Experiments with neutron beams for the astrophysical s process

C Lederer; S Altstadt; J Andrzejewski; L Audouin; M Barbagallo; V Bécares; F Bečvář; F Belloni; E Berthoumieux; J Billowes; V Boccone; D Bosnar; M Brugger; M Calviani; F Calviño; D Cano-Ott; C Carrapiço; F Cerutti; E Chiaveri; M Chin; N Colonna; G Cortés; M A Cortés-Giraldo; M Diakaki; C Domingo-Pardo; I Duran; R Dressler; N Dzysiuk; C Eleftheriadis; A Ferrari; K Fraval; S Ganesan; A R García; G Giubrone; M B Gómez-Hornillos; I F Gonçalves; E González-Romero; E Griesmayer; C Guerrero; F Gunsing; P Gurusamy; A Hernández-Prieto; D G Jenkins; E Jericha; Y Kadi; F Käppeler; D Karadimos; N Kivel; P Koehler; M Kokkoris; G Korschinek; M Krtička; J Kroll; C Lampoudis; C Langer; E Leal-Cidoncha; H Leeb; L S Leong; R Losito; A Mallick; A Manousos; J Marganiec; T Martínez; C Massimi; P F Mastinu; M Mastromarco; M Meaze; E Mendoza; A Mengoni; P M Milazzo; F Mingrone; M Mirea; W Mondalaers; C Paradela; A Pavlik; J Perkowski; M Pignatari; A Plompen; J Praena; J M Quesada; T Rauscher; R Reifarth; A Riego; M S Robles; F Roman; C Rubbia; M Sabaté-Gilarte; R Sarmento; A Saxena; P Schillebeeckx; S Schmidt; D Schumann; G Tagliente; J L Tain; D Tarrío; L Tassan-Got; A Tsinganis; S Valenta; G Vannini; V Variale; P Vaz; A Ventura; R Versaci; M J Vermeulen; V Vlachoudis; R Vlastou; A Wallner; T Ware; M Weigand; C Weiβ; T Wright; P Žugec

doi:10.1088/1742-6596/665/1/012020

Paper • The following article is Open access

Experiments with neutron beams for the astrophysical s process

C Lederer^1,2,34, S Altstadt¹, J Andrzejewski³, L Audouin⁴, M Barbagallo⁵, V Bécares⁶, F Bečvář⁷, F Belloni⁸, E Berthoumieux^8,9, J Billowes¹⁰, V Boccone⁹, D Bosnar¹¹, M Brugger⁹, M Calviani⁹, F Calviño¹², D Cano-Ott⁶, C Carrapiço¹³, F Cerutti⁹, E Chiaveri^8,9, M Chin⁹, N Colonna⁵, G Cortés¹², M A Cortés-Giraldo¹⁴, M Diakaki¹⁵, C Domingo-Pardo¹⁶, I Duran¹⁷, R Dressler¹⁸, N Dzysiuk¹⁹, C Eleftheriadis²⁰, A Ferrari⁹, K Fraval⁸, S Ganesan²¹, A R García⁶, G Giubrone¹⁶, M B Gómez-Hornillos¹², I F Gonçalves¹³, E González-Romero⁶, E Griesmayer²², C Guerrero⁹, F Gunsing⁸, P Gurusamy²¹, A Hernández-Prieto^9,12, D G Jenkins²³, E Jericha²², Y Kadi⁹, F Käppeler²⁴, D Karadimos¹⁵, N Kivel¹⁸, P Koehler²⁵, M Kokkoris¹⁵, G Korschinek²⁶, M Krtička⁷, J Kroll⁷, C Lampoudis⁸, C Langer¹, E Leal-Cidoncha¹⁷, H Leeb²², L S Leong⁴, R Losito⁹, A Mallick²¹, A Manousos²⁰, J Marganiec³, T Martínez⁶, C Massimi²⁷, P F Mastinu¹⁹, M Mastromarco⁵, M Meaze⁵, E Mendoza⁶, A Mengoni²⁸, P M Milazzo²⁹, F Mingrone²⁷, M Mirea³⁰, W Mondalaers³¹, C Paradela¹⁷, A Pavlik², J Perkowski³, M Pignatari³², A Plompen³¹, J Praena¹⁴, J M Quesada¹⁴, T Rauscher³², R Reifarth¹, A Riego¹², M S Robles¹⁷, F Roman^9,30, C Rubbia^9,33, M Sabaté-Gilarte¹⁴, R Sarmento¹³, A Saxena²¹, P Schillebeeckx³¹, S Schmidt¹, D Schumann¹⁸, G Tagliente⁵, J L Tain¹⁶, D Tarrío¹⁷, L Tassan-Got⁴, A Tsinganis⁹, S Valenta⁷, G Vannini²⁷, V Variale⁵, P Vaz¹³, A Ventura²⁸, R Versaci⁹, M J Vermeulen²³, V Vlachoudis⁹, R Vlastou¹⁵, A Wallner², T Ware¹⁰, M Weigand¹, C Weiβ²², T Wright¹⁰ and P Žugec¹¹

