NSR Query Results
Output year order : Descending NSR database version of April 11, 2024. Search: Author = S.Romano Found 133 matches. Showing 1 to 100. [Next]2023CA14 Phys.Rev. C 108, 045802 (2023) D.P.Carrasco-Rojas, M.Williams, P.Adsley, L.Lamia, B.Bastin, T.Faestermann, C.Fougeres, F.Hammache, D.S.Harrouz, R.Hertenberger, M.La Cognata, A.Meyer, F.de Oliveira Santos, S.Palmerini, R.G.Pizzone, S.Romano, N.de Sereville, A.Tumino, H.-F.Wirth Searching for resonance states in 22Ne(p, γ)23Na
doi: 10.1103/PhysRevC.108.045802
2023GU07 Eur.Phys.J. A 59, 65 (2023) G.L.Guardo, T.Petruse, D.Lattuada, M.La Cognata, D.L.Balabanski, E.Aciksoz, L.Acosta, L.Capponi, D.Carbone, S.Cherubini, D.Choudhury, G.D'Agata, A.Di Pietro, P.Figuera, M.Gulino, A.I.Kilik, M.La Commara, L.Lamia, C.Matei, S.Palmerini, R.G.Pizzone, G.G.Rapisarda, S.Romano, M.L.Sergi, P.-A.Soderstrom, R.Sparta, A.Tumino, S.Vinals Direct measurement of the 19F(p, α0)16O reaction at Ecm= 0.4-0.9 using the LHASA detector array NUCLEAR REACTIONS 1H(19F, α), E(cm)=0.4-0.9 MeV; measured reaction products, Eα, Iα; deduced σ(θ), S-factor. Comparison with NACRE compilation, available data. INFN-Laboratori Nazionali del Sud, Catania (Italy).
doi: 10.1140/epja/s10050-023-00957-1
2023TU05 Commun. Phys. 6, 106 (2023) A.Tumino, G.G.Rapisarda, M.La Cognata, A.Oliva, A.Kievsky, C.A.Bertulani, G.D'Agata, M.Gattobigio, G.L.Guardo, L.Lamia, D.Lattuada, R.G.Pizzone, S.Romano, M.L.Sergi, R.Sparta, M.Viviani Coulomb-free 1So p - p scattering length from the quasi-freep p + d → p + p + n reaction and its relation to universality NUCLEAR REACTIONS 2H(p, 2p), E(cm)<1 MeV; analyzed available data; deduced p-p scattering σ, σ(θ), scattering length and effective range from a Bayesian approach analysis.
doi: 10.1038/s42005-023-01221-0
2022HA03 Phys.Rev. C 105, 015805 (2022) D.S.Harrouz, N.de Sereville, P.Adsley, F.Hammache, R.Longland, B.Bastin, T.Faestermann, R.Hertenberger, M.La Cognata, L.Lamia, A.Meyer, S.Palmerini, R.G.Pizzone, S.Romano, A.Tumino, H.-F.Wirth Experimental study of the 30Si(3He, d)31P reaction and thermonuclear reaction rate of 30Si(p, γ)31P NUCLEAR REACTIONS 30Si(3He, d)31P, E=25 MeV beam from the Tandem Van de Graaff accelerator at MLL-Garching; measured E(d), I(d), σ(θ), deuterons momentum analyzed using a Q3D magnetic spectrometer, and detected in the focal plane of proportional counters. 31P; deduced levels, J, π, L-transfers, spectroscopic factors, single-particle widths, DWBA analysis of angular distribution data. 30Si(p, γ)31P, T9=0.010-10.0; deduced proton resonance energies, Γp, resonance strengths, astrophysical reaction rates. Comparison with previous experimental results and evaluated data for 31P structure, and with available data for proton resonances.
doi: 10.1103/PhysRevC.105.015805
2022LA14 Astrophys.J. 941, 96 (2022) M.La Cognata, S.Palmerini, P.Adsley, F.Hammache, A.Di Pietro, P.Figuera, F.Dell'Agli, R.Alba, S.Cherubini, G.L.Guardo, M.Gulino, L.Lamia, D.Lattuada, C.Maiolino, A.Oliva, R.G.Pizzone, P.M.Prajapati, G.G.Rapisarda, S.Romano, D.Santonocito, R.Sparta, M.L.Sergi, A.Tumino, P.Ventura A New Reaction Rate of the 27Al(p/α)24Mg Reaction Based on Indirect Measurements at Astrophysical Energies and Implications for 27Al Yields of Intermediate-mass Stars NUCLEAR REACTIONS 2H(27Al, α24Mg), E=80 MeV; measured reaction products. 28Si, 24Mg; deduced σ(θ), σ(θ, E), resonance strengths. Comparison with Monte Carlo code RatesMC. Indirect Trojan Horse Method (THM), the INFN-LNS Tandem (Catania, Italy).
doi: 10.3847/1538-4357/ac9c5e
2022PI06 Eur.Phys.J. A 58, 234 (2022) R.G.Pizzone, S.Degl'Innocenti, M.La Cognata, L.Lamia, G.G.Rapisarda, S.Romano, M.L.Sergi, A.Tumino Indirect investigations on fusion reactions NUCLEAR REACTIONS 10B(p, α), E(cm)<0.10 MeV; 17O(p, α), (p, γ), E not given; 2H(17O, α14N)1NN, E(cm)<0.25 MeV; analyzed available data; deduced S-factors, astrophysical reaction rates. The Trojan Horse Method (THM), Asymptotic Normalisation Coefficient (ANC).
doi: 10.1140/epja/s10050-022-00889-2
2021DA04 Phys.Rev. C 103, 015806 (2021) G.D'Agata, A.I.Kilic, V.Burjan, J.Mrazek, V.Glagolev, V.Kroha, G.L.Guardo, M.La Cognata, L.Lamia, S.Palmerini, R.G.Pizzone, G.G.Rapisarda, S.Romano, M.L.Sergi, R.Sparta, C.Spitaleri, I.Sivacek, A.Tumino 26Si(p, γ)27P direct proton capture by means of the asymptotic normalization coefficients method for mirror nuclei NUCLEAR REACTIONS 26Mg(d, p)27Mg, E=19.2 MeV; measured reaction products, σ(θ) for ground and first excited states using ΔE-E telescopes at INFN-LNS-Catania accelerator facility; deduced Optical Model Potential parameters for entrance and exit channels using DWBA calculations. 26Mg(n, γ)27Mg; 26Si(p, γ)27P; deduced spectroscopic factors and asymptotic normalization coefficients (ANCs) for capture in the ground and first excited states, width Γp for first resonance in 27P using the ANC methodology for mirror nuclei. 26Si(p, γ)27P, T9=0.1-2.0; calculated astrophysical reaction rates.
