Rapid neutral–neutral reactions at low temperatures: a new network and first results for TMC‐1

By Ian W. M. Smith, E. Herbst, Q. Chang. 2004

226 citations recorded by the source corpus.

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

View Paper: https://www.semanticscholar.org/paper/9992c6d24fcb2b3e534fafe9e18ae06b0e3e13af

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Atmospheric Science

1. E. Herbst
2. V. Wakelam
3. R. Garrod
4. P. Caselli
5. F. Hersant
6. A. Vasyunin
7. C. Walsh
8. T. Millar

In Atomic and Molecular Physics, and Optics

1. P. Caselli
2. R. Garrod
3. V. Wakelam
4. A. Vasyunin
5. E. Herbst
6. C. Walsh
7. T. Millar
8. D. Semenov

Citations in the corpus

• The molecular composition of the planet-forming regions of protoplanetary disks across the luminosity regime (2015, background): “CN has numerous formation routes via neutral neutral reactions: N + C2 (Smith et al. 2004), NH + C (Brownsword et al. 1996), and NO + C (Chastaing et al. 2000) where NO is formed via the reaction, N + OH (Wakelam et al. 2012).”
• The UMIST database for astrochemistry 2012 (2012, background): “for which the analogous reaction involving C2H was measured in the laboratory by Smith et al. (2004).”
• Non-thermal desorption from interstellar dust grains via exothermic surface reactions (2007, methodology): “The “yes or no” method employed by Smith et al. (2004) naturally discards such outliers.”
• Chemistry in Disks. IV. Benchmarking gas-grain chemical models with surface reactions (2010, methodology): “…ratefiles: the UDFA (Umist Database For Astrochemistry1) (Millar et al., 1997; Le Teuff et al., 2000; Woodall et al., 2007), the OSU database (Ohio State University2) (Smith et al., 2004), and a network incorporated in the “Photo-Dissociation Region” code from Meudon3 (Le Petit et al., 2006).”
• Diffuse Atomic and Molecular Clouds (2006, background): “Much of the recent work on dense clouds has been directed toward hot cloud cores where star formation is incipient (for a recent paper summarizing the current state of modeling of such clouds, see Smith et al. 2004).”
• Formation of Complex Molecules in Prestellar Cores: A Multilayer Approach (2017, background): “Since Smith et al. (2004), it is recognized that fast neutral-neutral reactions can affect the abundances of exotic carbonbearing species in cold clouds.”
• Discovery of Interstellar Propylene (CH2CHCH3): Missing Links in Interstellar Gas-Phase Chemistry (2007, methodology): “Reaction networks used to model interstellar chemistry are usually tested by comparing with the molecular abundances observed in TMC-1 (Smith et al. 2004; Woodall et al. 2007).”