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The nucleosynthesis of heavy elements in Stars: the key isotope25Mg

The key isotope 25Mg

descriptionPublicationkeyboard_double_arrow_right Article , Conference object , Journal 01 Jan 2014 Croatia, Austria, Austria, Croatia, Italy, Spain, Spain, Spain Publisher:EDP SciencesJournal:EPJ Web of Conferences, volume 66, page 7,016 (eissn: 2100-014X,

Authors: Srinivasan Ganesan; E. Griesmayer; A. K. Saxena; C. Lampoudis; E. Leal-Cidoncha; F. Gunsing; T. Martinez; +98 Authors

doi: 10.1051/epjconf/20146607016

handle: 20.500.12079/5049 , 11585/571873

The nucleosynthesis of heavy elements in Stars: the key isotope25Mg

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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.

Countries

Croatia, Austria, Austria, Croatia, Italy, Spain, Spain, Spain

Related Organizations

Goethe University Frankfurt
Germany
European Organization for Nuclear Research
Switzerland
Uniwersytet Łódzki (University of Lodz)
Poland
Instituto Tecnologico e Nuclear
Portugal
National Technical University of Athens
Greece

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Keywords

:Energies::Energia nuclear [Àrees temàtiques de la UPC], 103014 Kernphysik, Physics, QC1-999, 25Mg ; stellar nucleosynthesis ; neutron capture, Nuclear energy, Àrees temàtiques de la UPC::Energies::Energia nuclear, 25Mg, Physics and Astronomy (all), stellar nucleosynthesis, Energia nuclear, 103014 Nuclear physics, neutron capture

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