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Formation of the NH molecule and its isotopologues through radiative association
Luleå University of Technology, Department of Engineering Sciences and Mathematics, Material Science.ORCID iD: 0000-0002-0271-4846
Luleå University of Technology, Department of Engineering Sciences and Mathematics, Material Science.ORCID iD: 0000-0002-7629-0169
2019 (English)In: Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, E-ISSN 1365-2966, Vol. 483, no 3, p. 3574-3578Article in journal (Refereed) Published
Abstract [en]

The rate coefficients and the cross-sections for the formation of imidogen (NH) molecule (and its isotopologues: 15NH and ND) through radiative association are determined by employing quantum mechanical perturbation theory, classical Larmor formula, and Breit–Wigner theory. We suggest the radiative association process as possible route for NH production in diffuse interstellar clouds.

Place, publisher, year, edition, pages
Oxford Journals , 2019. Vol. 483, no 3, p. 3574-3578
Keywords [en]
molecular processes, scattering, ISM: atoms, ISM: clouds, ISM: molecules
National Category
Atom and Molecular Physics and Optics Composite Science and Engineering Other Physics Topics
Research subject
Applied Physics
Identifiers
URN: urn:nbn:se:ltu:diva-73251DOI: 10.1093/mnras/sty3246ISI: 000462280000046OAI: oai:DiVA.org:ltu-73251DiVA, id: diva2:1297168
Funder
The Kempe FoundationsKnut and Alice Wallenberg Foundation
Note

Validerad;2019;Nivå 2;2019-04-10 (oliekm)

Available from: 2019-03-19 Created: 2019-03-19 Last updated: 2019-04-10Bibliographically approved

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Publisher's full texthttps://academic.oup.com/mnras/article/483/3/3574/5218521

Authority records BETA

Szabo, PeterGustafsson, Magnus

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