Astrophysics (Index)About

bremsstrahlung

(breaking radiation, free-free radiation)
(photon emission when a charged particle is decelerated)

Bremsstrahlung (braking radiation) is electromagnetic radiation produced when a charged particle decelerates, when its course is changed by another charged particle. A photon is emitted that balances the energy equation. The resulting radiation emission (from a gas/plasma) has a continuous spectrum (continuum emission), as opposed, for example, to emission lines. It is also called free-free radiation, expressing the point that its production does not involve an electron bound, before or afterward, to an atom. The term electron-ion bremsstrahlung (e-ion bremsstrahlung) refers to bremsstrahlung caused by a free electron encounter with an ion and electron-electron bremsstrahlung (e-e bremsstrahlung) is that between two electrons. Other types of generation include bremsstrahlung induced during beta decay, and bremsstrahlung due to interaction between an atom's orbiting (bound) electron and a passing charged particle.

An astronomical source of bremsstrahlung is the intracluster medium associated with a galaxy clusters.

The reverse of bremsstrahlung radiation is also possible, called free-free absorption or inverse bremsstrahlung, where an electron and another particle interact and a photon is absorbed. Free-free absorption occurs in HII regions, affecting their spectrum.


(EMR)
Further reading:
http://en.wikipedia.org/wiki/Bremsstrahlung

Referenced by pages:
anomalous microwave emission (AME)
continuum emission
electron scattering
Kramers opacity law
microwave
non-thermal emission
spectral index (α)
synchrotron radiation
thermal bremsstrahlung

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