doi: 10.1103/PhysRevC.103.015806
2021HA53 Astrophys.J. 915, L13 (2021) S.Hayakawa, M.La Cognata, L.Lamia, H.Yamaguchi, D.Kahl, K.Abe, H.Shimizu, L.Yang, O.Beliuskina, S.M.Cha, K.Y.Chae, S.Cherubini, P.Figuera, Z.Ge, M.Gulino, J.Hu, A.Inoue, N.Iwasa, A.Kim, D.Kim, G.Kiss, S.Kubono, M.La Commara, M.Lattuada, E.J.Lee, J.Y.Moon, S.Palmerini, C.Parascandolo, S.Y.Park, V.H.Phong, D.Pierroutsakou, R.G.Pizzone, G.G.Rapisarda, S.Romano, C.Spitaleri, X.D.Tang, O.Trippella, A.Tumino, N.T.Zhang Constraining the Primordial Lithium Abundance: New Cross Section Measurement of the 7Be + n Reactions Updates the Total 7Be Destruction Rate NUCLEAR REACTIONS 2H(7Be, p7Li)1H, E=3.16 MeV/nucleon; measured reaction products. 8Be; deduced σ, low-lying resonance parameters, astrophysical reaction rates for 7Be(n, p) and 7Be(n, α) reactions. Comparison with available data. the Trojan Horse Method (THM), Center-for-Nuclear-Study RI Beam separator (CRIB), the University of Tokyo, located atthe RI Beam Factory, RIKEN.
doi: 10.3847/2041-8213/ac061f
2021HU23 Phys.Rev.Lett. 127, 172701 (2021) J.Hu, H.Yamaguchi, Y.H.Lam, A.Heger, D.Kahl, A.M.Jacobs, Z.Johnston, S.W.Xu, N.T.Zhang, S.B.Ma, L.H.Ru, E.Q.Liu, T.Liu, S.Hayakawa, L.Yang, H.Shimizu, C.B.Hamill, A.St J.Murphy, J.Su, X.Fang, K.Y.Chae, M.S.Kwag, S.M.Cha, N.N.Duy, N.K.Uyen, D.H.Kim, R.G.Pizzone, M.La Cognata, S.Cherubini, S.Romano, A.Tumino, J.Liang, A.Psaltis, M.Sferrazza, D.Kim, Y.Y.Li, S.Kubono Advancement of Photospheric Radius Expansion and Clocked Type-I X-Ray Burst Models with the New 22Mg(α, p)25Al Reaction Rate Determined at the Gamow Energy NUCLEAR REACTIONS 1H(25Al, p), (25Al, p'), (25Al, X), E=142 MeV; measured reaction products, Ep, Ip, Eγ, Iγ. 26Si; deduced σ(θ), level energies, J, π, resonance parameters, astrophysical reaction rates. Comparison with available data.
doi: 10.1103/physrevlett.127.172701
2021KI06 Phys.Rev. C 104, 015807 (2021) G.G.Kiss, M.La Cognata, R.Yarmukhamedov, K.I.Tursunmakhatov, I.Wiedenhover, L.T.Baby, S.Cherubini, A.Cvetinovic, G.D'Agata, P.Figuera, G.L.Guardo, M.Gulino, S.Hayakawa, I.Indelicato, L.Lamia, M.Lattuada, F.Mudo, S.Palmerini, R.G.Pizzone, G.G.Rapisarda, S.Romano, M.L.Sergi, R.Sparta, C.Spitaleri, O.Trippella, A.Tumino, M.Anastasiou, S.A.Kuvin, N.Rijal, B.Schmidt, S.B.Igamov, S.B.Sakuta, Zs.Fulop, Gy.Gyurky, T.Szucs, Z.Halasz, E.Somorjai, Z.Hons, J.Mrazek, R.E.Tribble, A.M.Mukhamedzhanov Indirect determination of the astrophysical S factor for the 6Li (p, γ)7Be reaction using the asymptotic normalization coefficient method NUCLEAR REACTIONS 6Li(3He, d)7Be, E=3, 5 MeV; measured E(d), I(d), σ(θ) using ΔE-E silicon detector telescopes at the University of Catania and the FN tandem accelerator of Florida State University. 7Be; deduced levels, asymptotic normalization coefficient (ANCs) for the g.s. and the first excited state at 429 keV of 7Be from DWBA analysis of angular distributions. 6Li(p, γ)7Be, E=0.05-0.35 MeV; deduced asymptotic normalization coefficient (ANCs) using results from the 6Li(3He, d) reaction. 6Li(p, γ)7Be, E<1.0 MeV; analyzed available experimental data; deduced astrophysical S factor from direct experimental data, as well as present indirect method from ANCs determined in 6Li(3He, d) experiment. Relevance to big-bang and stellar nucleosynthesis.
doi: 10.1103/PhysRevC.104.015807
2021SP03 Eur.Phys.J. A 57, 170 (2021) R.Sparta, L.Lamia, M.La Cognata, C.Spitaleri, G.G.Rapisarda, G.L.Guardo, S.Cherubini, G.D'Agata, A.Di Pietro, P.Figuera, M.Gulino, D.Lattuada, M.Lattuada, S.Palmerini, R.G.Pizzone, S.Romano, M.L.Sergi, A.Tumino, S.Typel 10B(n, α0)7Li and 10B(n, α1)7Li reactions measured via Trojan Horse Method NUCLEAR REACTIONS 2H(10B, α7Be), E=28 MeV; measured reaction products, Eα, Iα; deduced momentum distribution for the spectator particle, σ(θ), σ(E), 10B(n, α) σ using the Trojan Horse Method.
doi: 10.1140/epja/s10050-021-00481-0
2020KI11 Phys.Lett. B 807, 135606 (2020) G.G.Kiss, M.La Cognata, C.Spitaleri, R.Yarmukhamedov, I.Wiedenhover, L.T.Baby, S.Cherubini, A.Cvetinovic, G.D'Agata, P.Figuera, G.L.Guardo, M.Gulino, S.Hayakawa, I.Indelicato, L.Lamia, M.Lattuada, F.Mudo, S.Palmerini, R.G.Pizzone, G.G.Rapisarda, S.Romano, M.L.Sergi, R.Sparta, O.Trippella, A.Tumino, M.Anastasiou, S.A.Kuvin, N.Rijal, B.Schmidt, S.B.Igamov, S.B.Sakuta, K.I.Tursunmakhatov, Zs.Fulop, G.Gyurky, T.Szucs, Z.Halasz, E.Somorjai, Z.Hons, J.Mrazek, R.E.Tribble, A.M.Mukhamedzhanov Astrophysical S-factor for the 3He(α, γ)7Be reaction via the asymptotic normalization coefficient (ANC) method NUCLEAR REACTIONS 6Li(3He, d)7Be, E=3, 5 MeV; measured reaction products; deduced σ(θ), S-factor, external capture contribution using the Asymptotic Normalization Coefficient (ANC) technique.
