The mean stopping power for high-energy muons in matter can be described by
(-dE/dx) = a(E) + b(E)E, where a(E) is the electronic stopping power and b
(E) is the energy-scaled contribution from radiative processes-bremsstrahlu
ng, pair production, and photonuclear interactions. a(E) and b(E) are both
slowly varying functions of the muon energy E where radiative effects are i
mportant. Tables of these stopping power contributions and continuous-slowi
ng-down-approximation ranges (which neglect multiple scattering and range s
traggling) are given for a selection of elements, compounds, mixtures, and
biological materials for incident kinetic energies in the range of 10 MeV t
o 100 TeV. Tables of the contributions to b(E) are given for the same mater
ials.