Zobrazeno 1 - 3
of 3
pro vyhledávání: '"R. G. Pizzone"'
Autor:
X. Tang, C. Spitaleri, V. Kroha, Michael Wiescher, M. L. Sergi, A. M. Mukhamedzhanov, J. Mrazek, M. La Cognata, G. G. Rapisarda, B. F. Irgaziev, R. G. Pizzone, L. Lamia
Publikováno v:
AIP Conference Proceedings.
In recent years, the Trojan Horse Method (THM) has been used to investigate the low-energy cross sections of proton-induced reactions on 17O nuclei, overcoming extrapolation procedures and enhancement effects due to electron screening. We will report
Autor:
V. Kroha, R. G. Pizzone, A. Coc, S. M. R. Puglia, Aurora Tumino, G. G. Rapisarda, C. Spitaleri, S. Romano, E. Somorjai, N. de Séréville, Z. Hons, Livio Lamia, M. L. Sergi, Gabor Kiss, B. F. Irgaziev, Marisa Gulino, S. Cherubini, A. M. Mukhamedzhanov, Fairouz Hammache, S. V. Burjan, M. La Cognata
Publikováno v:
EXOTIC NUCLEI AND NUCLEAR/PARTICLE ASTROPHYSICS (V). FROM NUCLEI TO STARS: Carpathian Summer School of Physics 2014
EXOTIC NUCLEI AND NUCLEAR/PARTICLE ASTROPHYSICS (V). FROM NUCLEI TO STARS: Carpathian Summer School of Physics 2014, Jul 2014, Sinaia, Romania. pp.392-396, ⟨10.1063/1.4909608⟩
EXOTIC NUCLEI AND NUCLEAR/PARTICLE ASTROPHYSICS (V). FROM NUCLEI TO STARS: Carpathian Summer School of Physics 2014, Jul 2014, Sinaia, Romania. pp.392-396, ⟨10.1063/1.4909608⟩
International audience; The O-17(p,alpha)N-14 reaction is of paramount importance for the nucleosynthesis in a number of stellar sites, including red giants (RG), asymptotic giant branch (AGB) stars, massive stars and classical novae. We report on th
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