Published under licence by IOP Publishing Ltd
Journal of Physics: Conference Series, Volume 665, Nuclear Physics in Astrophysics VI (NPA6) 19–24 May 2013, Lisbon, Portugal

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Author affiliations

¹ Johann-Wolfgang-Goethe Universität, Frankfurt, Germany

² University of Vienna, Faculty of Physics, Austria

³ Uniwersytet Łódzki, Lodz, Poland

⁴ Centre National de la Recherche Scientifique/IN2P3 - IPN, Orsay, France

⁵ Istituto Nazionale di Fisica Nucleare, Bari, Italy

⁶ Centro de Investigaciones Energeticas Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain

⁷ Charles University, Prague, Czech Republic

⁸ Commissariat à l'Énergie Atomique (CEA) Saclay - Irfu, Gif-sur-Yvette, France

⁹ European Organization for Nuclear Research (CERN), Geneva, Switzerland

¹⁰ University of Manchester, Oxford Road, Manchester, UK

¹¹ Department of Physics, Faculty of Science, University of Zagreb, Croatia

¹² Universitat Politecnica de Catalunya, Barcelona, Spain

¹³ Instituto Tecnológico e Nuclear, Instituto Superior Técnico, Universidade Técnica de Lisboa, Lisboa, Portugal

¹⁴ Universidad de Sevilla, Spain

¹⁵ National Technical University of Athens (NTUA), Greece

¹⁶ Instituto de Física Corpuscular, CSIC-Universidad de Valencia, Spain

¹⁷ Universidade de Santiago de Compostela, Spain

¹⁸ Paul Scherrer Institut, Villigen PSI, Switzerland

¹⁹ Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di Legnaro, Italy

²⁰ Aristotle University of Thessaloniki, Thessaloniki, Greece

²¹ Bhabha Atomic Research Centre (BARC), Mumbai, India

²² Atominstitut, Technische Universität Wien, Austria

²³ University of York, Heslington, York, UK

²⁴ Karlsruhe Institute of Technology, Campus Nord, Institut für Kernphysik, Karlsruhe, Germany

²⁵ Department of Physics, University of Oslo, N-0316 Oslo, Norway

²⁶ Physik Department E12 and Excellence Cluster Universe, Technische Universität München, Munich, Germany

²⁷ Dipartimento di Fisica, Università di Bologna, and Sezione INFN di Bologna, Italy

²⁸ Agenzia nazionale per le nuove tecnologie, l'energia e lo sviluppo economico sostenibile (ENEA), Bologna, Italy

²⁹ Istituto Nazionale di Fisica Nucleare, Trieste, Italy

³⁰ Horia Hulubei National Institute of Physics and Nuclear Engineering - IFIN HH, Bucharest - Magurele, Romania

³¹ European Commission JRC, Institute for Reference Materials and Measurements, Retieseweg 111, B-2440 Geel, Belgium

³² Department of Physics and Astronomy - University of Basel, Basel, Switzerland

³³ Laboratori Nazionali del Gran Sasso dell'INFN, Assergi (AQ),Italy

³⁴ Present Address: School of Physics and Astronomy, University of Edinburgh, UK

Citation

C Lederer et al 2016 J. Phys.: Conf. Ser. 665 012020

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DOI

https://doi.org/10.1088/1742-6596/665/1/012020

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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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