Published September 1998 | Version v1
Journal article

Branching Fractions in Dissociative Recombination of CH+2

  • 1. Department of Physics I, Royal Institute of Technology (KTH), S-100 44 Stockholm (Sweden)
  • 2. Department of Physics, Stockholm University, PO Box 6730, S-113 85 Stockholm (Sweden)
  • 3. Institute of Physics, Pedagogical University, ul. M Konopnickiej 15, 25-430 Kielce (Poland)
  • 4. FOM Institute for Atomic and Molecular Physics, Kruislaan 407, 1098 SJ Amsterdam (Netherlands)
  • 5. Manne Siegbahn Laboratory, Frescativaegen 24, S-104 05 Stockholm (Sweden)
  • 6. JILA, University of Colorado, Campus Box 440, Boulder, CO 80309-0390 (United States)
  • 7. Physics Division, Oak Ridge National Laboratory, PO Box 2008, Oak Ridge, TN 37831-6377 (United States)

Description

The absolute cross section and branching ratios for dissociative recombination of CH+2 with electrons have been measured by means of the heavy-ion storage ring CRYRING. Contrary to what has been previously believed, recombination of CH+2 is dominated by the three-body channel C + H + H (63%), whereas breakup into the CH + H and C + H2 channels occurs with branching ratios of 25% and 12%, respectively. The thermal rate coefficient for dissociative recombination at 300 K is 6.4 x 10-7 cm3 s-1, which is higher by a factor of 2.5 than the value used in modeling dark molecular clouds. The low CH production and the high production of energetic carbon atoms could be favorable factors for the turbulence model to explain the large abundance of interstellar CH+. The cross section for dissociative excitation was also measured and found to be in good agreement with results from a crossed electron-ion beam experiment. copyright copyright 1998. The American Astronomical Society

Additional details

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
505
Journal Issue
1
Journal Page Range
p. 459-465
ISSN
0004-637X
CODEN
ASJOAB