Karlsruhe Astrophysical Database of Nucleosynthesis in Stars
s-process
[Standards]   [Logbook]   [FAQ]   [Links]   [Contact]
p-process
Available isotopes for Promethium (Z=61)
  147Pm   148gPm   148mPm   149Pm
Go to isotope
Recommended MACS30 (Maxwellian Averaged Cross Section @ 30keV)
147Pm 148Pm




Cross sections do not include stellar enhancement factors!
History
VersionTotal MACS [mb]Partial to gs [mb]Partial to isomer [mb]
0.2709 ± 100313 ± 60395 ± 55
0.01290 ± 470* - -

(Version 0.0 corresponds to Bao et al.)
Comment
Last review: June 14th, 2005
List of all available values
originalrenorm.yeartypeCommentRef
709 ± 100
2003cVdG, Act., 1/v(kT), Au:RaK88Rei03a
938
1981eKNM81
2000
1971sAGM71
1050
2006eendfb7
1177
2004ejeff31
1050
2002ejendl33
1270
2000tRaT99
985 ± 250
1995tTDK95
1163
1986tWKW86
1135
1981tHar81
1400
1976tHWF76
344
2002tMOST 2002Gor02
452
2005tMOST 2005Gor05
Partial cross section to 148gPm:
313 ± 60
2003cRei03a
Partial cross section to 148mPm:
395 ± 55
2003cRei03a


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
Energy5keV10keV15keV20keV25keV30keV40keV50keV60keV80keV100keV
MACS
 2257 
1373 
1055 
887 
782 
709 ± 100
 613 
553 
 503 
 455 
 418 
SEF1.001.001.001.000.990.980.960.950.930.900.88
Rate
1.34
1.15
1.08
1.05
1.03
1.01
0.99
0.98
0.96
0.97
0.97

MACS:
Reference: Rei03a
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: 2003

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

Rate:
Reaction rate NA<σv> given in 108 cm3/mole/s, including SEF
Isotopic mass chain
Isotopic Mass Chain
Chart of nuclei
up
left
147Eu
24.10 d
β+
148Eu
54.50 d
β+
149Eu
93.10 d
β+
150Eu
36.89 a
β+
151Eu
47.81
3775 mb
146Sm
102.99 Ma
α
147Sm
106.00x109 y
973 mb, α
148Sm
11.24
241 mb
149Sm
13.82
1820 mb
150Sm
7.38
422 mb
145Pm
17.70 a
β+
146Pm
5.53 a
β+
147Pm
2.62 a
1290 mb, β-
148Pm
5.37 d
2453 mb, β-
149Pm
2.21 d
2510 mb, β-
144Nd
23.8
81.3 mb
145Nd
8.3
425 mb
146Nd
17.2
91.2 mb
147Nd
10.98 d
544 mb, β-
148Nd
5.7
147 mb
143Pr
13.57 d
350 mb, β-
144Pr
17.28 m
β-
145Pr
5.98 h
β-
146Pr
24.15 m
β-
147Pr
13.40 m
β-
right
down
Style: (Size: S, M, L, XL, Alberto; No-Macs: nox)


Isotope: Promethium