5 Papers
9 Citations
F. Barile is an academic researcher from Istituto Nazionale di Fisica Nucleare. The author has contributed to research in topics: Accelerator mass spectrometry & Neutron. The author has an hindex of 3, co-authored 5 publications.
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Papers
Towards micro-samples radiocarbon dating at INFN-LABEC, Florence
M.E. Fedi,Serena Barone,Serena Barone,F. Barile,L. Liccioli,M. Manetti,Luigi Schiavulli,Luigi Schiavulli +7 more
TL;DR: In this paper, the CHNet_Lilliput experiment aimed at reducing graphite sample masses down to a few tens of μg of carbon, while the typical masses collected at the end of our “standard” preparation process are about 700 μg.
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The new sample preparation line for radiocarbon measurements at the INFN Bari Laboratory
F. Barile,Serena Barone,Serena Barone,M.E. Fedi,L. Liccioli,V. Paticchio,Luigi Schiavulli,Francesco Taccetti +7 more
TL;DR: In this paper, a graphite preparation facility has been installed at the INFN Laboratory of Bari (Italy), where the CO 2 from the combusted sample is purified using a simple vacuum line set-up.
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A C-14 beam monitor using silicon solid state sensor for cultural heritage
F. Barile,Serena Barone,M.E. Fedi,L. Liccioli,V. Paticchio,R. Perrino,Luigi Schiavulli,Francesco Taccetti +7 more
TL;DR: In this article, the authors report the design and preliminary test results of a 14C beam monitor developed for the online monitoring for radiocarbon dating, which uses a silicon solid state detector made of four independent sectors, active area 50 × 50 mm2 and 300 μ m thickness.
5
Characterization of the LUNA neutron detector array for the measurement of the 13C(α, n)16O reaction
László Csedreki,G. F. Ciani,G. F. Ciani,J. Balibrea-Correa,A. Best,Marialuisa Aliotta,F. Barile,Daniel Bemmerer,A. Boeltzig,Carlo Broggini,C. G. Bruno,Antonio Caciolli,Antonio Caciolli,F. Cavanna,T. Chillery,P. Colombetti,P. Colombetti,P. Corvisiero,P. Corvisiero,Thomas Davinson,Rosanna Depalo,Rosanna Depalo,A. Di Leva,Z. Elekes,F. Ferraro,F. Ferraro,E. M. Fiore,E. M. Fiore,A. Formicola,Zs. Fülöp,G. Gervino,G. Gervino,A. Guglielmetti,C. Gustavino,Gy. Gyürky,Gianluca Imbriani,Z. Janas,M. Junker,I. Kochanek,Maria Lugaro,Maria Lugaro,Paola Marigo,Paola Marigo,E. Masha,C. Mazzocchi,Roberto Menegazzo,V. Mossa,F. R. Pantaleo,F. R. Pantaleo,V. Paticchio,R. Perrino,D. Piatti,D. Piatti,Paolo Prati,Paolo Prati,Luigi Schiavulli,Luigi Schiavulli,K. Stöckel,K. Stöckel,Oscar Straniero,Oscar Straniero,Tamás Szücs,M. P. Takács,M. P. Takács,Filippo Terrasi,Sandra Zavatarelli +65 more
TL;DR: In this paper, the LUNA detector array was used for the investigation of the 13C(α, n )16O reaction towards its astrophysical s-process Gamow peak in the low-background environment of the Laboratori Nazionali del Gran Sasso (LNGS).
A new approach to monitor $$^{13}\hbox {C}$$13C-targets degradation in situ for $$^{13}\hbox {C}(\alpha ,\hbox {n})^{16}\hbox {O}$$13C(α,n)16O cross-section measurements at LUNA
G. F. Ciani,G. F. Ciani,László Csedreki,J. Balibrea-Correa,J. Balibrea-Correa,A. Best,A. Best,Marialuisa Aliotta,F. Barile,Daniel Bemmerer,A. Boeltzig,Carlo Broggini,Carlo Bruno,Antonio Caciolli,Antonio Caciolli,F. Cavanna,T. Chillery,P. Colombetti,P. Colombetti,P. Corvisiero,P. Corvisiero,Thomas Davinson,R. Depalo,A. Di Leva,A. Di Leva,L. Di Paolo,Z. Elekes,F. Ferraro,F. Ferraro,E. M. Fiore,E. M. Fiore,A. Formicola,Zs. Fülöp,G. Gervino,G. Gervino,A. Guglielmetti,A. Guglielmetti,C. Gustavino,Gyuri Gyürky,Gianluca Imbriani,Gianluca Imbriani,M. Junker,I. Kochanek,M. Lugaro,Paola Marigo,Paola Marigo,E. Masha,E. Masha,Roberto Menegazzo,V. Mossa,F. R. Pantaleo,F. R. Pantaleo,V. Paticchio,R. Perrino,D. Piatti,D. Piatti,Paolo Prati,Paolo Prati,Luigi Schiavulli,Luigi Schiavulli,K. Stöckel,K. Stöckel,Oscar Straniero,Oscar Straniero,Tamás Szücs,M. P. Takács,M. P. Takács,M. P. Takács,Filippo Terrasi,Davide Trezzi,Davide Trezzi,Sandra Zavatarelli +71 more
TL;DR: In this paper, the shape analysis of primary gamma rays emitted by the radiative capture reaction was used to monitor target degradation in situ during the experiments at low energies at the Laboratory for Underground Nuclear Astrophysics (LUNA) in Italy.