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CERN Program Library Long Writeup W5013 - CERNLIB ...

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where<br />

N<br />

Z(Z i )<br />

A(A i )<br />

ρ<br />

σ<br />

Avogadro’s number<br />

atomic number (of i th component) of the medium<br />

atomic mass (of i th component) of the medium<br />

density<br />

cross-section<br />

n i proportion by number of the i th element in the material (n i = Wp i /A i<br />

where p i is the corresponding proportion by weight and W is the molecular<br />

weight).<br />

The binding energy of the inner shells has been parameterised as:<br />

E i (Z) =Z 2 (A i + B i Z + C i Z 2 + D i Z 3 ) MeV (7)<br />

where, i = K, L I ,L II and the constants A i ,B i ,C i and D i are tabulated below.<br />

A B C D<br />

K 0.66644·10 −5 0.22077·10 −6 -0.32552·10 −8 0.18199·10 −10<br />

L I -0.29179·10 −6 0.87983·10 −7 -0.12589·10 −8 0.69602·10 −11<br />

L II -0.68606·10 −6 0.10078·10 −6 -0.14496·10 −8 0.78809·10 −11<br />

The photoelectric effect total cross-section has been parameterised as:<br />

p 1 /Z + p 2 X + p 3 + p 4 Z + p 5 /X + p 6 Z<br />

⎧⎪ 2<br />

+ p 7 Z/X + p 8 /X 2 + p 9 Z 3 if E>E k (Z)<br />

⎨<br />

σ(Z, E) =Z α X β + p 10 Z 2 /X + p 11 Z/X 2 + p 12 /X 3 (8)<br />

p 13 /Z + p 14 X + p 15 if E LI

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