A. Boeltzig
Istituto Nazionale di Fisica Nucleare
3 Papers
A. Boeltzig is an academic researcher from Istituto Nazionale di Fisica Nucleare. The author has contributed to research in topics: Resonance (particle physics) & Orders of magnitude (time). The author has an hindex of 3, co-authored 3 publications. Previous affiliations of A. Boeltzig include Joint Institute for Nuclear Astrophysics.
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Papers
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.
Cross section of the reaction 18O(p,γ)19F at astrophysical energies: The 90 keV resonance and the direct capture component
A. Best,A. Best,F. R. Pantaleo,F. R. Pantaleo,A. Boeltzig,A. Boeltzig,Gianluca Imbriani,Gianluca Imbriani,Marialuisa Aliotta,J. Balibrea-Correa,J. Balibrea-Correa,Daniel Bemmerer,Carlo Broggini,C. G. Bruno,Raffaele Buompane,Raffaele Buompane,Antonio Caciolli,Antonio Caciolli,F. Cavanna,T. Chillery,G. F. Ciani,P. Corvisiero,P. Corvisiero,László Csedreki,Thomas Davinson,Richard deBoer,Rosanna Depalo,Rosanna Depalo,A. Di Leva,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,A. Guglielmetti,C. Gustavino,Gy. Gyürky,M. Junker,I. Kochanek,Maria Lugaro,Paola Marigo,Paola Marigo,Roberto Menegazzo,V. Mossa,V. Mossa,V. Paticchio,R. Perrino,D. Piatti,D. Piatti,Paolo Prati,Paolo Prati,L. Schiavulli,L. Schiavulli,K. Stöckel,K. Stöckel,Oscar Straniero,Oscar Straniero,Frank Strieder,Tamás Szücs,M. P. Takács,M. P. Takács,Davide Trezzi,Davide Trezzi,Michael Wiescher,Sandra Zavatarelli +70 more
TL;DR: In this article, a direct measurement of the O 18 ( p, γ ) 19 F cross section using a high-efficiency 4π BGO summing detector at the Laboratory for Underground Nuclear Astrophysics (LUNA) is presented.