NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = A.Rinollo Found 10 matches. 2013PI03 Phys.Rev. C 87, 025805 (2013) R.G.Pizzone, C.Spitaleri, C.A.Bertulani, A.M.Mukhamedzhanov, L.Blokhintsev, M.La Cognata, L.Lamia, A.Rinollo, R.Sparta, A.Tumino Updated evidence of the Trojan horse particle invariance for the 2H(d, p)3H reaction NUCLEAR REACTIONS 2H(6Li, pt)α, E=14 MeV; measured proton and triton spectra by energy-loss method, momentum distribution, σ(θ) at INFN-LNS facility in Catania; deduced momentum distribution width, quasifree (QF) contribution, astrophysical S(E) factor for 2H(d, p) reaction via Trojan-horse method (THM) after 6Li breakup. 2H(3He, pt), E(cm)<0.9 MeV; analyzed averaged astrophysical S(E) factor for 2H(d, p) reaction measured via THM after 3He breakup. PWIA analysis. Comparison with previous experimental studies.
doi: 10.1103/PhysRevC.87.025805
2005LA25 Nucl.Phys. A758, 98c (2005) M.La Cognata, A.Musumarra, C.Spitaleri, A.Tumino, C.Bonomo, S.Cherubini, P.Figuera, L.Lamia, M.G.Pellegriti, A.Rinollo, R.G.Pizzone, C.Rolfs, S.Romano, D.Schurmann, F.Strieder, S.Tudisco, S.Typel Study of the 3He(d, p)4He reaction through the Trojan Horse Method NUCLEAR REACTIONS 6Li(3He, pα), E=5, 6 MeV; measured Ep, Eα, angular correlations. 3He(d, p), E=low; deduced astrophysical S-factor.
doi: 10.1016/j.nuclphysa.2005.05.021
2005LA33 Phys.Rev. C 72, 065802 (2005) M.La Cognata, C.Spitaleri, A.Tumino, S.Typel, S.Cherubini, L.Lamia, A.Musumarra, R.G.Pizzone, A.Rinollo, C.Rolfs, S.Romano, D.Schurmann, F.Strieder Bare-nucleus astrophysical factor of the 3He(d, p)4He reaction via the "Trojan horse" method NUCLEAR REACTIONS 6Li(3He, pα), E=5, 6 MeV; measured Ep, Eα, pα-coin, σ(θ), angular correlations; deduced reaction mechanism features. 3He(d, p), E(cm) ≈ 0-600 keV; deduced σ, astrophysical S-factors. Trojan horse method.
doi: 10.1103/PhysRevC.72.065802
2005RI13 Nucl.Phys. A758, 146c (2005) A.Rinollo, S.Romano, C.Spitaleri, C.Bonomo, S.Cherubini, A.Del Zoppo, P.Figuera, M.La Cognata, L.Lamia, A.Musumarra, M.G.Pellegriti, R.G.Pizzone, C.Rolfs, D.Schurmann, F.Strieder, S.Tudisco, A.Tumino Measurement of cross section and astrophysical factor of the d(d, p)t reaction using the Trojan Horse Method NUCLEAR REACTIONS 6Li(d, pt), E=14 MeV; measured particle spectra, angular correlations. 2H(d, p), E ≈ 50-2000 keV; deduced S-factors. Trojan horse method, comparison with previous results.
doi: 10.1016/j.nuclphysa.2005.05.030
2005TU09 Eur.Phys.J. A 25, Supplement 1, 649 (2005) A.Tumino, C.Spitaleri, C.Bonomo, S.Cherubini, P.Figuera, M.Gulino, M.La Cognata, L.Lamia, A.Musumarra, M.G.Pellegriti, R.G.Pizzone, A.Rinollo, S.Romano Quasi-free 6Li(n, α)3H reaction at low energy from 2H break-up NUCLEAR REACTIONS 2H(6Li, tα), E=14 MeV; measured triton and α spectra. 6Li(n, α), E ≈ 0-1 MeV; deduced σ(θ).
