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PENELOPE 2003 - OECD Nuclear Energy Agency

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78 Chapter 3. Electron and positron interactions<br />

1 E - 1 2<br />

1 E - 1 3<br />

1 E - 1 4<br />

A u ( Z = 7 9 ) , e −<br />

p a r t i a l w a v e<br />

M W m o d el<br />

1 E - 1 5<br />

dσ el<br />

/dµ (cm 2 )<br />

1 E - 1 6<br />

1 E - 1 7<br />

1 E - 1 8<br />

1 E - 1 9<br />

1 keV<br />

10<br />

10 0<br />

1 E - 20<br />

1 E - 21<br />

10 0 0<br />

1 E - 22<br />

1 E - 6 1 E - 5 1 E - 4 1 E - 3 0.01<br />

µ<br />

0.2 0.4 0.6 0.8 1 .0<br />

Figure 3.4: Partial-wave and MW model DCSs for elastic scattering of electrons by gold<br />

atoms.<br />

Nevertheless, the important fact here is that both DCSs give exactly the same values of<br />

σ el , 〈µ〉 and 〈µ 2 〉.<br />

The information needed to determine the parameters of the MW model reduces to the<br />

characteristic functions σ el (E), σ el,1 (E) and σ el,2 (E). penelope reads these functions<br />

from a precalculated database for electrons and positrons, for the elements Z = 1–92<br />

and for a grid of energies that is dense enough to permit accurate cubic spline loglog<br />

interpolation. This elastic scattering database was generated by using the partialwave<br />

code of Salvat (2000); the atomic electron densities were obtained from the Dirac-<br />

Hartree-Fock code of Desclaux (1975), which correspond to free atoms. Before starting<br />

the simulation, penelope evaluates a table of the parameters A and B, and stores it in<br />

the computer memory. Instead of B, penelope tabulates the quantity B ′ = +B (case<br />

I) and B ′ = −B (case II); this avoids the need to specify the case, which can be inferred<br />

from the sign of B ′ . It is worth noting that A and B ′ are continuous functions of energy<br />

and, therefore, can be rapidly evaluated, for any energy, by interpolation in the stored<br />

table. In case I, 〈µ〉 concides with 〈µ〉 W,A , which is determined by A, eq. (3.22). Fig.<br />

3.5 displays the MW model parameters for aluminium and gold, as representative of<br />

low- and high-Z elements. Notice that at high energies, where the case I model applies,<br />

the strength of the delta contribution increases rapidly with energy, indicating that the<br />

partial-wave DCS is much narrower than the Wentzel distribution.<br />

The MW model is directly applicable to compounds (and mixtures) by using the

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