Astronomy and astrophysics Definition
Kompaneets equation
Builds on Inverse Compton scatteringThomson scatteringFokker–Planck equation
Definition
Consider an isotropic, spatially homogeneous photon gas scattering off a thermal gas of free electrons with number density and temperature . Let be the Boltzmann constant, the electron mass, the speed of light, the Planck constant and the photon frequency. Assume and . Let and let be the photon occupation number at time . The Kompaneets equation is where is the Thomson cross-section.
Remarks
Example: the Bose–Einstein distribution with a constant is a stationary solution, since , so the bracket vanishes. Non-example: a Planck distribution at a temperature different from , with and , is not stationary: the bracket does not vanish and the spectrum evolves. The three terms in the bracket describe diffusion in energy, recoil and induced scattering. The equation conserves the photon number , since the right side is times a derivative and the flux vanishes at and for regular solutions. One often writes it in terms of the Compton parameter with .
Reading path
To understand this page from the ground up, read these 4 pages in order. The foundations come first.
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- no evidence level
- Fokker–Planck equation concept
- Inverse Compton scattering concept
- Thomson scattering concept
- Kompaneets equation definition
Further reading
About this page
| Tag | 1W0K0JXZRJ |
|---|---|
| URI | m2://1W0K0JXZRJ |
| Kind | definition |
| Writing | W0 stub |
| MSC | 85A25, 35Q85, 82C40 |
| Defines | Kompaneets equation |
| Uses | Inverse Compton scattering, Thomson scattering, Fokker–Planck equation |
| Changed | 3 November 2026 |
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