https://doi.org/10.1140/epjad/i2005-06-069-1
ENAM 2004
The half-life of the doubly-magic r-process nucleus 78Ni
1
National Superconducting Cyclotron Laboratory, Michigan State University, 48824, East Lansing, MI, USA
2
Department of Physics and Astronomy, Michigan State University, 48824, East Lansing, MI, USA
3
Joint Institute for Nuclear Astrophysics, USA
4
Department of Physics, University of Notre Dame, 46556-5670, Notre Dame, IN, USA
5
Institut für Kernchemie, Universität Mainz, Fritz-Strassmann Weg 2, D-55128, Mainz, Germany
6
Department of Chemistry, Michigan State University, 48824, East Lansing, MI, USA
7
Pacific Northwest National Laboratory, MS P8-50, P.O. Box 999, 99352, Richland, WA, USA
8
Department of Chemistry and Biochemistry, University of Maryland, 20742, College Park, MD, USA
* e-mail: schatz@nscl.msu.edu
Received:
28
February
2005
Accepted:
28
February
2005
Published online:
12
May
2005
Despite a lot of experimental and theoretical progress the question of the r-process site and the origin of the heavy elements in nature remains one of the biggest open questions in nuclear astrophysics. We report first results from experiments with rare isotope beams of r-process nuclei at Michigan State University’s National Superconducting Cyclotron Laboratory. This includes a first measurement of the half-life of the doubly-magic waiting point nucleus 78Ni, which serves as a major bottle-neck for the synthesis of heavy elements in many r-process models.
PACS: 21.10.Tg Lifetimes – / 23.40.-s β decay; double β decay; electron and muon capture – / 26.50.+x Nuclear physics aspects of novae, supernovae, and other explosive environments –
© Società Italiana di Fisica and Springer-Verlag, 2005