Publication: Measurements of the reaction rate coefficients of atomic hydrogen with astrochemical anions: CN− and C3N−
dc.contributor.coauthor | Lochmann C., Melath S.P., Wild R., Martín Santa Daría A., González-Sánchez L., Gianturco F.A., Wester R. | |
dc.contributor.department | Department of Chemistry | |
dc.contributor.kuauthor | Yurtsever, İsmail Ersin | |
dc.contributor.schoolcollegeinstitute | College of Sciences | |
dc.date.accessioned | 2025-03-06T20:57:39Z | |
dc.date.issued | 2024 | |
dc.description.abstract | We present the temperature-dependent reaction rate coefficients of CN− and C3N− with atomic hydrogen in the temperature range from 7 to 290 K, measured in a 16-pole radio-frequency ion trap. The rate of C3N− with H steadily increases toward lower temperatures, while the rate coefficients for the CN− + H system show a sudden change around 160 K. Fits to the data were performed to determine temperature-dependent reaction rate coefficients. The fits reveal a rate coefficient of 4.1 ( 3 ) × 10 − 10 ( T / 300 ) − 0.31 ( 6 ) cm3 s−1 for C3N− + H. For CN−, we determined a rate coefficient for the temperature regime below 160 K of 3.2 ( 4 ) × 10 − 10 ( T / 300 ) − 0.31 ( 11 ) cm3 s−1. Given our present results, higher rate coefficients than previously reported must be assumed for the modeling of cold interstellar environments involving these H atom reactions. © 2024. The Author(s). Published by the American Astronomical Society. | |
dc.description.indexedby | WOS | |
dc.description.indexedby | Scopus | |
dc.description.publisherscope | International | |
dc.description.sponsoredbyTubitakEu | N/A | |
dc.description.sponsorship | This work has been supported by the Austrian Science Fund (FWF) through the Doctoral Programme Atoms, Light, and Molecules, Project No. W1259-N27 (grant doi:10.55776/W1259). L.G.S. and A.M.S.D. gratefully acknowledge grants PID2020-113147GA-100 and PID2021-122839NB-100 funded by the Spanish Ministry of Science and Innovation (MCIN/AEI/10.13039/MCIN/AEI/10.13039/501100011033). | |
dc.identifier.doi | 10.3847/1538-4357/ad808b | |
dc.identifier.eissn | 1538-4357 | |
dc.identifier.grantno | Austrian Science Fund, FWF: W1259-N27, PID2020-113147GA-100, PID2021-122839NB-100; Austrian Science Fund, FWF; Ministerio de Ciencia e Innovación, MCIN: MCIN/AEI/10.13039/MCIN/AEI/10.13039/501100011033; Ministerio de Ciencia e Innovación, MCIN | |
dc.identifier.issn | 0004-637X | |
dc.identifier.issue | 1 | |
dc.identifier.quartile | Q1 | |
dc.identifier.scopus | 2-s2.0-85210077882 | |
dc.identifier.uri | https://doi.org/10.3847/1538-4357/ad808b | |
dc.identifier.uri | https://hdl.handle.net/20.500.14288/27261 | |
dc.identifier.volume | 976 | |
dc.identifier.wos | 1355331400001 | |
dc.keywords | Electron attachment | |
dc.keywords | Ground state | |
dc.keywords | Quantum chemistry | |
dc.language.iso | eng | |
dc.publisher | Institute of Physics | |
dc.relation.ispartof | Astrophysical Journal | |
dc.subject | Chemistry | |
dc.title | Measurements of the reaction rate coefficients of atomic hydrogen with astrochemical anions: CN− and C3N− | |
dc.type | Journal Article | |
dspace.entity.type | Publication | |
local.contributor.kuauthor | Yurtsever, İsmail Ersin | |
local.publication.orgunit1 | College of Sciences | |
local.publication.orgunit2 | Department of Chemistry | |
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