C5 + CRP
Gaz phase reaction (type: Photo-processes induced by cosmic-rays (secondary photons))
Datasheet
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Channels | |||||
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C5 + CRP
→
C + C4
|
15 % | Cosmic-ray ionization |
ΔrH0 = N/A
Δ rH298 = N/A |
2010-10-01 |
C5 + CRP → C + C4
Branching ratio : 15 % Formula : Cosmic-ray ionization Δ rH0 = N/A Δ rH298 = N/A Date:2010-10-01 |
C5 + CRP
→
C2 + C3
|
85 % | Cosmic-ray ionization |
ΔrH0 = N/A
Δ rH298 = N/A |
2010-10-01 |
C5 + CRP → C2 + C3
Branching ratio : 85 % Formula : Cosmic-ray ionization Δ rH0 = N/A Δ rH298 = N/A Date:2010-10-01 |
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Details | ||||||||
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C5 + CRP
→
C + C4
|
1.50E+2 | 0.00E+0 | 0.00E+0 | 1.25 | 0 | lognormal |
C5 + CRP → C + C4
α = 1.50E+2 β = 0.00E+0 γ = 0.00E+0 F 0 = 1.25 g = 0 Type uncert: lognormal UVField: Method: Measurements Description: BR measurement |
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Method: Measurements
Description: BR measurement |
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C5 + CRP
→
C2 + C3
|
8.50E+2 | 0.00E+0 | 0.00E+0 | 1.25 | 0 | lognormal |
C5 + CRP → C2 + C3
α = 8.50E+2 β = 0.00E+0 γ = 0.00E+0 F 0 = 1.25 g = 0 Type uncert: lognormal UVField: Method: Measurements Description: BR measurement |
|
Method: Measurements
Description: BR measurement |
Other database : OSU
Show/Hide those values
Channels | |||||
---|---|---|---|---|---|
C5 + CRP
→
C + C4
|
100 % | Cosmic-ray ionization |
ΔrH0 = N/A
Δ rH298 = N/A |
2009-03-27 |
C5 + CRP → C + C4
Branching ratio : 100 % Formula : Cosmic-ray ionization Δ rH0 = N/A Δ rH298 = N/A Date:2009-03-27 |
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Details | ||||||||
---|---|---|---|---|---|---|---|---|
C5 + CRP
→
C + C4
|
1.00E+3 | 0.00E+0 | 0.00E+0 | 1.25 | 0 | lognormal |
C5 + CRP → C + C4
α = 1.00E+3 β = 0.00E+0 γ = 0.00E+0 F 0 = 1.25 g = 0 Type uncert: lognormal UVField: Method: Calculations |
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Method: Calculations
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Reference | |||||||
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Other database : OSU | Bettens, R. P. A. et al | 149,321-343 | 1995 | International Journal of Mass Spectrometry and Ion Processes | DOI |
Bibtex
RIS |
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Origin: Other database : OSU
Authors: Bettens, R. P. A. et al Volume,Page: 149,321-343 Year: 1995 DOI: 10.1016/0168-1176(95)04266-N DOI Download citation: Bibtex RIS |