Karlsruhe Astrophysical Database of Nucleosynthesis in Stars
s-process
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p-process
Available isotopes for Osmium (Z=76)
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Recommended MACS30 (Maxwellian Averaged Cross Section @ 30keV)
189Os 190Os




Cross sections do not include stellar enhancement factors!
History
VersionTotal MACS [mb]Partial to gs [mb]Partial to isomer [mb]
1.01083 ± 30--
0.01168 ± 47--

(Version 0.0 corresponds to Bao et al.)
Comment
Rec. value is from evaluated library jendl40 which reproduces data of SMN07 in the unresolved resonance region. Uncertainty assumed to be ca. 3% as in SMN07.
Last review: March 2014
List of all available values
originalrenorm.yeartypeCommentRef
1090 ± 30
E(n)= 31 (5) keV
2007cPelletron, TOF, Au:endfb7 and MaG67bSMN07
1168 ± 47
1987cLinac, TOF, 6Li, Au:Sat.WMH87
1560 ± 32
E(n)= 32 (4) keV
1981cLinac, TOF, 6Li:B-IV, 165Ho:Sat.BrB81
1083
2011eJENDL-4.0jendl40
765
1971sAGM71
1374
2005tMOST 2005Gor05
1983
2002tMOST 2002Gor02
913
2000tNON-SMOKERRaT99
1238
1981tHar81
858
1976tHWF76


Original:MACS [<σ v>/vT] (mb) for kT=30 keV, based on the published cross sections except where indicated otherwise.
Renorm:MACS [<σ v>/vT] (mb) for kT=30 keV for which the reference or standard cross section was meanwhile improved.
Type: The letters and numbers in the column labelled 'type' give information on how the cross section has been obtained:
cDirectly quoted from the reference itself
eEvaluated value taken directly from the reference
sSemiempirical estimates given in the reference
tTheoretical value
MACS, SEF and Reaction Rates for different energies
Energy5keV8keV10keV15keV20keV25keV30keV40keV50keV60keV80keV100keV
MACS
3938
-
2355
1768
1446
1235
1083 ± 30
876
739
641
509
424
Xfactor1.000.930.890.700.560.460.380.290.240.200.150.12
SEF1.001.001.001.021.061.081.101.141.161.181.211.23
Rate
2.33
-
1.97
1.86
1.81
1.77
1.74
1.67
1.61
1.56
1.46
1.38

MACS:
Reference: jendl40, SMN07
Procedure: 'e+t' (The MACS from kT=5 keV to 100 keV are derived from calculated cross sections, which are then normalized to experimental data, e.g. to the values at kT=25 keV obtained in activation measurements. In these cases the uncertainties should be linearly increased below 25 and above 30 keV to reach about 30% at the extreme kT values.)
Year: 2011

X-factor:
Reference: Rau12
Year: 2012

SEF (Stellar enhancement factor):
Reference: Rau09
Year: 2009
Comment:

Rate:
Reaction rate NA<σv> given in 108 cm3/mole/s, including SEF
Chart of nuclei
Style: (S, M, L, XL or Alberto)


Isotope: Osmium