出版社：SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要：Photodissociation reactions are of crucial interest for the network calculations of stellar nucleosynthesis.
On the one hand, they are directly used in p-process scenarios changing s- and rprocess
seed distributions to the observed abundance patterns. On the other hand, the study of
(g,n) reactions helps to constrain theoretical predictions on the (n,g) cross sections of the branching
points on the s-process path. The current status of different experimental efforts is presented
and recent developments are discussed.
