Zobrazeno 1 - 10
of 16
pro vyhledávání: '"R. G. Pizzone"'
Autor:
S. Ma, S. Hayakawa, M. S. Kwag, D. Kahl, N. T. Zhang, Shigeru Kubono, M. La Cognata, J. Su, Alexander Heger, H. Yamaguchi, Yaoyi Li, S. Romano, T. Liu, Y. H. Lam, X. Fang, L. H. Ru, K. Y. Chae, Michele Sferrazza, D. H. Kim, N. N. Duy, A. St. J. Murphy, J. Hu, S. Cherubini, A. Psaltis, Nguyen Kim Uyen, H. M. Shimizu, C. B. Hamill, S. M. Cha, Dh Kim, A. Tumino, L. Yang, E. Q. Liu, J. Liang, R. G. Pizzone, Zac Johnston, A. M. Jacobs, Song-Song Xu
Publikováno v:
Physical Review Letters. 127
We report the first (in)elastic scattering measurement of ^{25}Al+p with the capability to select and measure in a broad energy range the proton resonances in ^{26}Si contributing to the ^{22}Mg(α,p) reaction at type I x-ray burst energies. We measu
Autor:
Qun-Gang Wen, Livio Lamia, A. Tumino, Qiuying Meng, Yuanyong Fu, R. G. Pizzone, Shuhua Zhou, Jing Zhou, Chengbo Li, C. Spitaleri
Publikováno v:
Physical Review C. 95
The $^{2}\mathrm{H}(d,p)^{3}\mathrm{H}$ bare nucleus astrophysical $S(E)$ factor has been measured indirectly at energies from about 500 keV down to several keV by means of the Trojan-horse method applied to the $^{2}\mathrm{H}(^{6}\mathrm{Li},pt)^{4
Autor:
M. L. Sergi, R. Menegazzo, Giuseppe D’Agata, S. Cherubini, D. Dell'Aquila, A. M. Mukhamedzhanov, Ivano Lombardo, N. Carlin, S. Tudisco, Carlo Broggini, V. Rigato, C. Spitaleri, Roberta Spartà, S. Romano, G. L. Guardo, G. G. Rapisarda, A. Tumino, R. G. Pizzone, M. Gimenez del Santo, Rosanna Depalo, L. Lamia, I. Indelicato, A. Cvetinović, M. La Cognata, S. M. R. Puglia, Marcelo Gameiro Munhoz, A. Szanto de Toledo, Antonio Caciolli, F. A. Souza, M. Gulino
Publikováno v:
Physical Review C. 95
For the first time the astrophysical factor of the $^{10}\mathrm{B}(p,{\ensuremath{\alpha}}_{0})^{7}\mathrm{Be}$ reaction has been measured over a wide energy range, from 5 keV to 1.5 MeV, via the Trojan horse method (THM) applied to the quasifree $^
Autor:
C. Spitaleri, Richard deBoer, M. Notani, G. L. Guardo, L. Lamia, V. Kroha, Xiao Fang, Brian Bucher, M. La Cognata, J. Mrazek, G. G. Rapisarda, X. Tang, D. Roberson, R. G. Pizzone, Chi Ma, Paul Davies, S. O'Brien, V. Burjan, A. M. Mukhamedzhanov, Michael Wiescher, Wanpeng Tan, M. L. Sergi, Manoel Couder, M. Gulino
Publikováno v:
AIP Conference Proceedings volume 1852
The experimental study of the 17O(n,α)14C reaction has been performed in the energy range 0-350 keV. This reaction could play an important role in explaining heavy elements (s-process) nucleosynthesis in various astrophysical scenario. To over-come
Autor:
R. G. Pizzone, G. D’Agata, M. La Cognata, I. Indelicato, C. Spitaleri, S. Blagus, S. Cherubini, P. Figuera, L. Grassi, G. L. Guardo, M. Gulino, S. Hayakawa, R. Kshetri, L. Lamia, M. Lattuada, T. Mijatović, M. Milin, Đ. Miljanić D., L. Prepolec, G. G. Rapisarda, S. Romano, M. L. Sergi, N. Skukan, N. Soić, V. Tokić, A. Tumino, M. Uroić
Publikováno v:
Astrophysical Journal
Volume 836
Issue 1
Volume 836
Issue 1
The observational 19F abundance in stellar environments systematically exceeds the predicted one, thus representing one of the unsolved challenges for stellar modeling. It is therefore clear that further investigation is needed in this field. In this
