PENELOPE 2003 - OECD Nuclear Energy Agency
PENELOPE 2003 - OECD Nuclear Energy Agency
PENELOPE 2003 - OECD Nuclear Energy Agency
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2.3. Incoherent (Compton) scattering 45<br />
(i) Generate ν from π(ν) by using eq. (2.31).<br />
(ii) Generate a random number ξ.<br />
(iii) If ξg(0) > g(ν), go to step (i).<br />
(iv) Deliver cos θ e = 1 − ν.<br />
The efficiency of this algorithm is ∼ 0.33 at low energies and increases slowly with E e ;<br />
for E e = 1 MeV, the efficiency is 0.4. As photoelectric absorption occurs at most once<br />
in each photon history, this small sampling efficiency does not slow down the simulation<br />
significantly.<br />
2.3 Incoherent (Compton) scattering<br />
In Compton scattering, a photon of energy E interacts with an atomic electron, which<br />
absorbs it and re-emits a secondary (Compton) photon of energy E ′ in the direction Ω =<br />
(θ, φ) relative to the direction of the original photon. In penelope, Compton scattering<br />
events are described by means of the cross section obtained from the relativistic impulse<br />
approximation (Ribberfors, 1983). Contributions from different atomic electron shells<br />
are considered separately. After a Compton interaction with the i-th shell, the active<br />
target electron is ejected to a free state with kinetic energy E e = E −E ′ −U i > 0, where<br />
U i is the ionization energy of the considered shell, and the residual atom is left in an<br />
excited state with a vacancy in the i-th shell.<br />
In the case of scattering by free electrons at rest, the conservation of energy and momentum<br />
implies the following relation between the energy E ′ of the scattered (Compton)<br />
photon and the scattering angle θ [cf. eq. (A.19)]<br />
E ′ ≡<br />
E<br />
1 + κ(1 − cos θ) ≡ E C, (2.32)<br />
where κ = E/m e c 2 , as before. The DCS for Compton scattering by a free electron at<br />
rest is given by the familiar Klein-Nishina formula,<br />
dσ KN<br />
Co<br />
dΩ<br />
= r2 e<br />
2<br />
( EC<br />
E<br />
) 2 ( EC<br />
E + E )<br />
− sin 2 θ . (2.33)<br />
E C<br />
Although this simple DCS was generally used in old Monte Carlo transport codes, it<br />
represents only a rough approximation for the Compton interactions of photons with<br />
atoms. In reality, atomic electrons are not at rest, but move with a certain momentum<br />
distribution, which gives rise to the so-called Doppler broadening of the Compton line.<br />
Moreover, transitions of bound electrons are allowed only if the energy transfer E − E ′<br />
is larger than the ionization energy U i of the active shell (binding effect).<br />
The impulse approximation accounts for Doppler broadening and binding effects<br />
in a natural, and relatively simple, way. The DCS is obtained by considering that