Over the past three years, we have worked on developing a well-characterized
30S radioactive beam to be used in a future experiment aiming to directly
measure the 30S(alpha,p) stellar reaction rate within the Gamow window of Type
I X-ray bursts.
Authors
Kahl D; Chen AA; Kubono S; Binh DN; Chen J; Hashimoto T; Hayakawa S; Kaji D; Kim A; Kurihara Y