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Experiments with neutron beams for the astrophysical s process

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...

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Autores principales:	Lederer, C, Altstadt, S, Andrzejewski, J, Audouin, L, Barbagallo, M, Bécares, V, Bečvář, F, Belloni, F, Berthoumieux, E, Billowes, J, Boccone, V, Bosnar, D, Brugger, M, Calviani, M, Calviño, F, Cano-Ott, D, Carrapiço, C, Cerutti, F, Chiaveri, E, Chin, M, Colonna, N, Cortés, G, Cortés-Giraldo, M A, Diakaki, M, Domingo-Pardo, C, Duran, I, Dressler, R, Dzysiuk, N, Eleftheriadis, C, Ferrari, A, Fraval, K, Ganesan, S, García, A R, Giubrone, G, Gómez-Hornillos, M B, Gonçalves, I F, González-Romero, E, Griesmayer, E, Guerrero, C, Gunsing, F, Gurusamy, P, Hernández-Prieto, A, Jenkins, D G, Jericha, E, Kadi, Y, Käppeler, F, Karadimos, D, Kivel, N, Koehler, P, Kokkoris, M, Korschinek, G, Krtička, M, Kroll, J, Lampoudis, C, Langer, C, Leal-Cidoncha, E, Leeb, H, Leong, L S, Losito, R, Mallick, A, Manousos, A, Marganiec, J, Martínez, T, Massimi, C, Mastinu, P F, Mastromarco, M, Meaze, M, Mendoza, E, Mengoni, A, Milazzo, P M, Mingrone, F, Mirea, M, Mondalaers, W, Paradela, C, Pavlik, A, Perkowski, J, Pignatari, M, Plompen, A, Praena, J, Quesada, J M, Rauscher, T, Reifarth, R, Riego, A, Robles, M S, Roman, F, Rubbia, C, Sabaté-Gilarte, M, Sarmento, R, Saxena, A, Schillebeeckx, P, Schmidt, S, Schumann, D, Tagliente, G, Tain, J L, Tarrío, D, Tassan-Got, L, Tsinganis, A, Valenta, S, Vannini, G, Variale, V, Vaz, P, Ventura, A, Versaci, R, Vermeulen, M J, Vlachoudis, V, Vlastou, R, Wallner, A, Ware, T, Weigand, M, Weiβ, C, Wright, T, Žugec, P
Lenguaje:	eng
Publicado:	2016
Materias:	Nuclear Physics - Experiment Astrophysics and Astronomy
Acceso en línea:	https://dx.doi.org/10.1088/1742-6596/665/1/012020 http://cds.cern.ch/record/2312111

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author	Lederer, C Altstadt, S Andrzejewski, J Audouin, L Barbagallo, M Bécares, V Bečvář, F Belloni, F Berthoumieux, E Billowes, J Boccone, V Bosnar, D Brugger, M Calviani, M Calviño, F Cano-Ott, D Carrapiço, C Cerutti, F Chiaveri, E Chin, M Colonna, N Cortés, G Cortés-Giraldo, M A Diakaki, M Domingo-Pardo, C Duran, I Dressler, R Dzysiuk, N Eleftheriadis, C Ferrari, A Fraval, K Ganesan, S García, A R Giubrone, G