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The nucleosynthesis of heavy elements in stars: the key isotope 25Mg

Opened Access The nucleosynthesis of heavy elements in stars: the key isotope 25Mg

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Autor: Cortés Giraldo, Miguel Antonio
Praena Rodríguez, Javier
Quesada Molina, José Manuel
Sabaté Gilarte, Marta
Mingrone, F
Massimi, Christian
Vannini, Gianni
Departamento: Universidad de Sevilla. Departamento de Física Atómica, Molecular y Nuclear
Fecha: 2014
Publicado en: EPJ Web of Conferences, 66, 07016-1-07016-4.
Tipo de documento: Artículo
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 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.
Tamaño: 397.6Kb
Formato: PDF

URI: http://hdl.handle.net/11441/49382

DOI: 10.1051/epjconf/20146607016

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