English

Soft Bremsstrahlung

Astrophysics of Galaxies 2019-05-08 v1 High Energy Astrophysical Phenomena High Energy Physics - Phenomenology Plasma Physics

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.

Keywords

Cite

@article{arxiv.1903.11168,
  title  = {Soft Bremsstrahlung},
  author = {Steven Weinberg},
  journal= {arXiv preprint arXiv:1903.11168},
  year   = {2019}
}

Comments

14 pages, no figures

R2 v1 2026-06-23T08:20:11.183Z