doi: 10.1016/j.physletb.2020.135606
2020PI11 Eur.Phys.J. A 56, 199 (2020) R.G.Pizzone, C.Spampinato, R.Sparta, M.Couder, W.Tan, V.Burjan, G.D'Agata, G.L.Guardo, M.La Cognata, L.Lamia, J.Mrazek, S.Palmerini, S.Typel, A.Tumino, M.Wiescher, S.Anguilar, D.Bardayan, D.Blankstein, L.Boccioli, L.Callahan, S.M.Cha, K.Y.Chae, A.M.Clark, B.Frentz, M.R.Hall, A.Gula, S.Henderson, R.Kelmar, M.S.Kwag, I.Indelicato, M.La Commara, D.Lattuada, Q.Liu, J.Long, M.Mazzocco, A.Majumdar, S.McGuinness, A.Nelson, A.A.Oliva, P.O'Malley, P.M.Prajapati, G.G.Rapisarda, S.Romano, M.L.Sergi, C.Seymour, M.Skulski, C.Spitaleri, J.Wilkinson Indirect measurement of the 3He(n, p)3H reaction cross section at Big Bang energies NUCLEAR REACTIONS 2H(3He, pt), E=9 MeV; measured reaction products, Ep, Ip; deduced σ for 3He(n, p) reaction using the Trojan Horse Method (THM).
doi: 10.1140/epja/s10050-020-00212-x
2020SP02 Eur.Phys.J. A 56, 18 (2020) C.Spitaleri, M.Lattuada, A.Cvetinovic, N.Soic, M.Milin, P.Colovic, G.D'Agata, D.Dell'Aquila, G.L.Guardo, M.Gulino, O.Trippella, M.La Cognata, L.Lamia, D.Lattuada, C.Li, S.Messina, D.Nurkic, S.S.Perrotta, R.G.Pizzone, R.Popoconski, S.Romano, N.Skukan, R.Sparta, S.Szilner, M.Uroic, N.Vukman Study of the quasi-free 3He + 9Be → 3α reaction for the Trojan Horse Method
doi: 10.1140/epja/s10050-020-00026-x
2019BU17 Eur.Phys.J. A 55, 114 (2019) V.Burjan, Z.Hons, V.Kroha, J.Mrazek, S.Piskor, A.M.Mukhamedzhanov, L.Trache, R.E.Tribble, M.La Cognata, L.Lamia, R.G.Pizzone, S.Romano, C.Spitaleri, A.Tumino The determination of the astrophysical S-factor of the direct 18O(p, γ)19F capture by the ANC method
doi: 10.1140/epja/i2019-12801-8
2019GU32 Eur.Phys.J. A 55, 211 (2019) G.L.Guardo, C.Spitaleri, L.Lamia, R.Spartá, N.Carlin, S.Cherubini, G.Gimenez Del Santo, I.Indelicato, M.La Cognata, D.Lattuada, S.Messina, M.Munhoz, S.S.Perrotta, R.G.Pizzone, G.G.Rapisarda, S.Romano, M.L.Sergi, F.A.Souza, A.Szanto de Toledo, S.Tudisco, A.Tumino The 10B(n, α)7Li cross sections at ultra-low energy through the Trojan Horse Method applied to the 2H(10B, α7Li)1H
doi: 10.1140/epja/i2019-12914-0
2019LA08 Phys.Rev. C 99, 034301 (2019) M.La Cognata, M.Fisichella, A.Di Pietro, P.Figuera, V.Z.Goldberg, S.Cherubini, J.P.Fernandez-Garcia, M.Gulino, L.Lamia, D.Lattuada, M.Lattuada, R.G.Pizzone, G.G.Rapisarda, S.Romano, R.Sparta, C.Spitaleri, D.Torresi, A.Tumino, M.Zadro Observation of 15N α resonant structures in 19F using the thick target in inverse kinematics scattering method NUCLEAR REACTIONS 4He(15N, α), E=40.23 MeV; measured Eα, Iα, differential σ(θ) using ΔE-E silicon telescopes for α detection and surface barrier detectors for 15N-like recoils at the LNL-Catania Tandem accelerator facility. 19F; deduced levels, resonances, J, π, α-widths, proton widths and potential α-cluster states using R-matrix analysis using AZURE2 code. Comparison with previous experimental data, and with literature data for mirror nucleus 19Ne. Relevance to models of stars in different evolutionary stages, such as the asymptotic giant branch (AGB) stars asymptotic giant branch (AGB).
doi: 10.1103/PhysRevC.99.034301
2019LA13 Astrophys.J. 879, 23 (2019) L.Lamia, M.Mazzocco, R.G.Pizzone, S.Hayakawa, M.La Cognata, C.Spitaleri, C.A.Bertulani, A.Boiano, C.Boiano, C.Broggini, A.Caciolli, S.Cherubini, G.D'Agata, H.da Silva, R.Depalo, F.Galtarossa, G.L.Guardo, M.Gulino, I.Indelicato, M.La Commara, G.La Rana, R.Menegazzo, J.Mrazek, A.Pakou, C.Parascandolo, D.Piatti, D.Pierroutsakou, S.M.R.Puglia, S.Romano, G.G.Rapisarda, A.M.Sanchez-Benitez, M.L.Sergi, O.Sgouros, F.Soramel, V.Soukeras, R.Sparta, E.Strano, D.Torresi, A.Tumino, H.Yamaguchi, G.L.Zhang Cross-section Measurement of the Cosmologically Relevant 7Be(n, α)4He Reaction over a Broad Energy Range in a Single Experiment NUCLEAR REACTIONS 2H(7Be, 2α), E<2 MeV; measured reaction products, Ep, Ip. 8Be; deduced σ, astrophysical reaction rates. Trojan Horse Method.
doi: 10.3847/1538-4357/ab2234
2018CV01 Phys.Rev. C 97, 065801 (2018) A.Cvetinovic, C.Spitaleri, R.Sparta, G.G.Rapisarda, S.M.R.Puglia, M.La Cognata, S.Cherubini, G.L.Guardo, M.Gulino, L.Lamia, R.G.Pizzone, S.Romano, M.L.Sergi, A.Tumino Trojan horse measurement of the 10B(p, α0) cross section in the energy range from 3 keV to 2.2 MeV NUCLEAR REACTIONS 2H(10B, α7Be), E=3-2200 keV; measured Eα, 7Be particles, 7Beα-coin, angular distributions, and triple differential σ(E, θα, θBe) at INFN-Catania accelerator facility; deduced Trojan horse method (THM) bare-nucleus S(E) factors, and electron screening potential. 11C; deduced levels, resonances. Comparison with previous experimental results.
