Electromagnetic radiation that occurs when charged particles with energies large compared to their rest energies are decelerated over a very short distance. Since electrons are much lighter than protons, electron bremsstrahlung is the most common. In bremsstrahlung, a continuous spectrum with a characteristic profile and energy cutoff (i.e., wavelength minimum) is produced. In addition, lines can appear super imposed, corresponding to the ejection of K and L shell electrons knocked out of atoms in collisions with the high-energy electrons.
For the continuous bremsstrahlung spectrum, equate the quantities
[
where is the charge on the electron, V is the voltage change, h is Planck's constant, c is the speed of light, and is the minimum possible wavelength of radiation. Solving for then gives
[
The cross section for an electron to be observed in a solid angle is given by
where and are the initial and final velocities, respectively and is the range of wavenumbers. In the soft-photon limit, , and for scattering angle . In this limit, each of the last two integrals are given by
The first integral can be reduced to
This can be expanded in a series as
[
so combining ,,and gives
[
in the nonrelativistic limit (Bjorken and Drell 1964, pp. 126-127).
A line spectrum occurs when electrons are knocked out from low shells and electrons from higher shells drop down.
For the continuous bremsstrahlung spectrum, equate the quantities
(1)
where is the charge on the electron, V is the voltage change, h is Planck's constant, c is the speed of light, and is the minimum possible wavelength of radiation. Solving for then gives
(2)
The cross section for an electron to be observed in a solid angle is given by
(2)
where and are the initial and final velocities, respectively and is the range of wavenumbers. In the soft-photon limit, , and for scattering angle . In this limit, each of the last two integrals are given by
(4)
The first integral can be reduced to
(5)
This can be expanded in a series as
(6)
so combining ,,and gives
(7)
in the nonrelativistic limit (Bjorken and Drell 1964, pp. 126-127).
A line spectrum occurs when electrons are knocked out from low shells and electrons from higher shells drop down.
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