出版社：SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要：Rates of sub-barrier, radiative capture reactions involving radioactive
reactants, needed for understanding various astrophysical explosive scenarios, are often
quite difficult to measure directly at relevant stellar temperatures. In general relatively
intense radioactive beams (>1011/s) are needed for these inverse kinematic studies, as
cross sections are very low. A new production approach is described herein that would
supply such required intensities in a relatively straightforward fashion. While this
system may have many applications, one area could be increasing our understanding of
classical novae and X-ray bursts.
