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Dissociative recombination of nitrile ions : DCCCN+ and DCCCND

Geppert, W D (author)
Ehlerding, A (author)
Hellberg, F (author)
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Semaniak, J (author)
Österdahl, Fabian (author)
KTH,Fysik
Kaminska, M (author)
Al-Khalili, A (author)
Zhaunerchyk, V (author)
Thomas, R (author)
Af Ugglas, M (author)
Kallberg, A (author)
Simonsson, A (author)
Larsson, M (author)
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 (creator_code:org_t)
American Astronomical Society, 2004
2004
English.
In: Astrophysical Journal. - : American Astronomical Society. - 0004-637X .- 1538-4357. ; 613:2, s. 1302-1309
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • Branching ratios and absolute cross sections have been measured for the dissociative recombination of DCCCN+ and DCCCND+ using the CRYRING ion storage ring. In the case of DCCCN+ the dissociation yielding D + C3N and those leading to two fragments containing a pair of heavy atoms dominate, whereas pathways producing a fragment with three heavy atoms play only a minor role. Conversely, for DCCCND+, only those channels preserving the carbon chain or producing two fragments with a pair of heavy atoms each are detected. The cross sections of the reactions are very similar and can be fitted to the expressions sigma = (2.9 +/- 0.5) x 10(-15)E(eV)(-1.05 +/- 0.02) cm(2) and sigma = (2.3 +/- 0.4) x 10(-15)E(eV)(-1.10 +/- 0.02) cm(2) for DCCCN+ and DCCCND+, respectively. From these data, thermal reaction rates of k(T) = (1.5 +/- 0.3) x 10(-6)(T/300 K)(-0.60 +/- 0.02) cm(3) s(-1) and k(T) = (1.5 +/- 0.3) x 10(-6)(T/300 K)(-0.58 +/- 0.02) cm(3) s(-1) were calculated for DCCCN+ and DCCCND+, respectively. These rates and branching ratios are compared with those hitherto used in astrophysical models.

Subject headings

NATURVETENSKAP  -- Fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences (hsv//eng)

Keyword

astrochemistry
methods : laboratory
molecular data

Publication and Content Type

ref (subject category)
art (subject category)

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