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Total MACS at 30keV:

285

±

11

mb

Cross sections do not include stellar enhancement factors!

Version	Total MACS [mb]	Partial to gs [mb]	Partial to isomer [mb]
1.0	285 ± 11	-	-
0.0	274 ± 8	-	-

(Version 0.0 corresponds to Bao et al.)

Rec. value is average of recent evaluations (endfb71,jendl40). Uncertainty is from standard deviation of ca. 4% given in endfb71.
Last review: January 2014

original	renorm.	year	type	Comment	Ref
286 ± 13 E(n)= 30 (2) keV		1987	c	VdG, TOF, 7Li(p,n); Au+Ag+Nd+Ta+W:Sat.	BKK87
274 ± 8		1983	b	Linac, TOF, 6Li, Au:Sat.	MDA83
322		1969	c	Linac, TOF, 6Li, Au:Sat., quoted from BKW82	BHM69
292 ± 11		2011	e	ENDF/B-VII.1 incl. standard deviation	endfb71
278.5		2011	e	JENDL-4.0	jendl40
303.1		2006	e	ENDF/B-VII.0	endfb7
274.1		2004	e	JEFF-3.1	jeff31
274.1		2002	e	JENDL-3.3	jendl33
260 ± 30		1971	e		AGM71
405		2005	t	MOST 2005	Gor05
441		2002	t	MOST 2002	Gor02
394		2000	t	NON-SMOKER	RaT99
358 ± 46		1991	t		KJB91
365		1981	t		Har81
448		1976	t		HWF76

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
b	Calculated from smooth cross sections with model fit: ln(sigma) = a + a1 ln(E) + a2 ln^2(E)
e	Evaluated value taken directly from the reference
t	Theoretical value

Energy	5keV	8keV	10keV	15keV	20keV	25keV	30keV	40keV	50keV	60keV	80keV	100keV
MACS	785 ± 25	-	499 ± 18	400 ± 15	347 ± 13	312 ± 12	285 ± 11	246 ± 10	218 ± 9	197 ± 8	167 ± 7	148 ± 6
Xfactor	1.00	1.00	1.00	0.99	0.95	0.88	0.79	0.62	0.49	0.40	0.28	0.21
SEF	1.00	1.00	1.00	1.00	1.01	1.04	1.07	1.14	1.20	1.26	1.37	1.46
Rate	4.65	-	4.18	4.12	4.18	4.30	4.43	4.70	4.91	5.10	5.41	5.75

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 N_A<σv> given in 10⁷ cm³/mole/s, including SEF

	182Os 22.10 h β+ 183Os 13.00 h β+ 184Os 0.02 590 mb 185Os 93.60 d β+ 186Os 1.59 422 mb 181Re 19.90 h β+ 182Re 2.67 d β+ 183Re 70.00 d β+ 184Re 38.00 d β+ 185Re 37.4 1535 mb 180W 0.12 660 mb 181W 121.20 d β+ 182W 26.5 274 mb 183W 14.31 515 mb 184W 30.64 223 mb 179Ta 1.82 a 1334 mb, β+ 180Ta 8.15 h 1640 mb, β+ 181Ta 99.988 766 mb 182Ta 114.43 d 1120 mb, β- 183Ta 5.10 d β- 178Hf 27.28 314 mb 179Hf 13.62 956 mb 180Hf 35.08 179 mb 181Hf 42.39 d 194 mb, β- 182Hf 8.90 Ma 117 mb, β-

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