X-ray fluorescence (XRF) is the phenomenon where a material is exposed to X-rays of high energy, and as the X-ray (or photon) strikes an atom (or a molecule) in the sample, energy is absorbed by the atom. If the energy is high enough, a core electron is ejected out of its atomic orbital.
An electron from an outer shell then drops into the unoccupied orbital, to fill the hole left behind. This transition gives off an X-ray of fixed, characteristic energy that can be detected by a fluorescence detector. The energy needed to eject a core electron is characteristic of each element, and so is the energy emitted by the transition. The transition of an L shell electron dropping into the K shell is termed a Kα transition, while an M shell electron dropping into the K shell is a Kβ transition.
When the energy source is a synchrotron, or the X-ray are focussed by a optic, like a polycapillary, the X-ray beam can be very small and very intense, and atomic information on the sub-micrometer scale can be obtained.
Typically the lightest element that can be analysed is beryllium (Z = 4), but due to instrumental limitations and low x-ray yields for the light elements, it is often difficult to quantify elements lighter than sodium (Z = 11).
There are two types of spectrometer:
It is also possible to create a characteristic secondary X-ray emission with other incident radiation to excite the sample:
Atomic physics | Molecular physics | Spectroscopy X-rays
Spectrométrie de fluorescence X | Spettrofotometria XRF | Röntgenfluoreszenzanalyse | Röntgenfluorescentiespectrometrie
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"X-ray fluorescence".
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