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Total MACS at 30keV:

1065

±

65

mb

Cross sections do not include stellar enhancement factors!

Version	Total MACS [mb]	Partial to gs [mb]	Partial to isomer [mb]
1.0	1065 ± 65	-	-
0.0	1129 ± 56	-	-

(Version 0.0 corresponds to Bao et al.)

New rec. value is average from evaluated libraries (endfb71,jendl40). Uncertainty is deviation between libraries plus an assumed exp. uncertainty of 5%. Stellar enhancement factors corrected Rau09.
Last review: December 2013

original	renorm.	year	type	Comment	Ref
1383		2002	r	TOF; W Spall., Au	WCD02
1081 E(n)= 30 (5) keV		1982	c	Linac, TOF, 6Li+235U: ENDF/B-V, Au:Sat., k= 1.0737	MDM78,Mac82c
1564 ± 235 E(n)= 23 (5) keV		1974	c	Sb-Be, Act., 1/v(E), 127I:832 (26) mb (24 keV)	SSR74
1080		2011	e	ENDF/B-VII.1	endfb71
1053		2011	e	JENDL-4.0	jendl40
1500 ± 200		1971	e		AGM71
583		2005	t	MOST 2005	Gor05
635		2002	t	MOST 2002	Gor02
690		2000	t	NON-SMOKER	RaT99
1716		1981	t		Har81
1030		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:

r	Recalculated for kT = 30keV with the code described in Ref. 2 after renormalizing the original data to updated standard cross sections
c	Directly quoted from the reference itself
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	3259 ± 341	-	2082 ± 191	1613 ± 128	1353 ± 96	1185 ± 77	1065 ± 65	901 ± 50	793 ± 41	714 ± 37	604 ± 35	531 ± 34
Xfactor	0.68	0.56	0.47	0.39	0.35	0.33	0.30	0.27	0.23	0.20	0.16	0.13
SEF	1.07	1.11	1.14	1.18	1.22	1.24	1.26	1.29	1.32	1.35	1.37	1.38
Rate	2.07	-	1.99	1.96	1.96	1.95	1.95	1.95	1.96	1.98	1.96	1.94

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, corrected
Year: 2009
Comment:

Rate:
Reaction rate N_A<σv> given in 10⁸ cm³/mole/s, including SEF

	169Lu 1.42 d β+ 170Lu 2.01 d β+ 171Lu 8.24 d β+ 172Lu 6.70 d β+ 173Lu 1.37 a β+ 168Yb 0.13 1214 mb 169Yb 32.02 d β+ 170Yb 3.04 768 mb 171Yb 14.28 1210 mb 172Yb 21.83 341 mb 167Tm 9.25 d β+ 168Tm 93.10 d β+ 169Tm 100 1129 mb 170Tm 128.59 d 1870 mb, β- 171Tm 1.92 a 486 mb, β- 166Er 33.503 563 mb 167Er 22.869 1425 mb 168Er 26.978 338 mb 169Er 9.39 d 653 mb, β- 170Er 14.91 170 mb 165Ho 100 1280 mb 166Ho 1.12 d β- 167Ho 3.00 h β- 168Ho 2.99 m β- 169Ho 4.72 m β-

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