Gómez-Hornillos, M B Gonçalves, I F González-Romero, E Griesmayer, E Guerrero, C Gunsing, F Gurusamy, P Hernández-Prieto, A Jenkins, D G Jericha, E Kadi, Y Käppeler, F Karadimos, D Kivel, N Koehler, P Kokkoris, M Korschinek, G Krtička, M Kroll, J Lampoudis, C Langer, C Leal-Cidoncha, E Leeb, H Leong, L S Losito, R Mallick, A Manousos, A Marganiec, J Martínez, T Massimi, C Mastinu, P F Mastromarco, M Meaze, M Mendoza, E Mengoni, A Milazzo, P M Mingrone, F Mirea, M Mondalaers, W Paradela, C Pavlik, A Perkowski, J Pignatari, M Plompen, A Praena, J Quesada, J M Rauscher, T Reifarth, R Riego, A Robles, M S Roman, F Rubbia, C Sabaté-Gilarte, M Sarmento, R Saxena, A Schillebeeckx, P Schmidt, S Schumann, D Tagliente, G Tain, J L Tarrío, D Tassan-Got, L Tsinganis, A Valenta, S Vannini, G Variale, V Vaz, P Ventura, A Versaci, R Vermeulen, M J Vlachoudis, V Vlastou, R Wallner, A Ware, T Weigand, M Weiβ, C Wright, T Žugec, P
author_facet	Lederer, C Altstadt, S Andrzejewski, J Audouin, L Barbagallo, M Bécares, V Bečvář, F Belloni, F Berthoumieux, E Billowes, J Boccone, V Bosnar, D Brugger, M Calviani, M Calviño, F Cano-Ott, D Carrapiço, C Cerutti, F Chiaveri, E Chin, M Colonna, N Cortés, G Cortés-Giraldo, M A Diakaki, M Domingo-Pardo, C Duran, I Dressler, R Dzysiuk, N Eleftheriadis, C Ferrari, A Fraval, K Ganesan, S García, A R Giubrone, G Gómez-Hornillos, M B Gonçalves, I F González-Romero, E Griesmayer, E Guerrero, C Gunsing, F Gurusamy, P Hernández-Prieto, A Jenkins, D G Jericha, E Kadi, Y Käppeler, F Karadimos, D Kivel, N Koehler, P Kokkoris, M Korschinek, G Krtička, M Kroll, J Lampoudis, C Langer, C Leal-Cidoncha, E Leeb, H Leong, L S Losito, R Mallick, A Manousos, A Marganiec, J Martínez, T Massimi, C Mastinu, P F Mastromarco, M Meaze, M Mendoza, E Mengoni, A Milazzo, P M Mingrone, F Mirea, M Mondalaers, W Paradela, C Pavlik, A Perkowski, J Pignatari, M Plompen, A Praena, J Quesada, J M Rauscher, T Reifarth, R Riego, A Robles, M S Roman, F Rubbia, C Sabaté-Gilarte, M Sarmento, R Saxena, A Schillebeeckx, P Schmidt, S Schumann, D Tagliente, G Tain, J L Tarrío, D Tassan-Got, L Tsinganis, A Valenta, S Vannini, G Variale, V Vaz, P Ventura, A Versaci, R Vermeulen, M J Vlachoudis, V Vlastou, R Wallner, A Ware, T Weigand, M Weiβ, C Wright, T Žugec, P
author_sort	Lederer, C
collection	CERN
description	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.
