron-Photon shower distribution, Pergamon Press} (1970)
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| 116 | \item R. Ford and W. Nelson.
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| 117 | {\em SLAC-265, UC-32} (1985)
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| 118 | \item
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| 119 | ``New Photon, Positron and Electron Interaction Data for Geant in Energy
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| 120 | Range from 1 eV to 10 TeV",
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| 121 | J. Stepanek, Draft to be submitted for publication
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| 122 |
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| 123 | \end{enumerate}
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| 124 |
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| 125 | \end{htmlonly}
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