Karlsruhe Astrophysical Database of Nucleosynthesis in Stars
s-process
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p-process
Available isotopes for Ruthenium (Z=44)
  96Ru   98Ru   99Ru   100Ru   101Ru   102Ru   103Ru   104Ru   105Ru   106Ru
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Recommended MACS30 (Maxwellian Averaged Cross Section @ 30keV)
102Ru 103Ru




Cross sections do not include stellar enhancement factors!
History
VersionTotal MACS [mb]Partial to gs [mb]Partial to isomer [mb]
1.0171 ± 11--
0.2151 ± 7--
0.0186 ± 11--

(Version 0.0 corresponds to Bao et al.)
Comment
Rec. value is the weighted average of the renormalized value from Rap02 and MaH80. New MACS vs. kT table is the normalized energy dependency from jeff32/endfb71/jendl40. Uncertainty towards kT=5 and 100 keV is the extrapolated uncertainty from the deviation between the libraries.
Last review: January 2017
List of all available values
originalrenorm.yeartypeCommentRef
151 ± 7
163 ± 82002cVdG, Act., Au:RaK88 corrected by 632/586= 1.0785Rap02
186 ± 11
1980c,1Linac, TOF, 6Li+235U:endfb52, Au:Sat., k=0.985MaH80
313 ± 84
2671973cSb-Be, Act., 1/v(E), 127I: 832 mb (24keV)MSR73
251.6
2015eTENDL-2015 using the TALYS codetendl15
190.7
2014eJEFF-3.2jeff32
190.7 ± 26.6
2011eENDF/B-VII.1 incl. covariancesendfb71
189.6
2011eJENDL-4.0jendl40
190.0
2004eJEFF-3.1jeff31
189.8
2002eJENDL-3.3jendl33
314
1981eKNM81
330 ± 50
1971eAGM71
224
2005tMOST 2005Gor05
282
2002tMOST 2002Gor02
146.9
2000tNON-SMOKERRaT99
133
1981tHar81
91
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
1Including k from Ref. MaW81, where k is a correction factor which has been applied to the originally reported cross section
eEvaluated value taken directly from the reference
tTheoretical value
MACS, SEF and Reaction Rates for different energies
Energy5keV8keV10keV15keV20keV25keV30keV40keV50keV60keV80keV100keV
MACS
459 ± 50
-
327 ± 33
259 ± 24
218 ± 18
191 ± 14
171 ± 11
145 ± 11
129 ± 11
118 ± 11
105 ± 12
97 ± 13
Xfactor1.001.001.001.001.001.001.001.001.001.000.980.95
SEF1.001.001.001.001.001.001.001.001.001.001.001.01
Rate
2.73
-
2.75
2.67
2.59
2.54
2.49
2.44
2.42
2.43
2.50
2.61

MACS:
Reference: Rap02,MaH80 jeff32/endfb71/jendl40
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: 2017

X-factor:
Reference: Rau12
Year: 2012

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

Rate:
Reaction rate NA<σv> given in 107 cm3/mole/s, including SEF
Chart of nuclei
up
left
102Pd
1.02
369 mb
103Pd
16.99 d
β+
104Pd
11.14
289 mb
105Pd
22.33
1200 mb
106Pd
27.33
252 mb
101Rh
3.30 a
β+
102Rh
206.94 d
β+
103Rh
100
811 mb
104Rh
42.30 s
β-
105Rh
1.47 d
β-
100Ru
12.6
206 mb
101Ru
17.06
996 mb
102Ru
31.55
186 mb
103Ru
39.26 d
343 mb, β-
104Ru
18.62
161 mb
99Tc
211.11 ka
781 mb, β-
100Tc
15.80 s
β-
101Tc
14.22 m
β-
102Tc
5.28 s
β-
103Tc
54.20 s
β-
98Mo
24.13
99 mb
99Mo
2.75 d
240 mb, β-
100Mo
9.63
108 mb
101Mo
14.61 m
β-
102Mo
11.30 m
β-
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Style: (S, M, L, XL or Alberto)


Isotope: Ruthenium