C4 + Photon

Gaz phase reaction (type: Photo-processes)  


     
 
Datasheet   
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Channels
C4 + Photon → C2 + C2
Branching ratio : 15 %
Formula : Photo (Draine)
Δ rH0 = N/A
Δ rH298 = N/A
Date:2011-04-27
C4 + Photon → C + C3
Branching ratio : 85 %
Formula : Photo (Draine)
Δ rH0 = N/A
Δ rH298 = N/A
Date:2011-04-27
Details
C4 + Photon → C2 + C2
α = 1.28E-9
β = 0.00E+0
γ = 2.30E+0
F 0 = 2
g = 0
Type uncert: lognormal
UVField: Draine
Method: Calculations
Description: Total rate is from van Hemert & van Dishoeck (2008). Branching ratios are from Chabot et al. (2010).
C4 + Photon → C + C3
α = 7.23E-9
β = 0.00E+0
γ = 2.30E+0
F 0 = 2
g = 0
Type uncert: lognormal
UVField: Draine
Method: Calculations
Description: Total rate is from van Hemert & van Dishoeck (2008). Branching ratios are from Chabot et al. (2010).
Reference
Origin: Datasheet
Authors: Chabot, M. et al
Volume,Page: 524,A39
Year: 2010
DOI: 10.1051/0004-6361/201015010 DOI
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Other database : Leiden   
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Channels
C4 + Photon → C + C3
Branching ratio : 100 %
Formula : Photo (Draine)
Δ rH0 = N/A
Δ rH298 = N/A
Date:2018-05-11
Details
C4 + Photon → C + C3
α = 8.48E-9
β = 0.00E+0
γ = 2.22E+0
F 0 = 2
g = 0
Type uncert: logn
UVField: Draine
Method: Reviews and Evaluations
Reference
Origin: Other database : Leiden
Authors: Heays, A.~N. et al
Volume,Page: 602, A105
Year: 2017
DOI: 10.1051/0004-6361/201628742 DOI
Download citation: Bibtex RIS
 
Other database : OSU   
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Channels
C4 + Photon → C2 + C2
Branching ratio : 50 %
Formula : Photo (Draine)
Δ rH0 = N/A
Δ rH298 = N/A
Date:2009-03-27
C4 + Photon → C + C3
Branching ratio : 50 %
Formula : Photo (Draine)
Δ rH0 = N/A
Δ rH298 = N/A
Date:2009-03-27
Details
C4 + Photon → C2 + C2
α = 2.00E-10
β = 0.00E+0
γ = 2.30E+0
F 0 = 2
g = 0
Type uncert: lognormal
UVField: Draine
Method: Estimation
Description: Rate computed for the standard interstellar radiation field cf. Draine (1978, ApJS, 36, 595).
C4 + Photon → C + C3
α = 2.00E-10
β = 0.00E+0
γ = 2.30E+0
F 0 = 2
g = 0
Type uncert: lognormal
UVField: Draine
Method: Estimation
Description: Rate computed for the standard interstellar radiation field cf. Draine (1978, ApJS, 36, 595).
Reference
Origin: Other database : OSU
Authors:
Volume,Page:
Year:
DOI: -
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