The photoionization processes are photoeffect (incident photon absorbed) and Compton scattering (incident photon scattered). Photoeffect dominates the total cross section at lower photon energies and its relative contribution in photon atom interaction decreases as photon energy increases. For a He-like system, at energies for which the incoming photon momentum k is comparable to the average momentum of the bound electrons pav (of a two electron atom or ion in its ground state), photoeffect and Compton scattering are comparable. For higher energies Compton scattering dominates. In the case of helium Compton scattering dominates above, roughly, 6.5 keV.
The simplest observable, for both experimental and theoretical treatment of the correlation effects, has been the ratio between probabilities for double and single photoionization. This ratio is nonzero because of electron-electron correlation; its value depends on incident photon energy. Also, the value depends on the process under consideration. Therefore we talk about the Compton double to single ionization ratio RC and the photoeffect ionization ratio RP. The energy dependence of these observables, and particularly their high energy limits, are subjects of extensive studies. In the last several years significant progress has been achieved [1]. However, the relatively large disagreements in theoretical predictions as well as in experimental data indicate that we still do not understand all relevant aspects of the processes which are involved in determining the ratio for the double to single ionization for both Compton scattering and photoeffect.
As we will see, much understanding of these processes can be obtained within the shake-off approximation, i.e. a sudden approximation. By shake-off approximation we mean the assumption that the final state electron-electron interaction can be neglected, and that one electron scatters the high energy photon and accepts almost all momentum transfer [2].