Published June 1991 | Version v1
Journal article

Calculations concerning the reaction C + H3(+) - CH(+) + H2

  • 1. Duke University, Durham, NC (USA)
  • 2. IBM Almaden Research Center, San Jose, CA (USA)
  • 3. Molecular Research Institute, Palo Alto (USA)
  • 4. Laboratoire de Radioastronomie Millimetrique, Paris (France)
  • 5. Molecular Research Institute, Palo Alto, CA (USA)

Description

The ion-molecule reaction of C + H3(+) - CH(+) + H2 has not been studied in the laboratory but is thought to be important in the gas phase synthesis of organic molecules in dense interstellar clouds. This reaction was studied theoretically by performing quantum chemical ab initio calculations on the potential surface. It is found that there is no activation barrier to the reaction and that it proceeds smoothly to the first excited electronic state of CH(+). The rate coefficient as a function of temperature can then be estimated using the proper long-range potentials. The rate coefficient at 10 K is calculated to be 2.9 x 10 to the -9th cu cm/sec. 18 refs

Additional details

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
374
Series
Astrophys. J.
Journal Page Range
390-393
ISSN
0004-637X
CODEN
ASJOA

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
22078950
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
CHEMICAL COMPOSITION; COSMIC GASES; COSMOCHEMISTRY; HYDROCARBONS; INTERSTELLAR SPACE; MOLECULAR STRUCTURE; ORGANIC COMPOUNDS; SYNTHESIS
Descriptors DEC
CHEMISTRY; FLUIDS; GASES; SPACE