Nd2007 2007
DOI: 10.1051/ndata:07712
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From the microcosm of the atomic nuclei to the macrocosm of the stars

Abstract: Abstract.A necessary condition for the reliable modelling of the structure or evolution of the stars and of their concomitant nucleosynthesis is the availability of good quality nuclear data in a very wide area of the chart of nuclides. This short review presents a non-exhaustive list of nuclear data of astrophysics interest (masses, β-decays, thermonuclear and non-thermonuclear reaction rates) for nuclides at the bottom of the valley of nuclear stability (mainly involved in the modelling of non-explosive phas… Show more

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Cited by 3 publications
(1 citation statement)
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“…These extrapolations are essential because the relevant energy domain cannot be reached in the laboratory, except in very few cases. This situation has motivated the launch of the NACRE II compilation, which aims at revising some of the NACRE rates (Aikawa et al 2006;Katsuma 2006;Arnould & Katsuma 2007;Xu et al 2009Xu et al , 2012. In its current version, NACRE II surveys 34 two-body exothermic reactions (15 particle-transfer and 19 radiative capture reactions) on targets with A ≤ 16 listed in Table 1.…”
Section: Experiment-based Reaction Rates: the Nacre II Compilationmentioning
confidence: 99%
“…These extrapolations are essential because the relevant energy domain cannot be reached in the laboratory, except in very few cases. This situation has motivated the launch of the NACRE II compilation, which aims at revising some of the NACRE rates (Aikawa et al 2006;Katsuma 2006;Arnould & Katsuma 2007;Xu et al 2009Xu et al , 2012. In its current version, NACRE II surveys 34 two-body exothermic reactions (15 particle-transfer and 19 radiative capture reactions) on targets with A ≤ 16 listed in Table 1.…”
Section: Experiment-based Reaction Rates: the Nacre II Compilationmentioning
confidence: 99%