| 1 | \section{Rayleigh Scattering}
|
|---|
| 2 |
|
|---|
| 3 | \subsection{Total Cross Section}
|
|---|
| 4 | The total cross section for the Rayleigh scattering process
|
|---|
| 5 | %(also called coherent scattering~\footnote{Coherent scattering
|
|---|
| 6 | %is usually described as an interaction
|
|---|
| 7 | %between a photon and the inner most, most tightly bound electrons of an atom.})
|
|---|
| 8 | is determined from the data as described in section \ref{subsubsigmatot}.
|
|---|
| 9 |
|
|---|
| 10 | \subsection{Sampling of the Final State}
|
|---|
| 11 |
|
|---|
| 12 | The coherent scattered photon angle $\theta$ is sampled according to the
|
|---|
| 13 | distribution obtained from the product of the Rayleigh formula $(1+\cos^2\theta)\sin\theta $ and the square of Hubbel's form factor
|
|---|
| 14 | $FF^2(q)$~\cite{re-hubbel2}~\cite{re-reda}
|
|---|
| 15 | \begin{equation}
|
|---|
| 16 | \Phi(E, \theta) = [ 1+\cos^2 \theta] \sin \theta \times FF^2(q) ,
|
|---|
| 17 | \end{equation}
|
|---|
| 18 | where $q = 2 E \sin(\theta/2)$ is the momentum transfer.
|
|---|
| 19 |
|
|---|
| 20 | Form factors introduce a dependency on the initial energy $E$ of the photon
|
|---|
| 21 | that is not taken into account in the Rayleigh formula. At low energies,
|
|---|
| 22 | form factors are isotropic and do not affect angular distribution, while at
|
|---|
| 23 | high energies they are forward peaked.
|
|---|
| 24 |
|
|---|
| 25 | The sampling procedure is as follows~\cite{re-stepanek}:
|
|---|
| 26 | \begin{enumerate}
|
|---|
| 27 | \item $cos\theta$ is chosen from a uniform distribution between -1 and 1
|
|---|
| 28 | \item the form factor $FF$ is extracted from the data table for the
|
|---|
| 29 | considered element, using logarithmic data interpolation,
|
|---|
| 30 | for $q = 2 E \cdot\sin(\theta/2)$
|
|---|
| 31 | \item if the value obtained for $\Phi(E, \theta)$ is larger than a random
|
|---|
| 32 | number uniformly distributed between 0 and $Z^2$, the procedure is repeated
|
|---|
| 33 | from step 1, otherwise $\theta$ is taken as the photon scattering angle
|
|---|
| 34 | with respect to its incident direction.
|
|---|
| 35 | \item the azimuthal direction of the scattered photon is chosen at random.
|
|---|
| 36 | \end{enumerate}
|
|---|
| 37 |
|
|---|
| 38 |
|
|---|
| 39 | \subsection{Status of this document}
|
|---|
| 40 |
|
|---|
| 41 | \noindent
|
|---|
| 42 | 30.09.1999 created by Alessandra Forti\\
|
|---|
| 43 | 07.02.2000 modified by V\'eronique Lef\'ebure\\
|
|---|
| 44 | 08.03.2000 reviewed by Petteri Nieminen and Maria Grazia Pia\\
|
|---|
| 45 | 10.06.2002 modified by Francesco Longo and Gerardo Depaola\\
|
|---|
| 46 | 26.01.2003 minor re-write and correction of equations by D.H. Wright
|
|---|
| 47 |
|
|---|
| 48 | \begin{latexonly}
|
|---|
| 49 |
|
|---|
| 50 | \begin{thebibliography}{99}
|
|---|
| 51 | \bibitem{re-hubbel2}
|
|---|
| 52 | "Relativistic Atom Form Factors and Photon Coherent Scattering Cross Sections",
|
|---|
| 53 | J.H. Hubbell et al., J.Phys.Chem.Ref.Data, 8,69(1979)
|
|---|
| 54 | \bibitem{re-reda}
|
|---|
| 55 | "A simple model of photon transport",
|
|---|
| 56 | D.E. Cullen, Nucl. Instr. Meth. in Phys. Res. B 101(1995)499-510
|
|---|
| 57 | \bibitem{re-stepanek}
|
|---|
| 58 | "New Photon, Positron and Electron Interaction Data for Geant in Energy Range
|
|---|
| 59 | from 1 eV to 10 TeV",
|
|---|
| 60 | J. Stepanek, Draft to be submitted for publication
|
|---|
| 61 | \end{thebibliography}
|
|---|
| 62 |
|
|---|
| 63 | \end{latexonly}
|
|---|
| 64 |
|
|---|
| 65 | \begin{htmlonly}
|
|---|
| 66 |
|
|---|
| 67 | \subsection{Bibliography}
|
|---|
| 68 |
|
|---|
| 69 | \begin{enumerate}
|
|---|
| 70 | \item
|
|---|
| 71 | "Relativistic Atom Form Factors and Photon Coherent Scattering Cross
|
|---|
| 72 | Sections", J.H. Hubbell et al., J.Phys.Chem.Ref.Data, 8,69(1979)
|
|---|
| 73 | \item
|
|---|
| 74 | "A simple model of photon transport",
|
|---|
| 75 | D.E. Cullen, Nucl. Instr. Meth. in Phys. Res. B 101(1995)499-510
|
|---|
| 76 | \item
|
|---|
| 77 | "New Photon, Positron and Electron Interaction Data for Geant in Energy
|
|---|
| 78 | Range from 1 eV to 10 TeV",
|
|---|
| 79 | J. Stepanek, Draft to be submitted for publication
|
|---|
| 80 | \end{enumerate}
|
|---|
| 81 |
|
|---|
| 82 | \end{htmlonly}
|
|---|