Publication:
Measurements of the reaction rate coefficients of atomic hydrogen with astrochemical anions: CN− and C3N−

dc.contributor.coauthorLochmann C., Melath S.P., Wild R., Martín Santa Daría A., González-Sánchez L., Gianturco F.A., Wester R.
dc.contributor.departmentDepartment of Chemistry
dc.contributor.kuauthorYurtsever, İsmail Ersin
dc.contributor.schoolcollegeinstituteCollege of Sciences
dc.date.accessioned2025-03-06T20:57:39Z
dc.date.issued2024
dc.description.abstractWe 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.indexedbyWOS
dc.description.indexedbyScopus
dc.description.publisherscopeInternational
dc.description.sponsoredbyTubitakEuN/A
dc.description.sponsorshipThis 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.doi10.3847/1538-4357/ad808b
dc.identifier.eissn1538-4357
dc.identifier.grantnoAustrian 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.issn0004-637X
dc.identifier.issue1
dc.identifier.quartileQ1
dc.identifier.scopus2-s2.0-85210077882
dc.identifier.urihttps://doi.org/10.3847/1538-4357/ad808b
dc.identifier.urihttps://hdl.handle.net/20.500.14288/27261
dc.identifier.volume976
dc.identifier.wos1355331400001
dc.keywordsElectron attachment
dc.keywordsGround state
dc.keywordsQuantum chemistry
dc.language.isoeng
dc.publisherInstitute of Physics
dc.relation.ispartofAstrophysical Journal
dc.subjectChemistry
dc.titleMeasurements of the reaction rate coefficients of atomic hydrogen with astrochemical anions: CN− and C3N−
dc.typeJournal Article
dspace.entity.typePublication
local.contributor.kuauthorYurtsever, İsmail Ersin
local.publication.orgunit1College of Sciences
local.publication.orgunit2Department of Chemistry
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