Here, I introduce photon interations with matter the way I believe most accessible and understandable. The various interaction types are competing possibilities, so they should be introduced side by side — rather than introduced under separate headings. It is important to appreciate that a single photon interacting with matter typically gives rise to a sea of progeny (or secondary) particles of different type and energy — chances are we will see photoelectric absorption, Compton scattering, Rayleigh scattering and pair production many times over. That is, from a single photon only.
The slides will also demonstrate all four ways of expression interaction probability: cross section (barns/atom), mass attenuation coefficient (mu per rho), linear attenuation coefficient (mu) and mean free path (lambda). The units are convertible to and fro each other. Numerical work examples are given. Differences in meaning are highlighted.
A guided practical session is given here.
In the slides, photoneutron production (and photonuclear reaction in general) is put into context alongside photoelectric absorption, Compton scattering, Rayleigh scattering and pair production. The two sides are often discussed in isolation by textbooks; sometimes given attention by separate communnities. Yet, when a photon enters a material, it stands a chance to undergo one of the possibilities: photoelectric absorption, Compton scattering, Rayleigh scattering, pair production or photonuclear reaction -- if the photon exceeds the threshold.
(gamma,neutron) production thresholds are not that low after all. It is 2.22 MeV for 2H, 1.67 MeV for 9Be, 4.95 MeV for 13C, 10.55 MeV for 14N. The list goes on. We can either calculate the thresholds (Q values) ourselves or look them up from Brookhaven's QCalc.