Dissociative Recombination of H3O+, HD2O+, and D3O+

By M. J. Jensen, R. Bilodeau, C. Safvan, K. Seiersen, L. H. Andersen, H. Pedersen, O. Heber. 2000

135 citations recorded by the source corpus.

Subfields: Atmospheric Science, Atomic and Molecular Physics, and Optics, Spectroscopy

View Paper: https://www.semanticscholar.org/paper/8997d81d85c4c0958e4d0e0f301bba4a3126dada

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In Atmospheric Science

1. E. Herbst
2. V. Wakelam
3. H. Cuppen
4. S. Glover
5. H. Linnartz
6. E. Bergin
7. R. Garrod
8. Ralf Klessen

In Atomic and Molecular Physics, and Optics

1. E. Bergin
2. E. Herbst
3. V. Wakelam
4. H. Linnartz
5. K. Oberg
6. T. Millar
7. H. Cuppen
8. H. Roberts

In Spectroscopy

1. E. Herbst
2. E. Bergin
3. V. Wakelam
4. T. Millar
5. H. Cuppen
6. K. Oberg
7. R. Garrod
8. H. Linnartz

Citations in the corpus

• WATER, O2, AND ICE IN MOLECULAR CLOUDS (2008, background): “We find that generally the route that takes over from photodissociation is reaction with H+3 to form H3O +. H3O+ recombines one-fourth of the time to reform water (not a net destruction) and three-fourths of the time to form OH (Jensen et al. 2000; Neufeld et al. 2002).”
• Physical Processes in the Interstellar Medium (2014, background): “…further with H2, but instead is removed from the gas via dissociative recombination, yielding a variety of products that include OH and water (see e.g. Jensen et al., 2000) H3O+ + e− → H2O + H, (171) H3O+ + e− → OH + H2, (172) H3O+ + e− → OH + H + H, (173) H3O+ + e− → O + H2 + H. (174) The other…”
• The chemistry of multiply deuterated species in cold, dense interstellar cores (2004, background): “Walmsley et al. (2004). species have more product channels than their un-deuterated analogues, we have assumed statistical branching ratios (Millar et al. 1989), except for the cases where experimental measurements indicate otherwise; e.g., for the recombination of the deuterated isotopomers of H2D+”
• Modelling CO formation in the turbulent interstellar medium (2009, unknown): “…(2004), 71: Takagi, Kosugi, & Le Dourneuf (1991), 72: Larson et al. (1998), 73: Mitchell (1990), 74: Guberman (1995), 75: Rosén et al. (2000), 76: Jensen et al. (2000), 77: Alge, Adams & Smith (1983), 78: Rosén et al. (1998), 79: Geppert et al. (2005), 80: Gerlich & Horning (1992), 81: Stancil…”
• Reaction Networks for Interstellar Chemical Modelling: Improvements and Challenges (2010, background): “Although some ions such as HCO+ follow that rule, many other important species such as H3O + (Jensen et al. 2000) and protonated methanol (CH3OH + 2 ) do not (Geppert et al. 2006).”
• A KINETIC DATABASE FOR ASTROCHEMISTRY (KIDA) (2012, unknown): “…et al. (1989); Gu et al. (2006);Sun & Li (2004); Harada & Herbst (2008); Herbst et al. (1989a); Herbst (1985, 1987); Herbst et al. (1989b, 2000); Jensen et al. (2000); Kaiser et al. (2002); Kalhori et al. (2002); Lee et al. (1978); Lilenfeld & Richardson (1977); Lique et al. (2009); Loison &…”