Kompaneets equation 2026-10-14
The Kompaneets equation describes frequency diffusion of a mean photon occupation number through repeated nonrelativistic Compton scattering. For thermal Electrons, with and , its full homogeneous form is . The drift and stimulated terms permit a thermal stationary spectrum. In the hot-electron limit , with low photon energies, they can be neglected relative to the diffusion term; any fixed linear frequency variable then gives . The quantity is not the frequency-integrated photon number density.
Past exam of the mathematics course of the University of Cambridge 2004 iii Paper 67 3 a Solution Created 2026-10-03 Updated 2026-10-14
In the Maxwell-Boltzmann velocity distribution, each Cartesian component has mean-square velocity . Thus . The original PDF calls this quantity an rms velocity, but the rms speed is its square root. Also, its must mean the dimensionless mean occupation number , since its equilibrium value is a Planck photon distribution; it is not the frequency-integrated photon number density.
Take at a fixed local radiation temperature. Because is proportional to frequency,The hot-electron Kompaneets equation therefore becomesFor traversal length , the Compton y parameter isIt measures electron pressure integrated along the line of sight, or the Thomson scattering optical depth weighted by . In this hot-electron limit the mean fractional energy gain is approximately . The derivation assumes nonrelativistic electrons, Thomson-limit photon energies and . The original PDF uses , as required for ordinary frequency; the converted TeX incorrectly substitutes .
Thermal Sunyaev-Zeldovich effect 2026-10-14
For a Planck photon distribution, the hot-electron Kompaneets equation gives , where . The equivalent thermodynamic temperature perturbation has the displayed form, while the Rayleigh-Jeans law gives . The distortion changes sign at . This first-order expression assumes a small Compton y parameter and nonrelativistic thermal Electrons.