doi: 10.1103/PhysRevC.97.065801
2018DA14 Astrophys.J. 860, 61 (2018) G.D'Agata, R.G.Pizzone, M.La Cognata, I.Indelicato, C.Spitaleri, S.Palmerini, O.Trippella, D.Vescovi, S.Blagus, S.Cherubini, P.Figuera, L.Grassi, G.L.Guardo, M.Gulino, S.Hayakawa, R.Kshetri, L.Lamia, M.Lattuada, T.Mijatovic, M.Milin, D.Miljanic, L.Prepolec, G.G.Rapisarda, S.Romano, M.L.Sergi, N.Skukan, N.Soic, V.Tokic, A.Tumino, M.Uroic The 19F(α, p)22Ne Reaction at Energies of Astrophysical Relevance by Means of the Trojan Horse Method and Its Implications in AGB Stars NUCLEAR REACTIONS 19F(6Li, p22Ne), E=6 MeV; measured reaction products. 23Na; deduced yields, σ(θ), σ, reaction rates. Comparison with available data.
doi: 10.3847/1538-4357/aac207
2018LA14 Phys.Rev. C 98, 054601 (2018) H.Y.Lan, Y.Xu, W.Luo, D.L.Balabanski, S.Goriely, M.La Cognata, C.Matei, A.Anzalone, S.Chesnevskaya, G.L.Guardo, D.Lattuada, R.G.Pizzone, S.Romano, C.Spitaleri, A.Taffara, A.Tumino, Z.C.Zhu Determination of the photodisintegration reaction rates involving charged particles: Systematic calculations and proposed measurements based on the facility for Extreme Light Infrastructure--Nuclear Physics NUCLEAR REACTIONS 74Se, 84Sr, 92Mo, 96Ru, 102Pd, 106Cd, 112Sn, 120Te(γ, p), E(cm)=8-20 MeV; 74Se, 84Sr, 92Mo, 96Ru, 102Pd, 106Cd, 112Sn, 120Te, 132Ba, 144Sm, 148Gd, 184Os(γ, α), E(cm)=6-20 MeV; calculated σ(E), proton and α-particle spectra and yields, Gamow windows at T9=2.5 and minimum required energies of the incident γ beam satisfying the measurable criteria of the minimum detectable limit and the particle identification. Z=10-100, N=10-160; calculated ratios of the (γ, p) and (γ, α) astrophysical reaction rates at T9=2.5 for 3000 targets of stable and proton-rich nuclei. Optical potential model calculations using Woods-Saxon and microscopic folding JLMB optical model potentials. Relevance to p-process nucleosynthesis, and the measurements of six (γ, p) and eight (γ, α) reactions based on the γ-beam facility and the Extreme Light Infrastructure Silicon Strip Array (ELISSA) for the detection of charged particles at ELI-NP, Bucharest facility.
doi: 10.1103/PhysRevC.98.054601
2018RA17 Acta Phys.Pol. B49, 669 (2018) G.G.Rapisarda, C.Spitaleri, A.Cvetinovic, R.Sparta, S.Cherubini, G.L.Guardo, M.Gulino, M.La Cognata, L.Lamia, S.M.R.Puglia, S.Romano, M.L.Sergi Recent Results on the 10B(p, α)7Be Reaction Studied via THM at Low Energies NUCLEAR REACTIONS 2H(10B, α7Be)1n, (p, α)1n, E=28 MeV; measured reaction products using the Trojan Horse Method (THM); deduced Q-value spectrum for the 2H(10B, α7Be)1n reaction; σ(α0) from 3 keV to 2.2 MeV; deduced that better energy resolution would lead to improvement in astrophysical S(E) factor determination, results for the σ(θ1) indication feasibility of measurements of several 11C excited levels. Results preliminary, final results to be available soon.
doi: 10.5506/aphyspolb.49.669
2018RA25 Eur.Phys.J. A 54, 189 (2018) G.G.Rapisarda, C.Spitaleri, A.Cvetinovic, R.Sparta, S.Cherubini, G.L.Guardo, M.Gulino, M.La Cognata, L.Lamia, R.G.Pizzone, S.Romano, M.L.Sergi, A.Tumino Study of the 10B(p, α1)7Be reaction by means of the Trojan Horse Method NUCLEAR REACTIONS 10B(p, α1)7Be, E not given; measured using 2H(10B, α7Be) as the Trojan Horse partner; deduced σ(θ) vs E* of 11C (unnormalized), Γ widths for six lowest lying resonances. 2H(10B, α7Be); measured reaction products; measured 7Be-n and α-n Q-value.
doi: 10.1140/epja/i2018-12622-3
2017DE25 Phys.Rev.Lett. 119, 132501 (2017) D.Dell'Aquila, I.Lombardo, G.Verde, M.Vigilante, L.Acosta, C.Agodi, F.Cappuzzello, D.Carbone, M.Cavallaro, S.Cherubini, A.Cvetinovic, G.D'Agata, L.Francalanza, G.L.Guardo, M.Gulino, I.Indelicato, M.La Cognata, L.Lamia, A.Ordine, R.G.Pizzone, S.M.R.Puglia, G.G.Rapisarda, S.Romano, G.Santagati, R.Sparta, G.Spadaccini, C.Spitaleri, A.Tumino High-Precision Probe of the Fully Sequential Decay Width of the Hoyle State in 12C NUCLEAR REACTIONS 14N(d, α)12C, E=10.5 MeV; measured reaction products, Eα, Iα; deduced decay path of the Hoyle state, decay width limit. Comparison with available data.
doi: 10.1103/PhysRevLett.119.132501
2017IN01 Astrophys.J. 845, 19 (2017) I.Indelicato, M.La Cognata, C.Spitaleri, V.Burjan, S.Cherubini, M.Gulino, S.Hayakawa, Z.Hons, V.Kroha, L.Lamia, M.Mazzocco, J.Mrazek, R.G.Pizzone, S.Romano, E.Strano, D.Torresi, and A.Tumino New Improved Indirect Measurement of the 19F(p, α)16O Reaction at Energies of Astrophysical Relevance NUCLEAR REACTIONS C, 2H(19F, α16O), E=55 MeV; measured reaction products, Eα, Iα; deduced σ(θ, E), S-factors, reaction rates. Comparison with R-matrix analysis, available data.
