Experiments with neutron beams for the astrophysical s process

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To access the full text documents, please follow this link: http://hdl.handle.net/2117/96479

dc.contributor	Universitat Politècnica de Catalunya. Departament de Física
dc.contributor	Universitat Politècnica de Catalunya. ANT - Advanced Nuclear Technologies Research Group
dc.contributor.author	Lederer, Claudia
dc.contributor.author	Altstadt, Sebastian
dc.contributor.author	Andrzejewski, Józef
dc.contributor.author	Calviño Tavares, Francisco
dc.contributor.author	Cortés Rossell, Guillem Pere
dc.contributor.author	Gómez Hornillos, María Belén
dc.date	2013
dc.identifier.citation	Lederer, C., Altstadt , S., Andrzejewski, J., Calviño, F., Cortes, G., Gómez-Hornillos, M.B. Experiments with neutron beams for the astrophysical s process. A: Nuclear Physics in Astrophysics. "Journal of Physics: Conference Series, vol. 665, no. 1, January 5, 2016". Lisboa: Institute of Physics (IOP), 2013, p. 1-6.
dc.identifier.citation	10.1088/1742-6596/665/1/012020
dc.identifier.uri	http://hdl.handle.net/2117/96479
dc.language.iso	eng
dc.publisher	Institute of Physics (IOP)
dc.relation	http://iopscience.iop.org/article/10.1088/1742-6596/665/1/012020
dc.relation	info:eu-repo/grantAgreement/ES/6PN/FPA2008-04972-C03-03
dc.rights	info:eu-repo/semantics/openAccess
dc.rights	http://creativecommons.org/licenses/by-nc-nd/3.0/es/
dc.subject	Àrees temàtiques de la UPC::Física::Astronomia i astrofísica
dc.subject	Àrees temàtiques de la UPC::Energies::Energia nuclear
dc.subject	Astrophysics
dc.subject	Neutrons
dc.subject	Astrophysics
dc.subject	Neutron
dc.subject	Cross section
dc.subject	Astrofísica
dc.subject	Neutrons
dc.title	Experiments with neutron beams for the astrophysical s process
dc.type	info:eu-repo/semantics/publishedVersion
dc.type	info:eu-repo/semantics/conferenceObject
dc.description.abstract	Neutron capture cross sections are the key nuclear physics input to study the slow neutron capture process, which is responsible for forming about half of the elemental abundances above Fe. Stellar neutron capture cross section can be measured by the time-of-flight technique, or by activation. Both techniques will be discussed and recent experiments in the Fe/Ni mass region will be presented.

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