The cross-sections from [] have been used to calculate
data points for () and (
).
These have been parameterised as:
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where is the maximum possible value of the photon energy. The functions ( ) are polynomials:
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A least-squares fit has been performed on more than 2000 points for Z = 1, 6, 13, 26, 50, 82, 92 and 1 GeV 10 TeV and 10 keV . The resulting values of , , , , , and
can be found in the DATA statements within the functions
GBRSGM and GBRELM which
compute formulae () and (
) respectively.
The accuracy of the fit can be estimated as:
The contribution of the bremsstrahlung to the total energy loss of the muons is less than 1% for 5 GeV.
When
, a parameterisation different from
() can be used for the total muon energy loss due to
bremsstrahlung:
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where
.
The accuracy of the formula () for
is rather good:
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