Transition Cross Sections
In laser physics, transition cross sections are used to quantify the likelihood of optically induced transition events, e.g. of absorption or stimulated emission. For a laser ion in a certain electronic state, the rate of transitions (in events per second) is given as the corresponding cross section times the photon flux (in photons per square meter and second):
Absorption and Gain Coefficient
If absorbing atoms or ions with an absorption cross section σabs are distributed with a number density N in a medium, this leads to an intensity absorption coefficient α of the medium which is the product of N and σabs. (For fibers or other waveguides with an undoped cladding, it may be necessary to include also an overlap factor Γ.) In an analogous fashion, the gain coefficient for atoms or ions with a given emission cross section σem can be calculated.
Transition Cross Sections of Laser Gain Media
For a laser gain medium, the most relevant cross sections are the absorption and emission cross sections at the pump and laser wavelengths. In many cases, there is only an absorption cross section for the pump wavelength and an emission cross section (also called laser cross section) for the laser wavelengths. The other transition cross sections are effectively zero, because the lower laser level is quickly depopulated. For such a four-level gain medium, the threshold pump power is inversely proportional to the product of emission cross section and upper-state lifetime. The cross sections influence not only the achievable pump absorption and gain, but also the saturation behavior and the rates of spontaneous transition processes. If there is a non-zero absorption cross section at the laser wavelength, this causes reabsorption (→ four-level and three-level laser gain media).
In solid-state gain media, laser transitions normally involve different Stark levels of the upper and lower electronic levels (or more precisely, upper and lower Stark manifolds). These sublevel-transitions are spectrally overlapping, so that they are hard to distinguish (at least at room temperature). Depending on the exact wavelength, transitions between different Stark levels contribute with varying degrees. A convenient technique for laser modeling is therefore to use so-called effective transition cross sections, which are a kind of averages of the cross sections of different sublevel transitions, with weight factors depending on population densities in thermal equilibrium (which implies that they are intrinsically temperature-dependent). Effective transition cross sections can directly be obtained from spectroscopic measurements without resolving the different sublevel transitions (which would be difficult e.g. in the case of doped glasses). Also, they can be directly used in laser models.
Typical values of absorption and emission cross sections of laser crystals are in the range 10−20–10−18 cm2. Single ions in glasses exhibit similar values, but due to inhomogeneous broadening, the average cross sections of the ions in a glass are often substantially smaller – often several times or even by an order of magnitude. For gain media operating on allowed transitions (rather than forbidden transitions), such as laser dyes or semiconductors, the cross sections are much higher.
Gain media with high emission cross sections and/or broad gain bandwidth tend to have a low upper-state lifetime because of strong spontaneous emission (→ radiative lifetime). Even though quantum noise processes determine the rate of spontaneous emission, that rate is also proportional to the emission cross section and bandwidth. See the article on radiative lifetime for more details.
Measurement of Transition Cross Sections
Absorption cross sections for transitions starting at the ground-state manifold are often obtained from absorption spectra, measured e.g. with a white light source, if the number density (concentration) of the ions is known.
The spectral profile of emission cross sections can be obtained from fluorescence spectra, if no reabsorption modifies the spectral shape and there is no spectral overlap of different fluorescent transitions. Absolute values of emission cross sections can be calculated with the reciprocity method, e.g. via the Füchtbauer–Ladenburg equation. The McCumber relation  can also be useful. Emission cross sections e.g. for rare earth ions can also be estimated from absorption cross sections using Judd–Ofelt theory.
Excited-state absorption (e.g. from the upper laser level) is also characterized with cross sections. These are more difficult to measure than those for ground-state absorption, because (a) it is necessary to populate at least partially the corresponding starting level during the measurement, (b) it can be difficult to determine the fraction of ions in that level, and (c) the measured absorption may be modified by absorption or stimulated emission from other levels, which are also populated.
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See also: stimulated emission, spontaneous emission, laser transitions, radiative lifetime, effective transition cross sections, Giles parameters, McCumber theory, doping concentration
and other articles in the categories lasers, physical foundations