Characteristic radiation

Last revised by Candace Makeda Moore on 03 Dec 2020

Characteristic radiation is a type of energy emission relevant for X-ray production. This energy emission happens when a fast-moving electron collides with a K-shell electron, the electron in the K-shell is ejected (provided the energy of the incident electron is greater than the binding energy of K-shell electron) leaving behind a 'hole'. An outer shell electron fills this hole (from the L-shell, M-shell, etc. ) with an emission of a single x-ray photon, sometimes called a characteristic photon, with an energy level equivalent to the energy level difference between the outer and inner shell electron involved in the transition.

As opposed to the continuous spectrum of bremsstrahlung radiation, characteristic radiation is represented by a line spectrum. As each element has a specific arrangement of electrons at discrete energy level, then it can be appreciated that the radiation produced from such interactions is 'characteristic' of the element involved.

For example, in a tungsten target electron transitions from the L-shell to the K-shell produce x-rays photons of 57.98 and 59.32 keV. The two energy levels are as a result of the Pauli exclusion principle which states that no two particles of half-integer spin (such as electrons) in an atom can occupy exactly the same energy state at the same time; therefore the K-shell represents two different energy states, the L-shell eight states and so on.

When an electron falls (cascades) from the L-shell to the K-shell, the x-ray emitted is called a K-alpha x-ray. Similarly, when an electron falls from the M-shell to the K-shell, the x-ray emitted is called a K-beta x-ray1. However, it is possible to have M-L transitions and so on but their likelihood is so low they can be safely ignored.

Each element differs in nuclear binding energies, and characteristic radiation depends on the binding energy of particular element.

Characteristic radiation never exists in isolation and the line spectra is usually superimposed on the continuous spectra of bremsstrahlung radiation.

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Cases and figures

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