doi: 10.3847/1538-4357/aa7de7
2017LA19 Astrophys.J. 850, 175 (2017) L.Lamia, C.Spitaleri, C.A.Bertulani, S.Q.Hou, M.La Cognata, R.G.Pizzone, S.Romano, M.L.Sergi, A.Tumino On the Determination of the 7Be(n, α)4He Reaction Cross Section at BBN Energies NUCLEAR REACTIONS 7Be(n, α), E(cm)<8 MeV; analyzed available data; deduced σ using Trojan Horse method.
doi: 10.3847/1538-4357/aa965c
2017PI03 Astrophys.J. 836, 57 (2017) R.G.Pizzone, G.D'Agata, M.La Cognata, I.Indelicato, C.Spitaleri, S.Blagus, S.Cherubini, P.Figuera, L.Grassi, G.L.Guardo, M.Gulino, S.Hayakawa, R.Kshetri, L.Lamia, M.Lattuada, T.Mijatovic, M.Milin, D.Miljanic, L.Prepolec, G.G.Rapisarda, S.Romano, M.L.Sergi, N.Skukan, N.Soic, V.Tokic, A.Tumino, M.Uroic First Measurement of the 19F(α, p)22Ne Reaction at Energies of Astrophysical Relevance NUCLEAR REACTIONS 19F(6Li, p22Ne), E=6 MeV; measured reaction products, Ep, Ep; deduced σ(θ), S factor, reaction rate. Comparison with available data.
doi: 10.3847/1538-4357/836/1/57
2017SP04 Phys.Rev. C 95, 035801 (2017) C.Spitaleri, S.M.R.Puglia, M.La Cognata, L.Lamia, S.Cherubini, A.Cvetinovic, G.D'Agata, M.Gulino, G.L.Guardo, I.Indelicato, R.G.Pizzone, G.G.Rapisarda, S.Romano, M.L.Sergi, R.Sparta, S.Tudisco, A.Tumino, M.Gimenez Del Santo, N.Carlin, M.G.Munhoz, F.A.Souza, A.Szanto de Toledo, A.Mukhamedzhanov, C.Broggini, A.Caciolli, R.Depalo, R.Menegazzo, V.Rigato, I.Lombardo, D.Dell'Aquila Measurement of the 10B(p, α0)7Be cross section from 5 keV to 1.5 MeV in a single experiment using the Trojan horse method NUCLEAR REACTIONS 2H(10B, α7Be), E=27 MeV; measured α and 7Be spectra using ΔE-E method at Pelletron-Linac laboratory of DFN-Sao Paulo; deduced Q-value spectrum, energy scatter plots, momentum distribution, astrophysical S(E) factors, Trojan horse method (THM) astrophysical factor, R-matrix fit of THM data 11C; deduced levels, resonances, center-of-mass energies, J, π, Γp, Γα0, Γα1.
doi: 10.1103/PhysRevC.95.035801
2016CA21 Eur.Phys.J. A 52, 136 (2016) A.Caciolli, R.Depalo, C.Broggini, M.La Cognata, L.Lamia, R.Menegazzo, L.Mou, S.M.R.Puglia, V.Rigato, S.Romano, C.Rossi Alvarez, M.L.Sergi, C.Spitaleri, A.Tumino A new study of 10B(p, α)7Be reaction at low energies NUCLEAR REACTIONS 10B(p, α), E=250-1182 keV; measured 7Li, 7Be activation Eγ, Iγ using HPGe; deduced 7Be yield. RADIOACTIVITY 7Be(β+), (EC). 7Li measured activation Eγ, Iγ using HPGe. 7Be deduced S-factor; calculated S-factor using R-matrix; deduced 11C resonances, parameters, justification of THM (Troian Horse Method) published. More detailed calculations in progress.
doi: 10.1140/epja/i2016-16136-8
2015CH41 Phys.Rev. C 92, 015805 (2015) S.Cherubini, M.Gulino, C.Spitaleri, G.G.Rapisarda, M.La Cognata, L.Lamia, R.G.Pizzone, S.Romano, S.Kubono, H.Yamaguchi, S.Hayakawa, Y.Wakabayashi, N.Iwasa, S.Kato, T.Komatsubara, T.Teranishi, A.Coc, N.de Sereville, F.Hammache, G.Kiss, S.Bishop, D.N.Binh First application of the Trojan horse method with a radioactive ion beam: Study of the 18F(p, α)15O reaction at astrophysical energies NUCLEAR REACTIONS 2H(18F, α15O), E=47.9 MeV, [18F secondary beam from 18O(p, n) primary reaction at CRIB-CNS-RIKEN facility]; measured Q-value spectra, σ for p-18F c.m. energy; deduced momentum distribution for the p-n intercluster motion in deuteron. 19Ne; deduced proton resonances, levels, J, π, and compared to previous experimental data and evaluations. 18F(p, α)15O, E<900 keV; deduced σ(E), astrophysical S(E) factor by Trojan horse method (THM) by considering interference effects.
doi: 10.1103/PhysRevC.92.015805
2014SP03 Phys.Rev. C 90, 035801 (2014) C.Spitaleri, L.Lamia, S.M.R.Puglia, S.Romano, M.La Cognata, V.Crucilla, R.G.Pizzone, G.G.Rapisarda, M.L.Sergi, M.Gimenez Del Santo, N.Carlin, M.G.Munhoz, F.A.Souza, A.Szanto de Toledo, A.Tumino, B.Irgaziev, A.Mukhamedzhanov, G.Tabacaru, V.Burjan, V.Kroha, Z.Hons, J.Mrazek, S.-H.Zhou, C.Li, Q.Wen, Y.Wakabayashi, H.Yamaguchi, E.Somorjai Measurement of the 10 keV resonance in the 10B(p, α0)7Be reaction via the Trojan Horse method NUCLEAR REACTIONS 2H(10B, α7Be), E=24.5 MeV; measured particle spectra by ΔE-E method using ionization chambers and position-sensitive detectors at LNS-Catania accelerator facility; analyzed data by Trojan Horse method (THM); deduced Eα-Be and Eα-n two-dimensional plots, experimental momentum distribution and its comparison with DWBA and PWIA calculations, THM bare nucleus astrophysical S(E) factors using R-matrix formalism for 5-100 keV resonances in 11C, dominated by 10-keV resonance corresponding to 8699-keV, 5/2+ level in 11C. 11C; deduced widths of three resonances.
doi: 10.1103/PhysRevC.90.035801
2014TU03 Astrophys.J. 785, 96 (2014) A.Tumino, R.Sparta, C.Spitaleri, A.M.Mukhamedzhanov, S.Typel, R.G.Pizzone, E.Tognelli, S.Degl'Innocenti, V.Burjan, V.Kroha, Z.Hons, M.La Cognata, L.Lamia, J.Mrazek, S.Piskor, P.G.Prada Moroni, G.G.Rapisarda, S.Romano, M.L.Sergi New Determination of the 2H(d, p)3H and 2H(d, n)3He Reaction Rates at Astrophysical Energies NUCLEAR REACTIONS 2H(3He, pt), E=17 MeV;2H(3He, n3He), E=18 MeV; measured reaction products, Ep, Ip; deduced σ(θ), S-factors, reaction rates, inputs for FRANEC evolutionary code. Comparison with available data.
