Journal article

Experimental Determination of the Dissociative Recombination Rate Coefficient for Rotationally Cold CH+ and Its Implications for Diffuse Cloud Chemistry


Authors listPaul, Daniel; Grieser, Manfred; Grussie, Florian; von Hahn, Robert; Isberner, Leonard W.; Kalosi, Abel; Krantz, Claude; Kreckel, Holger; Muell, Damian; Neufeld, David A.; Savin, Daniel W.; Schippers, Stefan; Wilhelm, Patrick; Wolf, Andreas; Wolfire, Mark G.; Novotny, Oldrich

Publication year2022

JournalThe Astrophysical Journal

Volume number939

Issue number2

ISSN0004-637X

eISSN1538-4357

Open access statusGold

DOI Linkhttps://doi.org/10.3847/1538-4357/ac8e02

PublisherAmerican Astronomical Society


Abstract
Observations of CH+ are used to trace the physical properties of diffuse clouds, but this requires an accurate understanding of the underlying CH+ chemistry. Until this work, the most uncertain reaction in that chemistry was dissociative recombination (DR) of CH+. Using an electron-ion merged-beams experiment at the Cryogenic Storage Ring, we have determined the DR rate coefficient of the CH+ electronic, vibrational, and rotational ground state applicable for different diffuse cloud conditions. Our results reduce the previously unrecognized order-of-magnitude uncertainty in the CH+ DR rate coefficient to similar to 20% and are applicable at all temperatures relevant to diffuse clouds, ranging from quiescent gas to gas locally heated by processes such as shocks and turbulence. Based on a simple chemical network, we find that DR can be an important destruction mechanism at temperatures relevant to quiescent gas. As the temperature increases locally, DR can continue to be important up to temperatures of similar to 600 K, if there is also a corresponding increase in the electron fraction of the gas. Our new CH+ DR rate-coefficient data will increase the reliability of future studies of diffuse cloud physical properties via CH+ abundance observations.



Citation Styles

Harvard Citation stylePaul, D., Grieser, M., Grussie, F., von Hahn, R., Isberner, L., Kalosi, A., et al. (2022) Experimental Determination of the Dissociative Recombination Rate Coefficient for Rotationally Cold CH+ and Its Implications for Diffuse Cloud Chemistry, The Astrophysical Journal, 939(2), Article 122. https://doi.org/10.3847/1538-4357/ac8e02

APA Citation stylePaul, D., Grieser, M., Grussie, F., von Hahn, R., Isberner, L., Kalosi, A., Krantz, C., Kreckel, H., Muell, D., Neufeld, D., Savin, D., Schippers, S., Wilhelm, P., Wolf, A., Wolfire, M., & Novotny, O. (2022). Experimental Determination of the Dissociative Recombination Rate Coefficient for Rotationally Cold CH+ and Its Implications for Diffuse Cloud Chemistry. The Astrophysical Journal. 939(2), Article 122. https://doi.org/10.3847/1538-4357/ac8e02



Keywords


CROSS-SECTIONHEH+TURBULENT

Last updated on 2025-10-06 at 11:46