NSR Query Results
Output year order : Descending NSR database version of April 25, 2024. Search: Author = E.Vangioni Found 8 matches. 2018PI08 Phys.Rep. 754, 1 (2018) C.Pitrou, A.Coc, J.-P.Uzan, E.Vangioni Precision big bang nucleosynthesis with improved Helium-4 predictions ATOMIC MASSES 2H, 3,4He, 7Li; calculated primordial mass fractions.
doi: 10.1016/j.physrep.2018.04.005
2017CO10 Int.J.Mod.Phys. E26, 1741002 (2017) Primordial nucleosynthesis NUCLEAR REACTIONS 2H(p, γ), E(cm)<3 MeV; analyzed available data; deduced ratio of experimental S-factors. calculated abundances of 2H, 3,4He, 7Li.
doi: 10.1142/S0218301317410026
2012CO01 Astrophys.J. 744, 158 (2012) A.Coc, S.Goriely, Y.Xu, M.Saimpert, E.Vangioni Standard Big Bang Nucleosynthesis up to CNO with an Improved Extended Nuclear Network NUCLEAR REACTIONS 7Li(d, γ), (t, n), (t, p), (d, n), 8Li(α, n), 11B(d, n), (d, p), (n, γ), 11C(d, p), (n, α), E<10 MeV; calculated astrophysical reaction rates. TALYS code, comparison with NACRE compilations.
doi: 10.1088/0004-637X/744/2/158
2012VA05 J.Phys.:Conf.Ser. 337, 012074 (2012) Cosmic chemical evolution with intermediate mass pop III stars
doi: 10.1088/1742-6596/337/1/012074
2010CO18 J.Phys.:Conf.Ser. 202, 012001 (2010) Big-Bang nucleosynthesis with updated nuclear data
doi: 10.1088/1742-6596/202/1/012001
2010HA28 Phys.Rev. C 82, 065803 (2010) F.Hammache, M.Heil, S.Typel, D.Galaviz, K.Summerer, A.Coc, F.Uhlig, F.Attallah, M.Caamano, D.Cortina, H.Geissel, M.Hellstrom, N.Iwasa, J.Kiener, P.Koczon, B.Kohlmeyer, P.Mohr, E.Schwab, K.Schwarz, F.Schumann, P.Senger, O.Sorlin, V.Tatischeff, J.P.Thibaud, E.Vangioni, A.Wagner, W.Walus High-energy breakup of 6Li as a tool to study the Big Bang nucleosynthesis reaction 2H(α, γ)6Li NUCLEAR REACTIONS 208Pb(6Li, dα), E=150 MeV/nucleon; measured 2H and α particle spectra, angles, positions and energy loss of 2H and α particles, cross section, σ(θ) of excited 6Li; deduced E1, E2, and total S24 factors. Comparison with previous experimental data and GEANT simulations. 2H(α, γ); deduced astrophysical nuclear reaction rates from breakup of 6Li. Predictions for the 6Li/1H production ratio in Big Bang nucleosynthesis. NUCLEAR REACTIONS 208Pb(d, d), E=110, 140 MeV; 208Pb(α, α), E=480, 699 MeV; 208Pb(6Li, 6Li), E=600 MeV; analyzed σ(θ) data; deduced Woods-Saxon potential parameters.
doi: 10.1103/PhysRevC.82.065803
2005AN30 Astrophys.J. 630, L105 (2005) C.Angulo, E.Casarejos, M.Couder, P.Demaret, P.Leleux, F.Vanderbist, A.Coc, J.Kiener, V.Tatischeff, T.Davinson, A.S.Murphy, N.L.Achouri, N.A.Orr, D.Cortina-Gil, P.Figuera, B.R.Fulton, I.Mukha, E.Vangioni The 7Be(d, p)2α Cross Section at Big Bang Energies and the Primordial 7Li Abundance NUCLEAR REACTIONS 2H(7Be, 2α), E=1.71, 5.55 MeV; measured particle spectra, σ. 7Be(d, p), E(cm) ≈ 0.38, 1.2 MeV; deduced astrophysical S-factors. Implications for primordial 7Li abundance discussed.
doi: 10.1086/491732
2005EL09 Phys.Lett. B 619, 30 (2005) J.Ellis, K.A.Olive, E.Vangioni The effects of unstable particles on light-element abundances: Lithium versus deuterium and 3He
doi: 10.1016/j.physletb.2005.05.066
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