The partial linear polarization of the cosmic microwave background radiation is the result of this physical process. In deriving this non-relativistic process, the magnetic component of the Lorentz force is neglected, and the relevant particles are modeled as being in a damped harmonic oscillator. I
The partial linear polarization of the cosmic microwave background radiation is the result of this physical process. In deriving this non-relativistic process, the magnetic component of the Lorentz force is neglected, and the relevant particles are modeled as being in a damped harmonic oscillator. Its total cross section is independent of the frequency of radiation and scales as the square of the particle's Compton radius. For ten points, identify this scattering of electromagnetic radiation from a charged particle, named after the discoverer of the electron.
The partial linear polarization of the cosmic microwave background radiation is the result of this physical process.
Thomson scattering