doi: 10.1088/0004-637X/785/2/96
2014TU04 Acta Phys.Pol. B45, 181 (2014) A.Tumino, C.Spitaleri, M.La Cognata, M.L.Sergi, S.Cherubini, M.Gulino, L.Lamia, R.G.Pizzone, S.M.R.Puglia, G.G.Rapisarda, S.Romano, R.SpartA From Nuclei to Stars with a Trojan Horse
doi: 10.5506/APhysPolB.45.181
2013TU05 Few-Body Systems 54, 745 (2013) A.Tumino, C.Spitaleri, S.Cherubini, M.Gulino, M.La Cognata, L.Lamia, R.G.Pizzone, S.M.R.Puglia, G.G.Rapisarda, S.Romano, M.L.Sergi, R.Sparta New Advances in the Trojan Horse Method as an Indirect Approach to Nuclear Astrophysics
doi: 10.1007/s00601-012-0407-1
2012LA01 J.Phys.(London) G39, 015106 (2012) L.Lamia, C.Spitaleri, V.Burjan, N.Carlin, S.Cherubini, V.Crucilla, M.G.Munhoz, M.G.Del Santo, M.Gulino, Z.Hons, G.G.Kiss, V.Kroha, S.Kubono, M.La Cognata, C.Li, J.Mrazek, A.Mukhamedzhanov, R.G.Pizzone, S.M.R.Puglia, Q.Wen, G.G.Rapisarda, C.Rolfs, S.Romano, M.L.Sergi, E.Somorjai, F.A.Souza, A.Szanto de Toledo, G.Tabacaru, A.Tumino, Y.Wakabayashi, H.Yamaguchi, S.-H.Zhou New measurement of the 11B(p, α0)8Be bare-nucleus S(E) factor via the Trojan horse method NUCLEAR REACTIONS 2H(11B, α), E=27 MeV; measured reaction products, Eα, Iα. 8Be; deduced σ(θ), S-factors.
doi: 10.1088/0954-3899/39/1/015106
2012LA29 Phys.Rev.Lett. 109, 232701 (2012) M.La Cognata, C.Spitaleri, O.Trippella, G.G.Kiss, G.V.Rogachev, A.M.Mukhamedzhanov, M.Avila, G.L.Guardo, E.Koshchiy, A.Kuchera, L.Lamia, S.M.R.Puglia, S.Romano, D.Santiago, R.Sparta Measurement of the -3 keV Resonance in the Reaction 13C(α, n)16O of Importance in the s-Process NUCLEAR REACTIONS 13C(6Li, X)16O, E=7.82 MeV; measured reaction products, deuterons; deduced σ(θ, E), S-factors. Comparison with available data.
doi: 10.1103/PhysRevLett.109.232701
2012RO32 Prog.Theor.Phys.(Kyoto), Suppl. 196, 184 (2012) G.V.Rogachev, M.Avila, S.Cherubini, V.Z.Goldberg, M.Gulino, E.D.Johnson, A.N.Kuchera, M.La Cognata, L.Lamia, S.Romano, L.E.Miller, R.G.Pizzone, G.G.Rapisarda, M.L.Sergi, C.Spitaleri, R.E.Tribble, W.H.Trzaska, A.Tumino Clustering in Non-Self-Conjugate Nuclei NUCLEAR REACTIONS 9Be(p, α), E(cm)=2-5.5 MeV; 4He(14C, X)18O, E(cm)=2-7 MeV; measured reaction products, Eα, Iα; deduced σ(θ), resonance parameters. Comparison with available data, R-matrix fit.
doi: 10.1143/PTPS.196.184
2012TU05 J.Phys.:Conf.Ser. 337, 012017 (2012) A.Tumino, C.Spitaleri, A.M.Mukhamedzhanov, S.Typel, M.Aliotta, V.Burjan, M.G.del Santo, G.G.Kiss, V.Kroha, Z.Hons, M.La Cognata, L.Lamia, J.Mrazek, R.G.Pizzone, S.Piskor, G.G.Rapisarda, S.Romano, M.L.Sergi, R.Sparta Bare nucleus S(E) factor of the 2H(d, p)3H and 2H(d, n)3He reactions via the Trojan Horse Method NUCLEAR REACTIONS 2H(3He, pT), (3He, n3He), E(cm)≈0.002-2 MeV; measured reaction products; deduced 2H(d, p) and 2H(d, n) S-factor using THM (Trojan horse method) with quasifree kinematics. Compared with other THM and also with direct data.
doi: 10.1088/1742-6596/337/1/012017
2011CH08 Acta Phys.Pol. B42, 769 (2011) S.Cherubini, C.Spitaleri, M.Gulino, M.La Cognata, R.G.Pizzone, L.Lamia, G.G.Rapisarda, S.Romano, L.Sergi, A.Mukhamedzhanov, L.Trache, R.E.Tribble, S.Kubono, H.Yamaguchi, A.Tumino Recent Studies on Trojan Horse Method
doi: 10.5506/APhysPolB.42.769
2011KU24 Phys.Rev. C 84, 054615 (2011); Erratum Phys.Rev. C 85, 069902 (2012); Erratum Phys.Rev. C 88, 039901 (2013) A.N.Kuchera, G.V.Rogachev, V.Z.Goldberg, E.D.Johnson, S.Cherubini, M.Gulino, M.La Cognata, L.Lamia, S.Romano, L.E.Miller, R.G.Pizzone, G.G.Rapisarda, M.L.Sergi, C.Spitaleri, R.E.Tribble, W.H.Trzaska, A.Tumino Molecular structures in T=1 states of 10B NUCLEAR REACTIONS 1H(9Be, α)6Li*, E=22.3-55.6 MeV; measure Eα, Iα, particle spectra, σ(E, θ). 10B; deduced levels, J, π, isospin, widths, cluster state, highly deformed molecular type rotational band. R-matrix analysis of excitation functions and angular distributions. Comparison with level structure in 10Be.
