出版社：SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要：The 12C(a,g )16O reaction remains an ongoing problem in Nuclear Astrophysics and has thus
drawn lots of attention over the past decades. The reason is for one its exceptional importance for
the nucleosynthesis products and even the dynamics of massive stars. The other reason is that it is
extremely difficult to determine the reaction cross section at astrophysically relevant energies.
