Reaction Rates for H-burning in Stars from Experiments with Radioactive Nuclear Beams

Abstract

In this lecture some of the indirect methods for nuclear astrophysics that can be applied to extract reaction rates for H‐burning in stars are treated. Instead of reviewing all methods, I chose for exemplification four different experiments of our Texas A&M group, each involving a different method, but all related to the study of the proton rich nucleus 23Al. They involve the use of radioactive nuclear beams. I will describe the use of one‐nucleon transfer reactions (the ANC method), breakup reactions at intermediate energies, β‐decay and β‐delayed proton‐decay to extract nuclear structure information that is then used for nuclear astrophysics. I will show the specificities of each method, talk about their complementarities and redundancies.