KnowraThomson scatteringLinked fromLinked fromThe 14 pages that link to Thomson scattering, each with the reason it gives.All 14Broader topic 1Related 9Compared with 4Rayleigh scatteringCompared with: Both involve accelerated charges, but Thomson scattering treats a free charge rather than a bound induced dipole.Compton scatteringCompared with: Unlike Compton scattering, its idealized elastic limit leaves photon wavelength unchanged.Sunyaev–Zel'dovich effectRelated: It describes the basic photon-electron interaction in the usual cluster approximation.Recombination (cosmology)Related: Before recombination, free electrons repeatedly scattered photons through this process.Inverse Compton scatteringRelated: It describes the underlying scattering when photon energies in the electron rest frame are low.Davisson–Germer experimentCompared with: It describes a non-quantum scattering model, unlike the electron diffraction pattern observed here.Cosmic microwave background anisotropyRelated: Scattering by moving electrons generates polarization from anisotropic radiation.Classical electron radiusRelated: Its classical cross section is conventionally expressed using the classical electron radius.Eddington luminosityRelated: For ionized gas, this opacity commonly determines how strongly radiation couples to matter.Stellar opacityRelated: It supplies an important nearly frequency-independent opacity in hot ionized stellar interiors.Plasma diagnosticsBroader topic: Scattered laser light yields local electron properties without inserting a probe.Rutherford scattering experimentsCompared with: This alternative scattering picture differs from deflection by a concentrated nucleus.Laboratory studies of space and astrophysical plasmasRelated: It measures laboratory plasma temperature, density, and flow without relying only on emitted light.Polarization in astronomyRelated: Scattering by electrons generates polarization in sources such as stellar atmospheres and accretion flows.