C10 + CRP

Gaz phase reaction (type: Photo-processes induced by cosmic-rays (secondary photons))  


     
 
Datasheet   
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Channels
C10 + CRP → C + C9
Branching ratio : 0 %
Formula : Cosmic-ray ionization
Δ rH0 = N/A
Δ rH298 = N/A
Date:2010-10-01
C10 + CRP → C3 + C7
Branching ratio : 75 %
Formula : Cosmic-ray ionization
Δ rH0 = N/A
Δ rH298 = N/A
Date:2010-10-01
C10 + CRP → C5 + C5
Branching ratio : 25 %
Formula : Cosmic-ray ionization
Δ rH0 = N/A
Δ rH298 = N/A
Date:2010-10-01
Details
C10 + CRP → C + C9
α = 0.00E+0
β = 0.00E+0
γ = 0.00E+0
F 0 = 1.25
g = 0
Type uncert: lognormal
UVField:
Method: Measurements
Description: BR measurement
C10 + CRP → C3 + C7
α = 7.50E+2
β = 0.00E+0
γ = 0.00E+0
F 0 = 1.25
g = 0
Type uncert: lognormal
UVField:
Method: Measurements
Description: BR measurement
C10 + CRP → C5 + C5
α = 2.50E+2
β = 0.00E+0
γ = 0.00E+0
F 0 = 1.25
g = 0
Type uncert: lognormal
UVField:
Method: Measurements
Description: BR measurement
Reference
Origin: Datasheet
Authors: Chabot, M. et al
Volume,Page: 524,A39
Year: 2010
DOI: 10.1051/0004-6361/201015010 DOI
Download citation: Bibtex RIS
 
Other database : OSU   
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Channels
C10 + CRP → C + C9
Branching ratio : 100 %
Formula : Cosmic-ray ionization
Δ rH0 = N/A
Δ rH298 = N/A
Date:2009-03-27
Details
C10 + CRP → C + C9
α = 1.00E+3
β = 0.00E+0
γ = 0.00E+0
F 0 = 1.5
g = 0
Type uncert: lognormal
UVField:
Method: Estimation
Description: Guess from Eric Herbst
Reference
Origin: Other database : OSU
Authors:
Volume,Page:
Year:
DOI: -
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