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arXiv:1903.11168astro-ph.GA

Soft Bremsstrahlung

Steven Weinberg

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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.

arXiv comments
14 pages, no figures
Journal reference
Phys. Rev. D 99, 076018 (2019)
DOI
doi:10.1103/PhysRevD.99.076018
Subjects
astro-ph.GAAstrophysics of Galaxies astro-ph.HEHigh Energy Astrophysical Phenomena hep-phHigh Energy Physics, Phenomenology physics.plasm-phPlasma Physics

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    • To follow on a bit, the wikipedia article: https://en.wikipedia.org/wiki/Bremsstrahlung links to a paper by Weinberg: https://arxiv.org/abs/1903.11168 and a quick skimming shows that he's perfectly happy to use the Coulomb field as an approximation...

      tgarrettView on HNParent context

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