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8bf00f6d7ebb219536210aebf439ecb2
https://www.bib.irb.hr/882998
https://www.bib.irb.hr/882998
Autor:
V. Kroha, L. Lamia, R. Sparta, M. La Cognata, V. Burjan, R. G. Pizzone, M. Gimenez del Santo, J. Mrazek, M. L. Sergi, G. G. Rapisarda, Gabor Kiss, Stefan Typel, S. Piskor, S. Romano, Aurora Tumino, A. M. Mukhamedzhanov, Marialuisa Aliotta, Claudio Spitaleri, Z. Hons
Publikováno v:
Physics Letters B. 700:111-115
The bare nucleus S ( E ) factors for the H 2 ( d , p ) H 3 and H 2 ( d , n ) He 3 reactions have been measured for the first time via the Trojan Horse Method off the proton in 3He from 1.5 MeV down to 2 keV. This range overlaps with the relevant regi
Autor:
L. Lamia, M. La Cognata, Silvio Cherubini, M. Gulino, S. M. R. Puglia, G. L. Guardo, M. L. Sergi, Roberta Spartà, R. G. Pizzone, C. Spitaleri, S. Romano, G. G. Rapisarda, A. Cvetinović
Publikováno v:
EPJ Web of Conferences, Vol 165, p 01018 (2017)
The 10 B(p,α 0 ) 7 Be reaction cross section has been measured in an wide energy range from 2.2 MeV down to 3 keV in a single experiment applying THM. Optimized experimental set-up ensured good energy resolution leading to a good separation of α 0
Study of the 17O(n,α)14C reaction: Extension of the Trojan Horse Method to neutron induced reactions
Autor:
A. M. Mukhamedzhanov, Wanpeng Tan, C. Li, G. L. Guardo, C. Spitaleri, J. Mrazek, Richard deBoer, S. Cherubini, G. G. Rapisarda, X. Tang, M. L. Sergi, V. Kroha, Z. Hons, V. Z. Goldberg, V. Burjan, Larry Lamm, Ian J. Thompson, Paul Davies, M. La Cognata, Chi Ma, Michael Wiescher, D. Roberson, Manoel Couder, M. Gulino, Brian Bucher, M. Notani, Xiao Fang, S. O'Brien, L. Lamia, R. G. Pizzone
Publikováno v:
AIP Conference Proceedings.
The experimental study of the 17O(n,α)14C reaction has been performed in the energy range 0-350 keV. This reaction could play an important role in explaining heavy elements (s-process) nucleosynthesis in various astrophysical scenario. To overcome t
Autor:
Stefan Typel, R. G. Pizzone, C. Rolfs, Claudio Spitaleri, M. G. Pellegriti, Đ. Miljanić, P. Figuera, A. Musumarra, M. Lattuada, H. H. Wolter
Publikováno v:
The Astrophysical Journal. 562:1076-1080
The astrophysically important 7Li(p, α)α reaction has been studied via the Trojan horse method in the energy range E = 10-400 keV. A new theoretical description, based on the distorted-wave Born approximation approach, allows one to extract informa
Autor:
V. Kroha, B. F. Irgaziev, Z. Hons, M. L. Sergi, F. Hammache, Gabor Kiss, E. Somorjai, C. Spitaleri, A. Coc, R. G. Pizzone, Marisa Gulino, Livio Lamia, A. M. Mukhamedzhanov, S. V. Burjan, M. La Cognata, N. de Séréville
Publikováno v:
Nuclear Physics A
Nuclear Physics A, Elsevier, 2010, 834, pp.676C-678C. ⟨10.1016/j.nuclphysa.2010.01.122⟩
Nuclear Physics A, Elsevier, 2010, 834, pp.676C-678C. ⟨10.1016/j.nuclphysa.2010.01.122⟩
The indirect measurement of 17O(p,α)14N cross section was performed by means of the Trojan Horse Method. This approach allowed to investigate the ultra-low energy range ( E c . m . = 0 − 300 keV ) relevant for several astrophysics environments, wh