Nuclear astrophysics projects at the low-energy RI beam separator CRIB
oleh: Yamaguchi H., Kahl D., Hayakawa S., Yang L., Shimizu H., Sakaguchi Y., Abe K., Nakao T., Suhara T., Iwasa N., Kim A., Kim D.H., Cha S.M., Kwag M.S., Lee J.H., Lee E.J., Chae K.Y., Wakabayashi Y., Imai N., Kitamura N., Lee P., Moon J.Y., Lee K.B., Akers C., Jung H.S., Duy N.N., Khiem L.H., Lee C.S., Hashimoto T., Kubono S., Kawabata T., Teranishi T., Kwon Y.K., Binh D.N.
| Format: | Article |
|---|---|
| Diterbitkan: | EDP Sciences 2017-01-01 |
Deskripsi
Studies on nuclear reactions relevant for astrophysics have been performed using the radioactive-isotope (RI) beams at the low-energy RI beam separator CRIB, operated by Center for Nuclear Study (CNS), the University of Tokyo. A type of measurement to study astrophysical reactions at CRIB is by the elastic resonant scattering with the thick-target method in inverse kinematics. We introduce the α resonant scattering with 7Be beam, related to the astrophysical 7Be(α, γ) reactions, which is relevant in the hot p-p chain and νp-process in supernovae. Other α resonant scattering measurements with 30S, 10Be, 15O, and 18Ne beams have been performed at CRIB, using the thick-target method.