id	oai-inspirehep.net-1646388
institution	Organización Europea para la Investigación Nuclear
language	eng
publishDate	2016
record_format	invenio
spelling	oai-inspirehep.net-16463882021-02-09T10:05:08Zdoi:10.1088/1742-6596/665/1/012020http://cds.cern.ch/record/2312111engLederer, CAltstadt, SAndrzejewski, JAudouin, LBarbagallo, MBécares, VBečvář, FBelloni, FBerthoumieux, EBillowes, JBoccone, VBosnar, DBrugger, MCalviani, MCalviño, FCano-Ott, DCarrapiço, CCerutti, FChiaveri, EChin, MColonna, NCortés, GCortés-Giraldo, M ADiakaki, MDomingo-Pardo, CDuran, IDressler, RDzysiuk, NEleftheriadis, CFerrari, AFraval, KGanesan, SGarcía, A RGiubrone, GGómez-Hornillos, M BGonçalves, I FGonzález-Romero, EGriesmayer, EGuerrero, CGunsing, FGurusamy, PHernández-Prieto, AJenkins, D GJericha, EKadi, YKäppeler, FKaradimos, DKivel, NKoehler, PKokkoris, MKorschinek, GKrtička, MKroll, JLampoudis, CLanger, CLeal-Cidoncha, ELeeb, HLeong, L SLosito, RMallick, AManousos, AMarganiec, JMartínez, TMassimi, CMastinu, P FMastromarco, MMeaze, MMendoza, EMengoni, AMilazzo, P MMingrone, FMirea, MMondalaers, WParadela, CPavlik, APerkowski, JPignatari, MPlompen, APraena, JQuesada, J MRauscher, TReifarth, RRiego, ARobles, M SRoman, FRubbia, CSabaté-Gilarte, MSarmento, RSaxena, ASchillebeeckx, PSchmidt, SSchumann, DTagliente, GTain, J LTarrío, DTassan-Got, LTsinganis, AValenta, SVannini, GVariale, VVaz, PVentura, AVersaci, RVermeulen, M JVlachoudis, VVlastou, RWallner, AWare, TWeigand, MWeiβ, CWright, TŽugec, PExperiments with neutron beams for the astrophysical s processNuclear Physics - ExperimentAstrophysics and AstronomyNeutron 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.oai:inspirehep.net:16463882016
spellingShingle	Nuclear Physics - Experiment Astrophysics and Astronomy Lederer, C Altstadt, S Andrzejewski, J Audouin, L Barbagallo, M Bécares, V Bečvář, F Belloni, F Berthoumieux, E Billowes, J Boccone, V Bosnar, D Brugger, M Calviani, M Calviño, F Cano-Ott, D Carrapiço, C Cerutti, F Chiaveri, E Chin, M Colonna, N Cortés, G Cortés-Giraldo, M A Diakaki, M Domingo-Pardo, C Duran, I Dressler, R Dzysiuk, N Eleftheriadis, C Ferrari, A Fraval, K Ganesan, S García, A R Giubrone, G Gómez-Hornillos, M B Gonçalves, I F González-Romero, E Griesmayer, E Guerrero, C Gunsing, F Gurusamy, P Hernández-Prieto, A Jenkins, D G Jericha, E Kadi, Y Käppeler, F Karadimos, D Kivel, N Koehler, P Kokkoris, M Korschinek, G Krtička, M Kroll, J Lampoudis, C Langer, C Leal-Cidoncha, E Leeb, H Leong, L S Losito, R Mallick, A Manousos, A Marganiec, J Martínez, T Massimi, C Mastinu, P F Mastromarco, M Meaze, M Mendoza, E Mengoni, A Milazzo, P M Mingrone, F Mirea, M Mondalaers, W Paradela, C Pavlik, A Perkowski, J Pignatari, M Plompen, A Praena, J Quesada, J M Rauscher, T Reifarth, R Riego, A Robles, M S Roman, F Rubbia, C Sabaté-Gilarte, M Sarmento, R Saxena, A Schillebeeckx, P Schmidt, S Schumann, D Tagliente, G Tain, J L Tarrío, D Tassan-Got, L Tsinganis, A Valenta, S Vannini, G Variale, V Vaz, P Ventura, A Versaci, R Vermeulen, M J Vlachoudis, V Vlastou, R Wallner, A Ware, T Weigand, M Weiβ, C Wright, T Žugec, P Experiments with neutron beams for the astrophysical s process
title	Experiments with neutron beams for the astrophysical s process
title_full	Experiments with neutron beams for the astrophysical s process
title_fullStr	Experiments with neutron beams for the astrophysical s process
title_full_unstemmed	Experiments with neutron beams for the astrophysical s process
title_short	Experiments with neutron beams for the astrophysical s process
title_sort	experiments with neutron beams for the astrophysical s process
topic	Nuclear Physics - Experiment Astrophysics and Astronomy
url	https://dx.doi.org/10.1088/1742-6596/665/1/012020 http://cds.cern.ch/record/2312111
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Experiments with neutron beams for the astrophysical s process

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