Karlsruhe Astrophysical Database of Nucleosynthesis in Stars
s-process
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p-process
Available isotopes for Manganese (Z=25)
  53Mn   54Mn   55Mn
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Recommended MACS30 (Maxwellian Averaged Cross Section @ 30keV)
55Mn 56Mn




Cross sections do not include stellar enhancement factors!
History
VersionTotal MACS [mb]Partial to gs [mb]Partial to isomer [mb]
1.032.7 ± 3.1--
0.039.6 ± 3.0--

(Version 0.0 corresponds to Bao et al.)
Comment
New rec. value is average from recent evaluation (endfb71,jendl40) using the uncertainty from given covariances. A small additional uncertainty is introduced by the different energy dependencies of endfb71 and jendl40.
Last review: May 2016
List of all available values
originalrenorm.yeartypeCommentRef
39.6 ± 3.0
1978rLinac, TOF, 6Li, Au:Sat., k=0.9587, Recalcul. including data of MDH81GMH78
31.6 ± 3.0
1978b,1Linac, TOF, 6Li, Au:Sat., k=0.9587GMH78
32.1 ± 3.0
1976bVdG, TOF, 10B+6LiRAT76
37 ± 3
1970cSb-Be, Act., 1/v(E), Au:640mb(24keV)ChP70
32.8
2015eTENDL-2015 using the TALYS codetendl15
32.8 ± 2.9
2011eENDF/B-VII.1 incl. covariancesendfb71
32.7 ± 3.3
2011eJENDL-4.0 incl. covariancesjendl40
31.02
2006eENDF/B-VII.0endfb7
31.02
2004eJEFF-3.1jeff31
31.02
2002eJENDL-3.3jendl33
50 ± 2
1971eAGM71
60.4
2005tMOST 2005Gor05
72.4
2002tMOST 2002Gor02
35.5
2000tNON-SMOKERRaT99
28
1978tWFH78


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:
rRecalculated for kT = 30keV with the code described in Ref. 2 after renormalizing the original data to updated standard cross sections
bCalculated from smooth cross sections with model fit: ln(sigma) = a + a1 ln(E) + a2 ln^2(E)
1Including k from Ref. MaW81, where k is a correction factor which has been applied to the originally reported cross section
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
182.9 ± 14.9
-
87.8 ± 7.6
59.5 ± 5.3
46.0 ± 4.2
38.0 ± 3.5
32.7 ± 3.1
26.1 ± 2.7
22.0 ± 2.4
19.2 ± 2.3
15.5 ± 2.1
13.1 ± 1.9
Xfactor1.001.001.001.001.001.000.990.970.940.920.860.81
SEF1.001.001.001.001.001.000.990.970.960.940.910.90
Rate
1.09
-
0.74
0.61
0.55
0.50
0.47
0.43
0.40
0.37
0.34
0.31

MACS:
Reference: 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: 2013

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
55Co
17.53 h
β+
56Co
77.23 d
β+
57Co
271.76 d
β+
58Co
70.86 d
β+
59Co
100
38 mb
54Fe
5.845
27.6 mb
55Fe
2.74 a
75 mb, β+
56Fe
91.754
11.7 mb
57Fe
2.119
40 mb
58Fe
0.282
12.1 mb
53Mn
3.74 Ma
β+
54Mn
312.15 d
β+
55Mn
100
39.6 mb
56Mn
2.58 h
β-
57Mn
1.42 m
β-
52Cr
83.789
8.8 mb
53Cr
9.501
58 mb
54Cr
2.365
6.7 mb
55Cr
3.50 m
β-
56Cr
5.94 m
β-
51V
99.75
38 mb
52V
3.74 m
β-
53V
1.60 m
β-
54V
49.80 s
β-
55V
6.54 s
β-
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Isotope: Manganese