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THE EGS5 CODE SYSTEM

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Figure 2.5: Feynman diagram for single photon e + e − annihilation.<br />

is assumed to have energy ˘k = m. The gamma angular distribution is taken to be isotropic the<br />

photons moving in opposite directions.<br />

It should be noted that a positron may annihilate and give off only one photon via the process<br />

shown in Figure 2.5. Messel and Crawford[103] make the point that the ratio of one photon<br />

annihilation to two photon annihilation is small until higher energies are reached, at which point<br />

the absolute value of the cross section is small. Thus, EGS ignores one photon positron annihilation.<br />

Note that it is also possible to have annihilation accompanied by three or more photons, but these<br />

interactions are even less likely than one photon annihilation and are not considered in EGS.<br />

2.13 Continuous Electron Energy Loss<br />

Recall the distinction made earlier between collisions contributing to discrete and to continuous<br />

energy losses in electron and positron scattering. In discrete collisions, secondary particles with<br />

energies above their cutoff energies are created and subsequently transported. Continuous energy<br />

losses result from interactions in which the energy transfered to the secondary particles is below<br />

the discrete transport energy thresholds. The resulting secondary particles, which are either soft<br />

bremsstrahlung photons or low energy atomic electrons. The mean total energy loss per unit length<br />

in these continuous loss collisions is thus given by<br />

−<br />

( ) dE±<br />

dx Total<br />

Continuous<br />

= −<br />

( ) dE±<br />

dx Soft<br />

Bremsstrahlung<br />

−<br />

( ) dE±<br />

dx Sub-Cutoff<br />

Atomic Electrons<br />

(2.253)<br />

where ± denotes positive or negative electrons. The first term on the right-hand side of Equation<br />

2.253 is the same for electrons and positrons (to the accuracy with which we treat bremsstrahlung)<br />

and is given by Equation 2.148.<br />

The second term may be expressed as the integral of the differential cross section for transferring<br />

a specified amount of energy, T , to an atomic electron, times the amount of the energy transfer<br />

73

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