doi: 10.1140/epjad/i2005-06-085-1
2004CH22 Eur.Phys.J. A 20, 355 (2004) S.Cherubini, P.Figuera, A.Musumarra, C.Agodi, R.Alba, L.Calabretta, L.Cosentino, A.Del Zoppo, A.Di Pietro, M.La Cognata, L.Lamia, L.Pappalardo, M.G.Pellegriti, R.G.Pizzone, A.Rinollo, C.Rolfs, S.Romano, C.Spitaleri, F.Strieder, S.Tudisco, A.Tumino Cross-section of 8Li(α, n)11B: Inhomogeneous Big Bang nucleosynthesis NUCLEAR REACTIONS 4He(8Li, n), E ≈ 10 MeV; measured neutron yield. 8Li(α, n), E(cm)=1.25 MeV; deduced σ. Astrophysical implications discussed.
doi: 10.1140/epja/i2003-10172-5
2004RO27 Nucl.Phys. A738, 406 (2004) S.Romano, C.Spitaleri, L.Lamia, A.Tumino, R.G.Pizzone, S.Cherubini, A.Del Zoppo, P.Figuera, M.Gulino M.La Cognata, A.Musumarra, M.G.Pellegriti, A.Rinollo, S.Tudisco The astrophysical factor for the 11B(p, α0)8Be reaction extracted via the Trojan Horse Method NUCLEAR REACTIONS 2H(11B, α8Be), E=27 MeV; measured particle spectra, relative energy. 11B(p, α), E(cm) ≈ 0-1 MeV; deduced σ, astrophysical S-factor. Trojan horse method.
doi: 10.1016/j.nuclphysa.2004.04.071
2004SP03 Phys.Rev. C 69, 055806 (2004); Erratum Phys.Rev. C 73, 049905 (2006) C.Spitaleri, L.Lamia, A.Tumino, R.G.Pizzone, S.Cherubini, A.Del Zoppo, P.Figuera, M.La Cognata, A.Musumarra, M.G.Pellegriti, A.Rinollo, C.Rolfs, S.Romano, S.Tudisco The 11B(p, α0)8Be reaction at sub-Coulomb energies via the Trojan-horse method NUCLEAR REACTIONS 2H(11B, α8Be), E=27 MeV; measured particle spectra, (8Be)α-coin, σ(E, θ). 11B(p, α), E(cm) < 1 MeV; deduced excitation function, astrophysical S-factor.
doi: 10.1103/PhysRevC.69.055806
2004TU02 Nucl.Phys. A734, 639 (2004) A.Tumino, C.Spitaleri, L.Pappalardo, S.Cherubini, A.Del Zoppo, M.La Cognata, A.Musumarra, M.G.Pellegriti, R.G.Pizzone, A.Rinollo, S.Romano, S.Typel The Trojan-horse Method applied to the 6Li(p, α)3He reaction down to astrophysical energies NUCLEAR REACTIONS 2H(6Li, 3Heα), E=14, 25 MeV; measured particle spectra, coincidence yields, angular correlations. 6Li(p, α), E=low; deduced astrophysical S-factors.
doi: 10.1016/j.nuclphysa.2004.01.117
2004TU06 Prog.Theor.Phys.(Kyoto), Suppl. 154, 341 (2004) A.Tumino, C.Spitaleri, L.Pappalardo, S.Cherubini, A.Del Zoppo, M.La Cognata, A.Musumarra, M.G.Pellegriti, R.G.Pizzone, A.Rinollo, C.Rolfs, S.Romano, S.Typel Indirect Study of the Astrophysically Relevant 6Li(p, α)3He Reaction by Means of the Trojan Horse Method NUCLEAR REACTIONS 2H(6Li, 3Heα), E=14, 25 MeV; measured particle spectra, (α)(3He)-coin, angular correlations; deduced R-matrix parameters. 6Li(p, α), E=low; deduced astrophysical S-factor. Trojan horse method, kinematically complete measurement.
doi: 10.1143/PTPS.154.341
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