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Astrophysics at n_TOF facility
G. Tagliente1, U. Abbondanno2, G. Aerts3, H. Alvarez4, F. Alvarez-Velarde5, S. Andriamonje3, J. Andrzejewski6, P. Assimakopoulos7, L. Audouin8, G. Badurek9, P. Baumann10, F. Becvar11, F. Belloni2, E. Berthoumieux3, S. Bisterzo12, F. Calvino13, M. Calviani14, D. Cano-Ott5, R. Capote15,16, C. Carrapico17, P. Cennini18, V. Chepel19, E. Chiaveri18, N. Colonna1, G. Cortes13, A. Couture20, J. Cox20, M. Dahlfors18, S. David10, I. Dillman8, C. Domingo-Pardo21, W. Dridi3, I. Duran4, C. Eleftheriadis22, M. Embid-Segura5, L. Ferrant12, A. Ferrari18, R. Ferreira-Marques19, K. Fujii2, W. Furman24, R. Gallino12, I. Goncalves19, E. Gonzalez-Romero5, F. Gramegna14, C. Guerrero5, F. Gunsing3, B. Haas25, R. Haight26, M. Heil8, A. Herrera-Martinez18, M. Igashira27, E. Jericha9, F. Kappeler8, Y. Kadi18, D. Karadimos7, D. Karamanis7, M. Kerveno10, P. Koehler28, E. Kossionides29, M. Krticka11, C. Lamboudis22, H. Leeb9, A. Lindote19, I. Lopes19, M. Lozano16, S. Lukic10, J. Marganiec6, S. Marrone1, T. Martinez5, C. Massimi30, P. Mastinu14, A. Mengoni15, P. M. Milazzo2, C. Moreau2, M. Mosconi8, F. Neves19, H. Oberhummer9, S. O'Brien20, J. Pancin3, C. Papachristodoulou7, C. Papadopoulos31, C. Paradela4, N. Patronis7, A. Pavlik32, P. Pavlopoulos33, L. Perrot3, M. T. Pigni9, R. Plag8, A. Plompen34, A. Plukis3, A. Poch13, J. Praena14, C. Pretel13, J. Quesada16, T. Rauscher35, R. Reifarth26, C. Rubbia36, G. Rudolf10, P. Rullhusen34, J. Salgado17, C. Santos17, L. Sarchiapone18, I. Savvidis22, C. Stephan23, J. L. Tain21, L. Tassan-Got23, L. Tavora17, R. Terlizzi1, G. Vannini30, P. Vaz17, A. Ventura37, D. Villamarin5, M. C. Vincente5, V. Vlachoudis18, R. Vlastou31, F. Voss9, S. Walter8, H. Wendler18, M. Wiescher20, K. Wisshak8 (The n_TOF Collaboration)
1INFN, Trieste, Italy
2INFN, Bari, Italy
3CEA/Saclay, Gif-sur-Yvette, France
4Univ. Santiago de Compostela, Spain
5CIEMAT, Madrid, Spain
6Univ. Lodz, Poland
7Univ. Ioannina, Greece
8FZK, Institut für Kernphysik, Germany
9Technische Universität Wien, Austria
10CNRS/IN2P3 - IReS, Strasbourg, France
11Univ. Prague, Czech Republic
12Dip. Fisica Generale, Univ. Torino, Italy
13Univ. Politecnica Catalunya, Barcelona, Spain
14INFN, Laboratori Nazionali di Legnaro, Italy
15IAEA, Vienna, Austria
16Univ. Sevilla, Spain
17ITN, Lisbon, Portugal
18CERN, Geneva, Switzerland
19LIP - Coimbra & Dep. Fisica Univ. Coimbra, Portugal
20Univ. Notre Dame, USA
21Inst. Fisica Corpuscular, CSIC-Univ. Valencia, Spain
22Aristotle Univ. Thessaloniki, Greece
23CNR S/IN2P3 - IPN, Orsay, France
24JINR, Frank Lab. Neutron Physics, Dubna, Russia
25CNRS/IN2P3 - IPN, Orsay, France
26LANL, USA
27Tokyo Inst. Technology, Japan
28ORNL, Physics Division, USA
29NCSR, Athens, Greece
30Dip. Fisica, Univ. Bologna, & INFN, Bologna, Italy
31National Technical Univ. Athens, Greece
32Inst. für Fakultät für Physik, Univ. Wien, Austria
33Pôle Univ. L. de Vinci, Paris, France
34CEC-JRC-IRMM, Geel, Belgium
35Dep. Physics and Astronomy, Univ. Basel, Switzerland
36Univ. Pavia, Italy
37ENEA, Bologna, Italy
Abstract: The neutron time of flight (n_TOF) facility at CERN is a neutron spallation source, its white neutron energy spectrum ranges from thermal to several GeV, covering the full energy range of interest for nuclear astrophysics, in particular for measurements of the neutron capture cross-section required in s-process nucleosynthesis. This contribution gives an overview on the astrophysical program made at n_TOF facility, the results and the implications will be considered.
Keywords: Astrophysics, r-process.
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