doi: 10.1103/PhysRevC.84.054615
2011LA13 Astrophys.J. 739, L54 (2011) M.La Cognata, A.M.Mukhamedzhanov, C.Spitaleri, I.Indelicato, M.Aliotta, V.Burjan, S.Cherubini, A.Coc, M.Gulino, Z.Hons, G.G.Kiss, V.Kroha, L.Lamia, J.Mrazek, S.Palmerini, S.Piskor, R.G.Pizzone, S.M.R.Puglia, G.G.Rapisarda, S.Romano, M.L.Sergi, A.Tumino The Fluorine Destruction in Stars: First Experimental Study of the 19F(p, α0)16O Reaction at Astrophysical Energies NUCLEAR REACTIONS 2H(19F, nα), E=50 MeV; 19F(3He, αd), E=18.2 MeV; measured reaction products, 16O recoils; deduced σ(E, θ), S-factors, reaction rates. Comparison with previous results.
doi: 10.1088/2041-8205/739/2/L54
2011MU14 Phys.Rev. C 84, 024616 (2011) A.M.Mukhamedzhanov, V.Burjan, M.Gulino, Z.Hons, V.Kroha, M.McCleskey, J.Mrazek, N.Nguyen, F.M.Nunes, S.Piskor, S.Romano, M.L.Sergi, C.Spitaleri, R.E.Tribble Asymptotic normalization coefficients from the 14C(d, p)15C reaction NUCLEAR REACTIONS 14C(d, p), E=17.06 MeV; measured ep, Ip, σ(θ). 15C; deduced levels, J, π, l-transfer, asymptotic normalization coefficients for removal of neutron from the g.s. and first exited state of 15C, FR-ADWA analysis with CH-89 potential parameters. 14C(d, d), E=17.06 MeV; measured deuteron spectra, σ(θ); deduced potential parameters. Relevance to 14C(n, γ)15C reaction at astrophysical energies.
doi: 10.1103/PhysRevC.84.024616
2011NO07 Eur.Phys.J. A 47, 73 (2011) M.Norrby, T.Lonnroth, V.Z.Goldberg, G.V.Rogachev, M.S.Golovkov, K.-M.Kallman, M.Lattuada, S.V.Perov, S.Romano, B.B.Skorodumov, G.P.Tiourin, W.H.Trzaska, A.Tumino, A.N.Vorontsov Highly excited alpha-cluster states in 34S NUCLEAR REACTIONS 4He(30Si, α), E=150 MeV; measured thick target Eα, Iα(θ). 34S; deduced levels, resonances, J, π, L-transfers, dσ(Eα), σ(θ), Γα/Γ, Γ, resonance parameters. R-matrix analysis.
doi: 10.1140/epja/i2011-11073-8
2011NO12 Eur.Phys.J. A 47, 96 (2011) M.Norrby, T.Lonnroth, V.Z.Goldberg, G.V.Rogachev, M.S.Golovkov, K.-M.Kallman, M.Lattuada, S.V.Perov, S.Romano, B.B.Skorodumov, G.P.Tiourin, W.H.Trzaska, A.Tumino, A.N.Vorontsov Elastic alpha-particle resonances as evidence of clustering at high excitation in 40Ca NUCLEAR REACTIONS 4He(36Ar, 36Ar), E=150 MeV; measured thick target Eα, Iα(θ). 40Ca deduced resonance parameters, moments of inertia.
doi: 10.1140/epja/i2011-11096-1
2011PI04 Phys.Rev. C 83, 045801 (2011) R.G.Pizzone, C.Spitaleri, L.Lamia, C.Bertulani, A.Mukhamedzhanov, L.Blokhintsev, V.Burjan, S.Cherubini, Z.Hons, G.G.Kiss, V.Kroha, M.La Cognata, C.Li, J.Mrazek, S.Piskor, S.M.R.Puglia, G.G.Rapisarda, S.Romano, M.L.Sergi, A.Tumino Trojan horse particle invariance studied with the 6Li(d, α)4He and 7Li( p, α)4He reactions NUCLEAR REACTIONS 6Li(3He, 2α), E=17.5 MeV; measured Eα, Iα, angular distribution; deduced momentum distribution, Q value, quasifree (QF) contribution. 6Li(d, α), E(cm)=0-5 MeV; 7Li(p, α), E(cm)=0-7 MeV; 7Li(3He, 2α), E not given; analyzed excitation functions, σ, differential σ. Trojan horse method (THM) in the framework of the plane wave approximation.
doi: 10.1103/PhysRevC.83.045801
2011TU04 Few-Body Systems 50, 323 (2011) A.Tumino, C.Spitaleri, A.Mukhamedzhanov, S.Typel, M.Aliotta, V.Burjan, M.G.del Santo, G.G.Kiss, V.Kroha, Z.Hons, M.La Cognata, L.Lamia, J.Mrazek, R.G. Pizzone, S.Piskor, G.G.Rapisarda, S.Romano, M.L.Sergi, R.Sparta Indirect Study of the 2H(d, p)3H and 2H(d, n)3He Reactions at Astrophysical Energies via the Trojan Horse Method NUCLEAR REACTIONS 2H(d, p), (d, n), E(cm)=0.02, 0.13, 0.98, 1.25 MeV; measured reaction products, proton spectra; deduced σ(θ). Trojan horse method.
doi: 10.1007/s00601-010-0213-6
2011TU06 Phys.Lett. B 700, 111 (2011), Erratum Phys.Lett. B 705, 546 (2011) A.Tumino, C.Spitaleri, A.M.Mukhamedzhanov, S.Typel, M.Aliotta, V.Burjan, M.G.del Santo, G.G.Kiss, V.Kroha, Z.Hons, M.La Cognata, L.Lamia, J.Mrazek, R.G.Pizzone, S.Piskor, G.G.Rapisarda, S.Romano, M.L.Sergi, R.Sparta Low-energy d+d fusion reactions via the Trojan Horse Method NUCLEAR REACTIONS 2H(3He, X), E=18 MeV; measured reaction products, 3H-p and 3He-p coin.; deduced σ(θ), S-factors for 2H(d, p), (d, n) reactions using Trojan Horse Method. Comparison with experimental data.
doi: 10.1016/j.physletb.2011.05.001
2010GU17 J.Phys.(London) G37, 125105 (2010) M.Gulino, C.Spitaleri, S.Cherubini, V.Crucilla, M.La Cognata, L.Lamia, R.G.Pizzone, S.Romano, M.L.Sergi, A.Tumino, C.-B.Li, Z.Elekes, E.Somorjai, V.Burjan, V.Kroha, A.Mukhamedzhanov Study of the 6Li(n, α)3H reaction via the 2H quasi-free break-up NUCLEAR REACTIONS 2H(6Li, tα), E=14, 17 MeV; measured reaction products; deduced σ for 6Li(n, α) reaction.
