KADoNiS - Karlsruhe Astrophysical Database of Nucleosynthesis in Stars

Karlsruhe Astrophysical Database of Nucleosynthesis in Stars

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¹⁸⁴Os ¹⁸⁶Os ¹⁸⁷Os ¹⁸⁸Os ¹⁸⁹Os ¹⁹⁰Os ¹⁹¹Os ¹⁹²Os

¹⁸⁴Os

¹⁸⁵Os

Total MACS at 30keV:

590

Cross sections do not include stellar enhancement factors!

Version	Total MACS [mb]	Partial to gs [mb]	Partial to isomer [mb]
0.3	590 ± 39	-	-
0.0	657 ± 202*	-	-

(Version 0.0 corresponds to Bao et al.)

Last review: July 9th, 2009

original	renorm.	year	type	Comment	Ref
590 ± 39		2009	c	VdG, Act., Au:RaK88	MDD09c
400		1971	s		AGM71
789		2000	t		RaT99
480		1981	t		Har81
869		1976	t		HWF76
693		2002	t	MOST 2002	Gor02
705		2005	t	MOST 2005	Gor05

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
s	Semiempirical estimates given in the reference
t	Theoretical value

Energy	5keV	10keV	15keV	20keV	25keV	30keV	40keV	50keV	60keV	80keV	100keV
MACS	1564	1021	816	708	639	590 ± 39	524	478	445	396	364
SEF	1.00	1.00	1.00	1.00	1.02	1.04	1.08	1.14	1.18	1.26	1.33
Rate	9.27	8.56	8.39	8.44	8.61	8.88	9.53	10.18	10.79	11.83	12.84

MACS:
Reference: MDD09c,RaT99
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: 2009

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

Rate:
Reaction rate N_A<σv> given in 10⁷ cm³/mole/s, including SEF

¹⁸⁴Pt 17.30 m β⁺	¹⁸⁵Pt 1.18 h β⁺	¹⁸⁶Pt 2.08 h β⁺	¹⁸⁷Pt 2.35 h β⁺	¹⁸⁸Pt 10.20 d β⁺
¹⁸³Ir 57.00 m β⁺	¹⁸⁴Ir 3.09 h β⁺	¹⁸⁵Ir 14.40 h β⁺	¹⁸⁶Ir 16.64 h β⁺	¹⁸⁷Ir 10.50 h β⁺
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

Isotope: Osmium