Karlsruhe Astrophysical Database of Nucleosynthesis in Stars
s-process
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p-process
Available isotopes for Hafnium (Z=72)
  174Hf   176Hf   177Hf   178Hf   179Hf   180Hf   181Hf   182Hf
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Recommended MACS30 (Maxwellian Averaged Cross Section @ 30keV)
182Hf 183Hf




Cross sections do not include stellar enhancement factors!
History
VersionTotal MACS [mb]Partial to gs [mb]Partial to isomer [mb]
0.2141 ± 8--
0.0117 ± 41*--

(Version 0.0 corresponds to Bao et al.)
Comment
Rec. value is from activation measurement of VDH07. MACS vs. kT table is calculated with normalized evaluated value from jendl40 (f(norm)= 0.982).
Last review: January 2014
List of all available values
originalrenorm.yeartypeCommentRef
141 ± 8
2007,2013cVdG, Act., Au:RaK88; using en.dep. from jendl40VDH07
141 ± 8
2007cVdG, Act., Au:RaK88; using en.dep. from RaT99VDH07
144.1
2011eJENDL-4.0jendl40
120 ± 35
kT= 25 keV
2007tHFSM; priv. comm. A. MengoniVDH07
51 ± 25
kT= 25 keV
2007tCoH; priv. comm. T. KawanoVDH07
59
kT= 25 keV
2007tTALYS; priv. comm. A. KoningVDH07
270
kT= 25 keV
2007tEMPIRE; priv. comm. M. HermanVDH07
53.8
2005tMOST 2005Gor05
65.9
2002tMOST 2002Gor02
125
2000tNON-SMOKERRaT99
241
1981tHar81


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
tTheoretical value
MACS, SEF and Reaction Rates for different energies
Energy5keV8keV10keV15keV20keV25keV30keV40keV50keV60keV80keV100keV
MACS
343
-
240
197
172
155
141 ± 8
121
107
96
80
69
Xfactor1.001.001.000.990.940.870.780.610.480.390.270.20
SEF1.001.001.001.001.021.041.071.141.211.281.421.55
Rate
2.03
-
2.01
2.03
2.08
2.15
2.20
2.32
2.43
2.52
2.69
2.84

MACS:
Reference: VDH07,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: 2014

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
182W
26.5
274 mb
183W
14.31
515 mb
184W
30.64
223 mb
185W
75.10 d
703 mb, β-
186W
28.43
235 mb
181Ta
99.988
766 mb
182Ta
114.43 d
1120 mb, β-
183Ta
5.10 d
β-
184Ta
8.70 h
β-
185Ta
49.40 m
β-
180Hf
35.08
179 mb
181Hf
42.39 d
194 mb, β-
182Hf
8.90 Ma
117 mb, β-
183Hf
1.07 h
β-
184Hf
4.12 h
β-
179Lu
4.59 h
β-
180Lu
5.70 m
β-
181Lu
3.50 m
β-
182Lu
2.00 m
β-
183Lu
58.00 s
β-
178Yb
1.23 h
β-
179Yb
8.00 m
β-
180Yb
2.40 m
β-
181Yb
1.00 m
β-
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Style: (S, M, L, XL or Alberto)


Isotope: Hafnium