Efficient computation of collisional $\ell$-mixing rate coefficients in astrophysical plasmas
Instrumentation and Methods for Astrophysics
2019-07-17 v1 Astrophysics of Galaxies
Abstract
We present analytical expressions for direct evaluation of -mixing rate coefficients in proton-excited hydrogen atom collisions and describe a software package for efficient numerical evaluation of the collisional rate coefficients. Comparisons between rate coefficients calculated with various levels of approximation are discussed, highlighting their range of validity. These rate coefficients are benchmarked via radio recombination lines for hydrogen, evaluating the corresponding departure coefficients from local thermal equilibrium.
Keywords
Cite
@article{arxiv.1907.00972,
title = {Efficient computation of collisional $\ell$-mixing rate coefficients in astrophysical plasmas},
author = {D. Vrinceanu and R. Onofrio and J. B. R. Oonk and P. Salas and H. R. Sadeghpour},
journal= {arXiv preprint arXiv:1907.00972},
year = {2019}
}