Issue |
EAS Publications Series
Volume 11, 2004
The Future Astronuclear Physics
|
|
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Page(s) | 227 - 234 | |
DOI | https://doi.org/10.1051/eas:2004016 | |
Published online | 12 July 2004 |
A. Jorissen, S. Goriely, M. Rayet, L. Siess and H. Boffin (eds)
EAS Publications Series, 11 (2004) 227-234
Required precision of mass and half-life measurements for r-process nuclei planned at future radioactive-ion-beam facilities
1
RIKEN, Hirosawa 2-1, Wako 351-0198, Japan
2
Senior High School of Waseda University,
Kami-Shakujii 3-31-1,
Nerima-ku, Tokyo 177-0044, Japan
3
Advanced Research Institute for Science and Engineering,
Waseda University,
Okubo 3-4-1, Shinjuku-ku, Tokyo 169-8555, Japan
4
Institut d'Astronomie et d'Astrophysique,
Université Libre de Bruxelles, CP 226, 1050 Bruxelles, Belgium
In order to understand the r-process nucleosynthesis, we evaluate the precision required for mass and β-decay half-life measurements planned at future radioactive-ion-beam facilities. To satisfy a simple requirement that we put on nuclear model predictions, it is concluded that the detectors for the mass measurements must have a precision of 1σ < ~ 250 keV, and that the detectors for the half-life measurements demand a precision of 1σ < ~ 0.15 ms. The above two specifications are required at the neutron richness of A/Z = 3.0 at the N=82 shell closure and A/Z = 2.9 at the N=50 shell closure. For the doubly magic nuclide 78Ni, a precision of 1σ < ~ 300 keV and 1σ < ~ 5 ms are required, respectively, for mass and half-life measurements. This analysis aims at providing a first rough guide for ongoing detector developments.
© EAS, EDP Sciences, 2004