The Role of Fe and Ni for S-process Nucleosynthesis and Innovative Nuclear Technologies

Author(s)

Giuseppe Giubrone, Jose Luis Tain, Claudia Lederer, Andreas Pavlik, Anton Wallner, Samuel Andriamonje, Markus Brugger, M Calviani, Fabio Cerutti, E Chiaveri, Arnaud Ferrari, Yacine Kadi, Elias Lebbos, Vassilis Vlachoudis, J Andrzejewski, J Marganiec, J. Perlowski, Ludmila Audouin, B Berthier, Laurent Tassan-Got, Vlad Avrigeanu, Mihail Mirea, Vicente Bécares, Daniel Cano Ott, Manuel Fernández-Ordóñez, E Gonzalez - Romero, Carlos Guerrero, Francisco Martin-Fuertes, Trinitario Martinez, Emilio Mendoza, Gabriel Pina, Javier Quinones, Frantisek Becvar, Frank Gunsing, Francisco Calvino, Guillem Cortes, M. Belén Gómez Hornillo, C. Carrapico, Isabel Maria Ferro Goncalves, Raúl Sarmento, Pedro Vaz, N Colonna, S Marrone, Moinul Haque Meaze, Giuseppe Tagliente, Vincenzo Variale, Iris Dillmann, César Domingo-Pardo, Michael Heil, I Duran, Carlos Paradela, Diego Tarrio, S. Ganesan, F Gramegna, P F Mastinu, Sotirios Harrisopulos, K G Ioannides, Dimitrios Karadimos, E Jericha, Helmut Leeb, C. Weiß, Franz Käppeler, M Lozano, Javier Praena, Jose Manuel Quesada Molina, Cristian Massimi, Gianni Vannini, Alberto Mengoni, A Ventura, Marita Mosconi, R Nolte, R Vlastou

Abstract

The accurate measurement of neutron capture cross sections of all Fe and Ni isotopes is important for disentangling the contribution of the s-process and the r-process to the stellar nucleosynthesis of elements in the mass range 60 <A <120. At the same time, Fe and Ni are important components of structural materials and improved neutron cross section data is relevant in the design of new nuclear systems. With the aim of obtaining improved capture data on all stable iron and nickel isotopes, a program of measurements has been launched at the CERN Neutron Time of Flight Facility n_TOF.

Organisation(s)

Isotope Physics

External organisation(s)

Universitat de València, European Organization for Nuclear Research (CERN), University of Lodz, Centre National De La Recherche Scientifique (CNRS), Institut de Physique Nucléaire d'Orsay (IPN), Horia Hulubei National Institute for R&D in Physics and Nuclear Engineering, Centro de Investigaciones Energeticas Medioambientales y Tecnológica, Charles University Prague, French Alternative Energies and Atomic Energy Commission (CEA), Universitat Politècnica de Catalunya, Instituto Superior Técnico, Nuclear and Technological Institute (ITN), Istituto Nazionale di Fisica Nucleare (INFN), Roma, Technische Universität München, GSI Helmholtzzentrum für Schwerionenforschung, Universidade de Santiago de Compostela (USC), Bhabha Atomic Research Center, National Centre for Scientific Research Demokritos (NCSR), University of Ioannina, Technische Universität Wien, Karlsruher Institut für Technologie, Universidad de Sevilla, Italian National Agency for New Technologies, Energy and Sustainable Economic Development, Physikalisch-Technische Bundesanstalt, National Technical University of Athens (NTUA)

Journal

Journal of the Korean Physical Society

Volume

59

Pages

2106-2109

No. of pages

4

ISSN

0374-4884

DOI

https://doi.org/10.3938/jkps.59.2106

Publication date

2011

Peer reviewed

Yes

Austrian Fields of Science 2012

103005 Atomic physics, 103004 Astrophysics

Portal url

https://ucrisportal.univie.ac.at/en/publications/cd68423e-e425-41b0-b7da-4144b5c7f098