PoS - Proceedings of Science
Volume 281 - The 26th International Nuclear Physics Conference (INPC2016) - Nuclear Astrophysics – Friday 16
Recent Results In Nuclear Astrophysics At The n-TOF Facility At CERN
G. Tagliente,* O. Aberle, J. Andrzejewski, L. Audouin, M. Bacak, J. Balibrea, M. Barbagallo, F. Bečvář, E. Berthoumieux, J. Billowes, D. Bosnar, A.K. Brown, M. Caamano, F. Calviño, M. Calviani, D. Cano-Ott, R. Cardella, A. Casanovas, F. Cerutti, Y.H. Chen, E. Chiaveri, N. Colonna, G. Cortes, M.A. Cortés-Giraldo, L. Cosentino, L.A. Damone, M. Diakaki, C. Domingo-Pardo, L.R. Dressler, E. Dupont, I. Duran, B. Fernández-Domínguez, A. Ferrari, P. Ferreira, P. Finocchiaro, V. Furman, K. Göbel, A. Garcia, A. Gawlik, S. Gilardoni, T. Glodariu, I. Goncalves, E. González, E. Griesmayer, C. Guerrero, F. Gunsing, H. Harada, S. Heinitz, J. Heyse, D.G. Jenkins, E. Jericha, F. Käppeler, Y. Kadi, A. Kalamara, P. Kavrigin, A. Kimura, N. Kivel, M. Kokkoris, M. Krticka, D. Kurtulgil, E. Leal-Cidoncha, C. Lederer, J. Lerendegui-Marco, H. Leeb, S. Lo Meo, S.J. Lonsdale, D. Macina, J. Marganiec, T. Martínez, A. Masi, C. Massimi, P. Mastinu, M. Mastromarco, E.A. Maugeri, A. Mazzone, E. Mendoza, A. Mengoni, F. Mingrone, P.M. Milazzo, A. Musumarra, A. Negret, R. Nolte, A. Oprea, N. Patronis, A. Pavlik, J. Perkowski, I. Porras, J. Praena, J. Quesada, D. Radeck, T. Rauscher, R. Reifarth, C. Rubbia, J.A. Ryan, M. Sabaté-Gilarte, A. Saxena, P. Schillebeeckx, D. Schumann, P. Sedyshev, A.R. Smith, N.V. Sosnin, A. Stamatopoulos, J.L. Tain, A. Tarifeño-Saldivia, L. Tassan-Got, S. Valenta, G. Vannini, V. Variale, P. Vaz, A. Ventura, V. Vlachoudis, R. Vlastou, A. Wallner, S. Warren, P.J. Woods, T. Wright, P.Č. Żugec on behalf of the n_TOF Collaboration
*corresponding author
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Pre-published on: May 04, 2017
Published on: May 09, 2017
Abstract
The neutron time of flight (n_TOF) facility at CERN is a spallation source characterized by a white neutron spectrum. The innovative features of the facility, in the two experimental areas, (20 m and 185 m), allow for an accurate determination of the neutron cross section for radioactive samples or for isotopes with small neutron capture cross section, of interest for Nuclear Astrophysics. The recent results obtained at n_TOF facility are presented.
DOI: https://doi.org/10.22323/1.281.0161
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