Artículo
The nucleosynthesis of heavy elements in stars: the key isotope 25Mg
Autor/es | Cortés Giraldo, Miguel Antonio
Praena Rodríguez, Javier Quesada Molina, José Manuel Sabaté Gilarte, Marta Mingrone, F Massimi, C. Vannini, Gianni |
Departamento | Universidad de Sevilla. Departamento de Física Atómica, Molecular y Nuclear |
Fecha de publicación | 2014 |
Fecha de depósito | 2016-11-30 |
Publicado en |
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Resumen | 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 ... 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 |
Cita | Cortés Giraldo, M.A., Praena Rodríguez, J., Quesada Molina, J.M., Sabaté Gilarte, M., Mingrone, F., Massimi, C. y Vannini, G. (2014). The nucleosynthesis of heavy elements in stars: the key isotope 25Mg. EPJ Web of Conferences, 66, 07016-1-07016-4. |
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