Math 2.0

Astronomy and astrophysics Definition

Bremsstrahlung

Builds on Electromagnetic radiation

Definition

Let a charged particle move past another charged particle and be accelerated by its Coulomb field. Assume the two are not bound before or after the encounter. Bremsstrahlung is the electromagnetic radiation emitted by the particle because of this acceleration. Thermal bremsstrahlung is the bremsstrahlung of a gas of free electrons and ions. In it the electrons have a Maxwell–Boltzmann distribution of velocities at a temperature TT.

Remarks

Example: let an electron of charge −e-e and mass mem_e pass an ion of charge ZeZe at distance bb. Near closest approach its acceleration has size about Ze2/(4πε0meb2)Z e^2 / (4\pi\varepsilon_0 m_e b^2), where ε0\varepsilon_0 is the vacuum permittivity. By the Larmor formula it radiates power proportional to the square of this acceleration. Non-example: radiation from an electron captured by an ion into a bound state is recombination radiation (free-bound), not bremsstrahlung, because the electron is bound after the event. Consider thermal bremsstrahlung of electrons of density nen_e and ions of density nin_i and charge ZeZe. Its emissivity per unit frequency is proportional to Z2neniT−1/2e−hν/(kBT)Z^2 n_e n_i T^{-1/2} e^{-h\nu/(k_B T)} times a slowly varying Gaunt factor. Its total power per unit volume is proportional to Z2neniT1/2Z^2 n_e n_i T^{1/2}. Collisions between identical particles, such as electron–electron, give no dipole radiation, so in a non-relativistic plasma electron–ion encounters dominate.

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Further reading

  1. Web https://en.wikipedia.org/wiki/Bremsstrahlung
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Kinddefinition
WritingW0 stub
MSC85A25, 78A40, 78A35
DefinesBremsstrahlung
UsesElectromagnetic radiation
Changed3 November 2026

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