The electric-charge distribution in dark molecular clouds

Abstract We have extended previous quantum mechanical calculations of cross sections and rate coefficients for electron attachment to small, spherical, uncharged grains. It is found that potential-dependent resonances can have large effects on the low-energy cross sections and hence on the low-temperature rate coefficients. Comparison is made with previous calculations of electron attachment to PAH molecules, which adopted a similar approach. At low temperatures ($T \mathrel {\hbox{\rlap{\hbox{\lower4pt\hbox{$\sim $}}}\hbox{$<$}}}100$ K), the value of the rate coefficient for electron attachment to PAH molecules is subject to the same uncertainties as for small grains. At higher temperatures, on the other hand, we would expect the rate coefficients for both PAH molecules and small grains to converge to classical (Langevin) values. Whilst this is observed to be the case for small grains, the values for PAH molecules remain much lower than the classical limit. The reasons for this discrepancy are considered, and we conclude that the rate coefficients previously reported for electron attachment to PAH molecules are underestimated by between 2 and 3 orders of magnitude. The consequences for the electric-charge distribution in dark clouds are investigated.

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Publication Details

Journal
Monthly Notices of the Royal Astronomical Society
Published
2026-09-25
DOI
https://doi.org/10.1093/mnras/stag1801
Primary Topic
Astrophysics and Star Formation Studies
Type
article
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The electric-charge distribution in dark molecular clouds

David R. Flower, G Pineau des Forêts
Monthly Notices of the Royal Astronomical Society
Astrophysics and Star Formation Studies
article

The electric-charge distribution in dark molecular clouds

David R. Flower, G Pineau des Forêts
article en

Abstract

Abstract We have extended previous quantum mechanical calculations of cross sections and rate coefficients for electron attachment to small, spherical, uncharged grains. It is found that potential-dependent resonances can have large effects on the low-energy cross sections and hence on the low-temperature rate coefficients. Comparison is made with previous calculations of electron attachment to PAH molecules, which adopted a similar approach. At low temperatures ($T \mathrel {\hbox{\rlap{\hbox{\lower4pt\hbox{$\sim $}}}\hbox{$<$}}}100$ K), the value of the rate coefficient for electron attachment to PAH molecules is subject to the same uncertainties as for small grains. At higher temperatures, on the other hand, we would expect the rate coefficients for both PAH molecules and small grains to converge to classical (Langevin) values. Whilst this is observed to be the case for small grains, the values for PAH molecules remain much lower than the classical limit. The reasons for this discrepancy are considered, and we conclude that the rate coefficients previously reported for electron attachment to PAH molecules are underestimated by between 2 and 3 orders of magnitude. The consequences for the electric-charge distribution in dark clouds are investigated.

Monthly Notices of the Royal Astronomical Society
Centre National de la Recherche Scientifique (FR), Durham University (GB), Université Paris Sciences et Lettres (FR), Université Paris-Saclay (FR), Sorbonne Université (FR), Institut d'Astrophysique Spatiale (FR)
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Openalex Percentile: Top 11%
Astrophysics and Star Formation Studies
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The electric-charge distribution in dark molecular clouds — David R. Flower, G Pineau des Forêts · Monthly Notices of the Royal Astronomical Society (2026) | TGRS Research Map | TGRS