التفاصيل البيبلوغرافية
العنوان:
Astrophysics at n_TOF facility
المؤلفون:
G. Tagliente, U. Abbondanno, G. Aerts, H. Alvarez, F. Alvarez-Velarde, S. Andriamonje, J. Andrzejewski, P. Assimakopoulos, L. Audouin, G. Badurek, P. Baumann, F. Becvar, F. Belloni, E. Berthoumieux, S. Bisterzo, F. Calvino, M. Calviani, D. Cano-Ott, R. Capote, C. Carrapico, P. Cennini, V. Chepel, E. Chiaveri, N. Colonna, G. Cortes, A. Couture, J. Cox, M. Dahlfors, S. David, I. Dillman, C. Domingo-Pardo, W. Dridi, I. Duran, C. Eleftheriadis, M. Embid-Segura, L. Ferrant, A. Ferrari, R. Ferreira-Marques, K. Fujii, W. Furman, R. Gallino, I. Goncalves, E. Gonzalez-Romero, F. Gramegna, C. Guerrero, F. Gunsing, B. Haas, R. Haight, M. Heil, A. Herrera-Martinez, M. Igashira, E. Jericha, F. Kappeler, Y. Kadi, D. Karadimos, D. Karamanis, M. Kerveno, P. Koehler, E. Kossionides, M. Krticka, C. Lamboudis, H. Leeb, A. Lindote, I. Lopes, M. Lozano, S. Lukic, J. Marganiec, S. Marrone, T. Martinez, C. Massimi, P. Mastinu, A. Mengoni, P. M.Milazzo, C. Moreau, M. Mosconi, F. Neves, H. Oberhummer, S. O'Brien, J. Pancin, C. Papachristodoulou, C. Papadopoulos, C. Paradela, N. Patronis, A. Pavlik, P. Pavlopoulos, L. Perrot, M. T. Pigni, R. Plag, A. Plompen, A. Plukis, A. Poch, J. Praena, C. Pretel, J. Quesada, T. Rauscher, R. Reifarth, C. Rubbia, G. Rudolf, P. Rullhusen, J. Salgado, C. Santos, L. Sarchiapone, I. Savvidis, C. Stephan, J. L. Tain, L. Tassan-Got, L. Tavora, R. Terlizzi, G. Vannini, P. Vaz, A. Ventura, D. Villamarin, M. C. Vincente, V. Vlachoudis, R. Vlastou, F. Voss, S. Walter, H. Wendler, M. Wiescher, K. Wisshak
المصدر:
Âderna Fìzika ta Energetika, Vol 10, Iss 3, Pp 257-262 (2009)
بيانات النشر:
Institute for Nuclear Research, National Academy of Sciences of Ukraine, 2009.
سنة النشر:
2009
المجموعة:
LCC:Atomic physics. Constitution and properties of matter
مصطلحات موضوعية:
Astrophysics , r-process. , Atomic physics. Constitution and properties of matter , QC170-197
الوصف:
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.
نوع الوثيقة:
article
وصف الملف:
electronic resource
اللغة:
English
تدمد:
1818-331X
Relation:
http://jnpae.kinr.kiev.ua/10.3/Articles_PDF/jnpae-2009-10-0257-Tagliente.pdf ; https://doaj.org/toc/1818-331X ; https://doaj.org/toc/2074-0565
DOI:
10.3/Articles_PDF/jnpae-2009-10-0257-Tagliente.pdf
URL الوصول:
https://doaj.org/article/9ab816bc92644e58ad6a27ff530e762d
رقم الأكسشن:
edsdoj.9ab816bc92644e58ad6a27ff530e762d
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