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The nucleosynthesis of heavy elements in Stars: the key isotope 25Mg
- Publication Year :
- 2014
-
Abstract
- We have measured the radiative neutron-capture cross section and the total neutron-induced cross section of one of the most important isotopes for the s process, the 25Mg. The measurements have been carried out at the neutron time-of-flight facilities n_TOF at CERN (Switzerland) and GELINA installed at the EC-JRC-IRMM (Belgium). The cross sections as a function of neutron energy have been measured up to approximately 300 keV, covering the energy region of interest to the s process. The data analysis is ongoing and preliminary results show the potential relevance for the s process.
- Subjects :
- Astrophysics::High Energy Astrophysical Phenomena
ddc:530
Nuclear Experiment
Subjects
Details
- Language :
- English
- Database :
- OpenAIRE
- Accession number :
- edsair.od.......603..2d0edd9423ac4edf475aacf7df89e802