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Total MACS at 30keV:

574

±

25

mb

Cross sections do not include stellar enhancement factors!

Version	Total MACS [mb]	Partial to gs [mb]	Partial to isomer [mb]
1.0	574 ± 25	-	-
0.0	515 ± 15	-	-

(Version 0.0 corresponds to Bao et al.)

Rec. value is average of recent evaluations (endfb71,jendl40). Uncertainty is from standard deviation of ca. 5% given in endfb71.
Last review: January 2014

original	renorm.	year	type	Comment	Ref
581 ± 27 E(n)= 30 (2) keV		1987	c	VdG, TOF, 7Li(p,n); Au+Ag+Nd+Ta+W:Sat.	BKK87
515 ± 15		1983	b	Linac, TOF, 6Li, Au:Sat.	MDA83
550		1969	c	Linac, TOF, 6Li, Au:Sat., quoted from BKW82	BHM69
575.3 ± 25.5		2011	e	ENDF/B-VII.1	endfb71
572.7		2011	e	JENDL-4.0	jendl40
528.6		2006	e	ENDF/B-VII.0	endfb7
453.1		2004	e	JEFF-3.1	jeff31
453.1		2002	e	JENDL-3.3	jendl33
550 ± 50		1971	e		AGM71
681		2005	t	MOST 2005	Gor05
1098		2002	t	MOST 2002	Gor02
701		2000	t	NON-SMOKER	RaT99
618 ± 75		1991	t		KJB91
1038		1981	t		Har81
1010		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	1786 ± 88	-	1131 ± 52	880 ± 39	738 ± 33	643 ± 28	574 ± 25	477 ± 21	411 ± 19	364 ± 17	298 ± 14	255 ± 12
Xfactor	1.00	0.99	0.98	0.90	0.79	0.69	0.60	0.46	0.37	0.30	0.21	0.15
SEF	1.00	1.00	1.01	1.02	1.04	1.06	1.08	1.13	1.17	1.20	1.26	1.31
Rate	1.06	-	0.95	0.92	0.91	0.90	0.90	0.90	0.90	0.90	0.89	0.89

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 10⁸ cm³/mole/s, including SEF

	183Os 13.00 h β+ 184Os 0.02 590 mb 185Os 93.60 d β+ 186Os 1.59 422 mb 187Os 1.6 896 mb 182Re 2.67 d β+ 183Re 70.00 d β+ 184Re 38.00 d β+ 185Re 37.4 1535 mb 186Re 3.72 d 1550 mb, β- 181W 121.20 d β+ 182W 26.5 274 mb 183W 14.31 515 mb 184W 30.64 223 mb 185W 75.10 d 703 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- 184Ta 8.70 h β- 179Hf 13.62 956 mb 180Hf 35.08 179 mb 181Hf 42.39 d 194 mb, β- 182Hf 8.90 Ma 117 mb, β- 183Hf 1.07 h β-

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