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CERN Program Library Long Writeup W5013 - CERNLIB ...

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∆σ<br />

σ<br />

=<br />

{<br />

12 − 15% for T ≤ 1MeV<br />

≤ 5 − 6% for 1MeV < T ≤ 10TeV<br />

∆E brem<br />

Loss<br />

E brem<br />

Loss<br />

=<br />

⎧<br />

⎪⎨<br />

⎪⎩<br />

10 − 15% for T ≤ 1MeV<br />

5 − 6% for 1MeV < T ≤ 100GeV<br />

10% for 100GeV < T ≤ 10TeV<br />

We have performed a fit to the “data” without the Midgal corrections, too. In this case we used the data of<br />

Seltzer and Berger without any correction for T ≤ 10 GeV and we used the Bethe-Heitler cross-section for<br />

T ≥ 10 GeV. The parameterised forms of the cross-section and energy loss are the same as they were in<br />

the first fit (i.e. (3) and (4)), only the numerical values of the parameters have changed. These values are<br />

in DATA statements in the functions GBRSGE and GBRELE and this second kind of parameterisation can be<br />

activated using the PATCHY switch +USE,BETHE. (The two parameterisations give different results for high<br />

electron energy.)<br />

The energy loss due to soft photon bremsstrahlung is tabulated at initialisation time as a function of the<br />

medium and of the energy by routine GBRELA (see JMATE data structure).<br />

The mean free path for discrete bremsstrahlung is tabuled at initialisation time as a function of the medium<br />

and of the energy by routine GBRSGA (see JMATE data structure).<br />

2.2 Corrections for e − /e + differences<br />

The radiative energy loss for electrons or positrons is:<br />

− 1 ( ) dE ±<br />

= N Avαre<br />

2<br />

ρ dx rad A (T + m)Z2 Φ ± rad (Z, T )<br />

∫<br />

Φ ± rad (Z, T ) = 1<br />

T<br />

αre 2 k dσ±<br />

Z2 (T + m) dk dk<br />

0<br />

Reference [77] says that:<br />

“The differences between the radiative loss of positrons and electrons are considerable and cannot be disregarded.<br />

[...] The ratio of the radiative energy loss for positrons to that for electrons obeys a simple scaling law, [...]<br />

is a function only of the quantity T/Z 2 ”<br />

In other words:<br />

η = Φ+ rad (Z, T )<br />

Φ − rad (Z, T ) = η ( T<br />

Z 2 )<br />

The authors have calculated this function in the range 10 −7 ≤ T Z 2 ≤ 0.5 (here the kinetic energy T is<br />

expressed in MeV). Their data can be fairly accurately reproduced using a parametrisation:<br />

η =<br />

⎧<br />

⎪⎨<br />

⎪⎩<br />

0 if x ≤−8<br />

1<br />

2 + 1 π arctan ( a 1 x + a 3 x 3 + a 5 x 5) if −8

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