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NSR database version of April 27, 2024.

Search: Author = C.Ananna

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2023SK01      J.Phys.(London) G50, 045201 (2023)

J.Skowronski, R.M.Gesue, A.Boeltzig, G.F.Ciani, D.Piatti, D.Rapagnani, M.Aliotta, C.Ananna, F.Barile, D.Bemmerer, A.Best, C.Broggini, C.G.Bruno, A.Caciolli, M.Campostrini, F.Cavanna, P.Colombetti, A.Compagnucci, P.Corvisiero, L.Csedreki, T.Davinson, R.Depalo, A.Di Leva, Z.Elekes, F.Ferraro, A.Formicola, Z.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, G.Gyurky, G.Imbriani, M.Junker, M.Lugaro, P.Marigo, E.Masha, R.Menegazzo, V.Paticchio, R.Perrino, P.Prati, V.Rigato, L.Schiavulli, R.S.Sidhu, O.Straniero, T.Szucs, S.Zavatarelli

Advances in radiative capture studies at LUNA with a segmented BGO detector

NUCLEAR REACTIONS ^12,13C, ¹⁴N, ¹⁷O, ²⁵Mg(p, γ), ¹³C(α, n), E ∼ 200 keV; measured reaction products, Eγ, Iγ; deduced yields, resonance parameters, a high-efficiency detection of shorter-lived nuclides. A BGO summing detector at LUNA.

doi: 10.1088/1361-6471/acb961
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2022AN15      Universe 8, 4 (2022)

C.Ananna, F.Barile, A.Boeltzig, C.G.Bruno, F.Cavanna, G.F.Ciani, A.Compagnucci, L.Csedreki, R.Depalo, F.Ferraro, E.Masha, D.Piatti, D.Rapagnani, J.Skowronski

Underground Measurements of Nuclear Reaction Cross-Sections Relevant to Asymptotic Giant Branch stars AGB Stars

NUCLEAR REACTIONS ¹⁷O(p, α)¹⁴N, E(cm)=64.5, 183 keV; ¹⁷O(p, γ)¹⁸F, E(cm)=64.5, 167-370 keV; ¹⁸O(p, α)¹⁵N, E(cm)=55-340 keV; ¹⁸O(p, γ)¹⁹F, E(cm)=85-150 keV; ^12,13C(p, γ)¹³N/¹⁴N, E(cm)=74-370 keV; ²²Ne(p, γ)²³Na, E(cm)=68-300 keV; ²⁰Ne(p, γ)²¹Na, E(cm)=366 keV; ²³Na(p, γ)²⁴Mg, E(cm)=138, 240, 296 keV; ¹³C(α, n)¹⁶O, E(cm)=230-300 keV; ²²Ne(α, γ)²⁶Mg, E(cm)=334 keV; ²²Ne(α, n)²⁵Mg, E(cm)>350 keV; reviewed results from 30 years of experiments by LUNA collaboration at INFN-Gran Sasso (LNGS); deduced resonance strengths, S factors, R-matrix analyses; Relevance to CNO, Ne-Na, and s-process burning networks in the evolution of Asymptotic Giant Branch (AGB) stars, and related nucleosynthesis processes. ¹⁸O(p, α)¹⁵N, E(cm)=55-340 keV; reviewed experimental results; deduced levels, resonances, Γ_p by R-matrix analysis. Comparison with other experimental results.

doi: 10.3390/universe8010004
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