In physics, the radiation length is a characteristic of a material, related to the energy loss of high energy, electromagnetic-interacting particles with it.
In materials of high atomic number (e.g. W, U, Pu) the electrons of energies >~10 MeV predominantly lose energy by bremsstrahlung, and high-energy photons by e+e− pair production. The characteristic amount of matter traversed for these related interactions is called the radiation length X0, usually measured in g·cm−2. It is both the mean distance over which a high-energy electron loses all but 1⁄e of its energy by bremsstrahlung, and 7⁄9 of the mean free path for pair production by a high-energy photon. It is also the appropriate scale length for describing high-energy electromagnetic cascades.
The radiation length for a given material consisting of a single type of nuclei can be approximated by the following expression:
Or exactly using:
While this definition may also be used for other electromagnetic interacting particles beyond leptons and photons, the presence of the stronger hadronic and nuclear interaction makes it a far less interesting characterisation of the material; the nuclear collision length and nuclear interaction length are more relevant.
- Mean free path
- Attenuation length
- Attenuation coefficient
- Range (particle radiation)
- Stopping power (particle radiation)
- Electron energy loss spectroscopy
- Eidelman, S. Review of Particle Physics.
- Conway, J. The LHC Experiments.
- "AtomicNuclearProperties on the Particle Data Group".
- S. Eidelman et al. (2004). "Review of particle physics". Phys. Lett. B 592. (http://pdg.lbl.gov/)
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