SwePub
Sök i LIBRIS databas

  Extended search

onr:"swepub:oai:DiVA.org:kth-26368"
 

Search: onr:"swepub:oai:DiVA.org:kth-26368" > Rate constants and ...

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist

Rate constants and branching ratios for the dissociative recombination of CO2+

Viggiano, A. A. (author)
Ehlerding, A. (author)
Hellberg, F. (author)
show more...
Thomas, R. D. (author)
Zhaunerchyk, V. (author)
Geppert, W. D. (author)
Montaigne, H. (author)
Larsson, M. (author)
Kaminska, M. (author)
Österdahl, Fabian (author)
KTH,Fysik
show less...
 (creator_code:org_t)
AIP Publishing, 2005
2005
English.
In: Journal of Chemical Physics. - : AIP Publishing. - 0021-9606 .- 1089-7690. ; 122:22, s. 226101-
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • The calculation of rate constants and branching ratios was carried out to study the dissociative recombination of CO2+. The recombination of CO2+ is significant in the atmospheres of Venus and Mars. Rate constants and cross sections were studied by ramping the electron beam around a center-of-mass energy of 0 eV. The results of the study confirms that all the recombination of CO2+ results in a simple bondbreaking to form CO plus O. The rate constants show good agreement with measurements at 300 K and the electron energy dependence is identical to storage ring results.

Subject headings

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

Keyword

Chemical bonds
Dissociation
Electron beams
Energy absorption
Extraterrestrial atmospheres
Planets
Rate constants
Physics
Fysik

Publication and Content Type

ref (subject category)
art (subject category)

Find in a library

To the university's database

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist

Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.

 
pil uppåt Close

Copy and save the link in order to return to this view