Radioactive ion beams and explosive nucleosynthesis

Details Radioactive ion beams and explosive nucleosynthesis Radioactive ion beams and explosive nucleosynthesis

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991nimpb..56..536g&link_type=abstract

Nuclear Instruments and Methods in Physics Research Section B, Volume 56, p. 536-539.

Physics

1

Scientific paper

Explosive hydrogen burning involves (p, γ) reactions on proton-rich, unstable nuclei. The knowledge of the reaction rates for these reactions is important to calculate the energy production and reaction paths in different astrophysical scenarios, e.g. nova, supernova and supermassive stars. A direct measurement of these reaction rates requires the use of radioactive ion beams. Two examples, 13N(p, γ)14O and 19Ne(p, γ)20Na, are used to define demands, which such a facility should meet to enable the direct measurements of these reaction rates.

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