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PENELOPE 2003 - OECD Nuclear Energy Agency

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46 Chapter 2. Photon interactions<br />

electrons in the i-th shell move with a momentum distribution ρ i (p). For an electron in<br />

an orbital ψ i (r), ρ i (p) ≡ |ψ i (p)| 2 , where ψ i (p) is the wave function in the momentum<br />

representation. The DCS for Compton scattering by an electron with momentum p<br />

is derived from the Klein-Nishina formula by applying a Lorentz transformation with<br />

velocity v equal to that of the moving target electron. The impulse approximation to<br />

the Compton DCS (per electron) of the considered shell is obtained by averaging over<br />

the momentum distribution ρ i (p).<br />

After some manipulations, the Compton DCS of an electron in the i-th shell can be<br />

expressed as [eq. (21) in Brusa et al., 1996]<br />

d 2 σ Co,i<br />

dE ′ dΩ = r2 e<br />

2<br />

( EC<br />

E<br />

) 2 ( EC<br />

E + E )<br />

− sin 2 θ F (p z ) J i (p z ) dp z<br />

E C dE ′, (2.34)<br />

where r e is the classical electron radius. E C is the energy of the Compton line, defined<br />

by eq. (2.32), i.e. the energy of photons scattered in the direction θ by free electrons at<br />

rest. The momentum transfer vector is given by q ≡ ¯hk − ¯hk ′ , where ¯hk and ¯hk ′ are<br />

the momenta of the incident and scattered photons; its magnitude is<br />

q = 1 c√<br />

E2 + E ′2 − 2EE ′ cos θ. (2.35)<br />

The quantity p z is the projection of the initial momentum p of the electron on the<br />

direction of the scattering vector ¯hk ′ − ¯hk = −q; it is given by 2<br />

or, equivalently,<br />

p z ≡ − p · q<br />

q<br />

= EE′ (1 − cos θ) − m e c 2 (E − E ′ )<br />

c 2 q<br />

p z<br />

m e c = E(E′ − E C )<br />

E C cq<br />

Notice that p z = 0 for E ′ = E C . Moreover,<br />

dp z<br />

= m (<br />

ec E<br />

+<br />

dE ′ cq E C<br />

E cos θ − E′<br />

cq<br />

(2.36)<br />

. (2.37)<br />

)<br />

p z<br />

. (2.38)<br />

m e c<br />

The function J i (p z ) in eq. (2.34) is the one-electron Compton profile of the active<br />

shell, which is defined as<br />

∫ ∫<br />

J i (p z ) ≡ ρ i (p) dp x dp y , (2.39)<br />

where ρ i (p) is the electron momentum distribution. That is, J i (p z ) dp z gives the probability<br />

that the component of the electron momentum in the z-direction is in the interval<br />

(p z , p z + dp z ). Notice that the normalization<br />

∫ ∞<br />

J i (p z ) dp z = 1 (2.40)<br />

−∞<br />

2 The expression (2.36) contains an approximation, the exact relation is obtained by replacing the<br />

electron rest energy m e c 2 in the numerator by the electron initial total energy, √ (m e c 2 ) 2 + (cp) 2 .

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