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PENELOPE 2003 - OECD Nuclear Energy Agency

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2.4. Electron-positron pair production 55<br />

electron shell i is sampled with relative probability f i and binding effects are accounted<br />

for by simply rejecting E ′ -values such that E − E ′ < U i .<br />

The azimuthal scattering angle φ of the photon is sampled uniformly in the interval<br />

(0, 2π). We assume that the Compton electron is emitted with energy E e = E − E ′ − U i<br />

in the direction of the momentum transfer vector q = ¯hk − ¯hk ′ , with polar angle θ e and<br />

azimuthal angle φ e = φ + π, relative to the direction of the incident photon. cos θ e is<br />

given by<br />

E − E ′ cos θ<br />

cos θ e = √<br />

E2 + E ′2 − 2EE ′ cos θ . (2.75)<br />

When E ′ = E C , this expression simplifies to<br />

cos θ e = E + m ec 2 (<br />

)<br />

E − E 1/2<br />

C<br />

, (2.76)<br />

E 2m e c 2 + E − E C<br />

which coincides with the result (A.20). Since the active electron shell is known, characteristic<br />

x rays and Auger electrons emitted in the de-excitation of the ionized atom<br />

can also be followed. This is important, for instance, to account for escape peaks in<br />

scintillation or solid state detectors<br />

Table 2.1: Average number n r of random numbers ξ needed to simulate a single incoherent<br />

scattering event for photons with energy E in aluminium, silver and gold.<br />

E (eV) Al Ag Au<br />

10 3 16.6 11.9 13.4<br />

10 4 11.0 11.4 11.5<br />

10 5 9.5 9.8 10.0<br />

10 6 8.2 8.2 8.3<br />

10 7 7.5 7.5 7.5<br />

As a measure of the efficiency of the sampling algorithm, we may consider the average<br />

number n r of random numbers ξ required to simulate an incoherent scattering event.<br />

n r is practically independent of the atomic number and decreases with photon energy<br />

(see table 2.1). The increase of n r at low energies stems from the loss of efficiency<br />

of the algorithm used to sample cos θ. Although the simulation of incoherent events<br />

becomes more laborious as the photon energy decreases, this has only a small influence<br />

on the speed of practical photon transport simulations since low-energy photons interact<br />

predominantly via photoelectric absorption (see fig. 2.10 below).<br />

2.4 Electron-positron pair production<br />

Electron-positron pairs can be created by absorption of a photon in the vicinity of a<br />

massive particle, a nucleus or an electron, which absorbs energy and momentum so that

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