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Total MACS at 30keV:

23.6

±

5.2

mb

Cross sections do not include stellar enhancement factors!

Version	Total MACS [mb]	Partial to gs [mb]	Partial to isomer [mb]
1.0	23.6 ± 5.2	-	-

(Version 0.0 corresponds to Bao et al.)

New dataset in v1.0. Rec. value is deduced from UAA14 by normalizing various theoretical predictions (RaT99, jendl40, jeff30A, tendl15) to the values of UAA14 between kT=80-100 keV, and extrapolating these cross sections down to kT= 5 keV. The uncertainty is the deviation between the predictions for kT=5-30 keV, and taken as 20% for kT>40 keV.
Last review: June 2016

original	renorm.	year	type	Comment	Ref
13.3 +2.0 -3.1 kT= 80 keV	23.6 ± 5.2	2014,2016	c	Coulomb dissociation; en.dep. from RaT99,jendl40,jeff30A,tendl15	UAA14
53.1		2015	t	TENDL-2015 using the TALYS code	tendl15
13.36		2011	t	JENDL-4.0	jendl40
16.2		2004	t	JEFF-3.0/A	jeff30A
53.8		2005	t	MOST 2005	Gor05
59		2002	t	MOST 2002	Gor02
22.5		2000	t	NON-SMOKER	RaT99

Original:MACS [<σ v>/v_T] (mb) for kT=30 keV, based on the published cross sections except where indicated otherwise.
Renorm:MACS [<σ v>/v_T] (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:

c	Directly quoted from the reference itself
t	Theoretical value

Energy	5keV	8keV	10keV	15keV	20keV	25keV	30keV	40keV	50keV	60keV	80keV	100keV
MACS	89 ± 39	-	50 ± 21	37 ± 14	30 ± 10	26.3 ± 7.0	23.6 ± 5.2	19.9 ± 4.0	17.4 ± 3.5	15.7 ± 3.1	13.2 ± 2.6	11.5 ± 2.3
Xfactor	1.00	1.00	1.00	1.00	1.00	1.00	1.00	1.00	1.00	1.00	0.99	0.98
SEF	1.00	1.00	1.00	1.00	1.00	1.00	1.00	1.00	1.00	0.99	0.99	0.97
Rate	5.31	-	4.22	3.82	3.58	3.51	3.45	3.36	3.28	3.22	3.11	2.98

MACS:
Reference: UAA14, RaT99,jendl40,jeff30A,tendl15
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: 2016

X-factor:
Reference: Rau12
Year: 2012

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

Rate:
Reaction rate N_A<σv> given in 10⁶ cm³/mole/s, including SEF

	59Ni 75.99 ka 87 mb, β+ 60Ni 26.223 30 mb 61Ni 1.14 82 mb 62Ni 3.634 22.3 mb 63Ni 100.11 a 31 mb, β- 58Co 70.86 d β+ 59Co 100 38 mb 60Co 5.27 a β- 61Co 1.65 h β- 62Co 1.50 m β- 57Fe 2.119 40 mb 58Fe 0.282 12.1 mb 59Fe 44.50 d β- 60Fe 1.50 Ma β- 61Fe 5.98 m β- 56Mn 2.58 h β- 57Mn 1.42 m β- 58Mn 3.00 s β- 59Mn 4.59 s β- 60Mn 51.00 s β- 55Cr 3.50 m β- 56Cr 5.94 m β- 57Cr 21.10 s β- 58Cr 7.00 s β- 59Cr 460.00 ms β-

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