Experimental determination of astrophysical reaction rates with radioactive nuclear beams
β Scribed by Shigeru Kubono
- Publisher
- Elsevier Science
- Year
- 2001
- Tongue
- English
- Weight
- 394 KB
- Volume
- 693
- Category
- Article
- ISSN
- 0375-9474
No coin nor oath required. For personal study only.
β¦ Synopsis
This paper is dedicated to the memory of our friend and the world-leader of RIB science, Jerry Garrett who made a great contribution to the promotion of RIB science.
π SIMILAR VOLUMES
The 19Ne(p,y)\*% a as well as the '9Ne(d,n)2%a reaction have been studied in inverse kinematics using '"Ne radioactive beams. Upper and lower limits for the '9Ne(p,y)20Na astrophysical reaction rate have been deduced, for the first time on the basis of direct experimental data. It is concluded that
Intermediate-energy projectile Coulomb excitation of the unstable nucleus 18 F g.s. and its short-lived E x ΒΌ 1.1 MeV (J p ΒΌ 5 + ) isomeric state (t 1/2 ΒΌ 162 ns) 18 F m have been studied at 30 MeV per nucleon. Radioactive beams of 18 F g.s. and 18 F m nuclei were produced by nucleon transfer on a c
Experimental data on ground-and excited-state properties for all nuclei with mass number A=144 have been compiled and evaluated. States populated in radioactive decay as well as in nuclear reactions have been considered. For these nuclei, level and decay schemes have been built, as well as tables of