Nonrelativistic Electron–Ion Bremsstrahlung: An Approximate Formula for All Parameters

Author:

Pradler JosefORCID,Semmelrock LukasORCID

Abstract

Abstract The evaluation of the electron–ion bremsstrahlung cross section—exact to all orders in the Coulomb potential—is computationally expensive due to the appearance of hypergeometric functions. Therefore, tabulations are widely used. Here, we provide an approximate formula for the nonrelativistic dipole process valid for all applicable relative velocities and photon energies. Its validity spans from the Born to the classical regime and from soft-photon emission to the kinematic endpoint. The error remains below 3% (and widely below 1%) except at an isolated region of hard-photon emission at the quantum-to-classical crossover. We use the formula to obtain the thermally averaged emission spectrum and cooling function in a Maxwellian plasma and demonstrate that they are accurate to better than 2%.

Funder

Austrian Academy of Sciences

Austrian Science Fund

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 4 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Stellar limits on scalars from electron-nucleus bremsstrahlung;Journal of Cosmology and Astroparticle Physics;2023-07-01

2. Suppression of bremsstrahlung losses from relativistic plasma with energy cutoff;Physical Review E;2023-06-12

3. Inverse Bremsstrahlung Absorption;Physical Review Letters;2023-04-04

4. Is there a Radio Excess from the Decoupling of Pre-recombination Bremsstrahlung?;Research Notes of the AAS;2022-12-15

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