Nuclear astrophysics with secondary (radioactive) beams

Details Nuclear astrophysics with secondary (radioactive) beams Nuclear astrophysics with secondary (radioactive) beams

Mar 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994nupha.570...87g&link_type=abstract

Nuclear Physics A, Volume 570, Issue 1-2, p. 87-100.

Physics

Nuclear Physics

Scientific paper

Some problems in nuclear astrophysics are discussed with emphasize on problems central to the field which were not solved over the last two decades, including helium burning in massive stars and the 12C(α,γ)16O reaction, as well as the 8B solar neutrino flux and the 7Be(p, γ)8B reaction. It will be demonstrated that these problems could be solved by measuring the time reversed process(es), such as the beta-delayed alpha-particle emission of 16N and the Coulomb Dissociation of 8B, using radioactive beams (of 8B and 16N), that allow for amplification of the sought for small cross section, of relevance for stellar processes.

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