论文信息 - Low-Background, High-Efficiency Setup for the Study of 22 Ne(p, γ) 23 Na Reaction at Low Energy - 字舞流文

Low-Background, High-Efficiency Setup for the Study of 22 Ne(p, γ) 23 Na Reaction at Low Energy

[1] F. Terrasi,et al. Shell and explosive hydrogen burning , 2016, The European Physical Journal A.

[2] G. Mattei,et al. Strengths of the resonances at 436, 479, 639, 661, and 1279 keV in the Ne 22 ( p , γ ) Na 23 reaction , 2015, 1507.03893.

[3] M. Menzel,et al. A new study of the 22Ne(p, γ)23Na reaction deep underground: Feasibility, setup and first observation of the 186 keV resonance , 2014, 1411.2888.

[4] Alessandra Guglielmetti,et al. LUNA: Nuclear Astrophysics Deep Underground , 2010, 1010.4165.

[5] H. Costantini,et al. LUNA: a laboratory for underground nuclear astrophysics , 2009, 0906.1097.

[6] F. Terrasi,et al. The LUNA II 400 kV accelerator , 2003 .

[7] P. Tupper,et al. The Effects of Thermonuclear Reaction-Rate Variations on Nova Nucleosynthesis: A Sensitivity Study , 2002, astro-ph/0206020.

[8] Jerry B. Marion,et al. NUCLEAR REACTIONS WITH THE NEON ISOTOPES IN STARS , 1957 .