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Soft bremsstrahlung

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Abstract

Simple analytic formulas are considered for the energy radiated in low frequency bremsstrahlung from fully ionized gases. A formula that has been frequently cited over many years turns out to have only a limited range of validity, more narrow than for a formula derived using the Born approximation. In an attempt to find a more widely valid simple formula, a soft photon theorem is employed, which in this context implies that the differential rate of photon emission in an electron-ion collision with definite initial and final electron momenta is correctly given for sufficiently soft photons by the Born approximation, to all orders in the Coulomb potential. Corrections to the Born approximation arise because the upper limit on photon energy for this theorem to apply to a given collision becomes increasingly stringent as the scattering approaches the forward direction. A general formula is suggested that takes this into account.


Publication:

Physical Review D

Pub Date:
April 2019
DOI:

10.1103/PhysRevD.99.076018

10.48550/arXiv.1903.11168

arXiv:
arXiv:1903.11168
Bibcode:
2019PhRvD..99g6018W
Keywords:
  • Astrophysics - Astrophysics of Galaxies;
  • Astrophysics - High Energy Astrophysical Phenomena;
  • High Energy Physics - Phenomenology;
  • Physics - Plasma Physics
E-Print:
14 pages, no figures