The emission of this can be understood as a type of first-order radiative scattering transition of electrons by an electric field and produces a characteristically continuous energy spectrum.
The dominant factor in the non-collisional term of a high-energy electron's linear energy transfer, this process adds a loss term proportional to the square of the effective charge to a star's energy balance. The emission of this can be understood as a type of first-order radiative scattering transition of electrons by an electric field and produces a characteristically continuous energy spectrum. For 10 points, name this type of radiation comprised of the x-ray photons given-off by a decelerating electron and named by Tesla from the German for "breaking radiation."
The dominant factor in the non-collisional term of a high-energy electron's linear energy transfer, this process adds a loss term proportional to the square of the effective charge to a star's energy balance.
{bremsstrahlung}