doi: 10.1088/0954-3899/37/12/125105
2010LA07 J.Phys.(London) G37, 105105 (2010) M.La Cognata, A.Del Zoppo, R.Alba, S.Cherubini, N.Colonna, A.Di Pietro, P.Figuera, M.Gulino, L.Lamia, A.Musumarra, M.G.Pellegriti, R.G.Pizzone, C.Rolfs, S.Romano, C.Spitaleri, A.Tumino Toward correction-free 8Li(α, n)11B data at the Gamow energy of explosive nucleosynthesis NUCLEAR REACTIONS 4He(8Li, n)11B, E=2-4 MeV; measured reaction products, time, En, In; deduced σ.
doi: 10.1088/0954-3899/37/10/105105
2010LA11 Nucl.Phys. A834, 655c (2010) L.Lamia, S.M.R.Puglia, C.Spitaleri, S.Romano, M.G.Del Santo, N.Carlin, M.G.Munhoz, S.Cherubini, G.G.Kiss, V.Kroha, S.Kubono, M.La Cognata, C.-B.Li, R.G.Pizzone, Q.-G.Wen, M.L.Sergi, A.Szanto de Toledo, Y.Wakabayashi, H.Yamaguchi, S.-H.Zhou Indirect study of 11B(p, α0)8Be and 10B(p, α)7Be reactions at astrophysical energies by means of the Trojan Horse Method: recent results NUCLEAR REACTIONS 2H(11B, α8Be), E=27 MeV; 2H(10B, α7Be), E=24.4 MeV; measured Eα, Iα(θ), E(particle), I(particle). 11B(p, α), E(cm)=0-0.6 MeV; 10B(p, α), E(cm)=0-0.15 MeV; deduced S-factor using Trojan Horse Method.
doi: 10.1016/j.nuclphysa.2010.01.115
2010LA19 J.Phys.:Conf.Ser. 202, 012019 (2010) M.La Cognata, C.Spitaleri, A.Mukhamedzhanov, R.E.Tribble, T.Al-Abdullah, A.Banu, S.Cherubini, A.Coc, V.Crucilla, V.Goldberg, M.Gulino, B.Irgaziev, G.G.Kiss, L.Lamia, J.Mrazek, R.G.Pizzone, S.M.R.Puglia, G.G.Rapisarda, S.Romano, M.L.Sergi, G.Tabacaru, L.Trache, W.Trzaska, S.Tudisco, A.Tumino First measurement of the 18O(p, α)15N cross section at astrophysical energies NUCLEAR REACTIONS 2H(18O, α15N), E=54 MeV; measured Eα, Iα(θ), E(particle), I(particle, θ); deduced dσ, resonances. 18O(p, α), E=0-8 keV; calculated; deduced reaction rate, resonance strengths from 2H(18O, α15N) using Trojan Horse method.
doi: 10.1088/1742-6596/202/1/012019
2010LO12 Eur.Phys.J. A 46, 5 (2010) T.Lonnroth, M.Norrby, V.Z.Goldberg, G.V.Rogachev, M.S.Golovkov, K.-M.Kallman, M.Lattuada, S.V.Perov, S.Romano, B.B.Skorodumov, G.P.Tiourin, W.H.Trzaska, A.Tumino, A.N.Vorontsov Highly excited alpha-cluster states in 32S studied with the thick-target inverse kinematics method NUCLEAR REACTIONS 4He(28Si, 28Si), E=150 MeV; measured thick target Eγ, Iγ, Eα, Iα(θ); deduced resonances E, J, π, α widths, resonance parameters, σ(θ); calculated σ(θ) using R-matrix. Comparison to other data.
doi: 10.1140/epja/i2010-11021-2
2010MU16 J.Phys.:Conf.Ser. 202, 012017 (2010) A.M.Mukhamedzhanov, A.Banu, P.Bem, V.Burjan, C.A.Gagliardi, V.Z.Goldberg, Z.Hons, V.Kroha, M.La Cognata, S.Piskor, R.G.Pizzone, S.Romano, E.Simeckova, C.Spitaleri, L.Trache, R.E.Tribble Asymptotic normalization coefficient and important astrophysical process 15N(p, γ)160 NUCLEAR REACTIONS 15N(p, α), E=0-1200 keV; analyzed published data; calculated S-factor using resonant and nonresonant parts of R-matrix; deduced p ANC (asymptotic normalization coefficient). 15N(p, γ), E=resonance; calculated S-factor using R-matrix and ANC.
doi: 10.1088/1742-6596/202/1/012017
2010PI09 Nucl.Phys. A834, 673c (2010) R.G.Pizzone, C.Spitaleri, S.Cherubini, M.La Cognata, L.Lamia, S.Romano, M.L.Sergi, A.Tumino, C.Li, Q.Wen, S.Zhou, V.Burjan, V.Kroha, J.Mrazek, N.Carlin, M.G.del Santo, A.Szanto de Toledo, S.Kubono, T.Wakabayashi, H.Yamaguchi, C.Rolfs Trojan Horse Method: a useful tool for electron screening effect investigation NUCLEAR REACTIONS 2H(3He, p), 6Li(p, α), 6Li(d, α), 7Li(p, α), 9Be(p, α), E not given; calculated electron screening effect with Trojan Horse Method.
doi: 10.1016/j.nuclphysa.2010.01.121
2010PI14 J.Phys.:Conf.Ser. 202, 012018 (2010) R.G.Pizzone, C.Spitaleri, S.Cherubini, M.La Cognata, L.Lamia, S.Romano, M.L.Sergi, C.Rolfs, F.Strieder, V.Burjan, V.Kroha, J.Mrazek, C.Li, Q.Wen, S.Zhou, A.Tumino Trojan Horse Method: A tool to explore electron screening effect
doi: 10.1088/1742-6596/202/1/012018
2010SE13 Phys.Rev. C 82, 032801 (2010) M.L.Sergi, C.Spitaleri, M.La Cognata, A.Coc, A.Mukhamedzhanov, S.V.Burjan, S.Cherubini, V.Crucilla, M.Gulino, F.Hammache, Z.Hons, B.Irgaziev, G.G.Kiss, V.Kroha, L.Lamia, R.G.Pizzone, S.M.R.Puglia, G.G.Rapisarda, S.Romano, N.de Sereville, E.Somorjai, S.Tudisco, A.Tumino New high accuracy measurement of the 17O(p, α)14N reaction rate at astrophysical temperatures NUCLEAR REACTIONS 2H(17O, α14N), E=41 MeV; measured 14N spectrum, σ(θ), momentum distribution and differential σ for resonances above the 18F proton threshold. 18F; deduced resonances and levels. Comparison of experimental momentum distribution with plane-wave impulse approximation (PWIA) and distorted-wave Born approximation (DWBA) calculations. 17O(p, α)14N; deduced reaction rates of astrophysical relevance.
doi: 10.1103/PhysRevC.82.032801
2010SE21 J.Phys.:Conf.Ser. 202, 012021 (2010) M.L.Sergi, C.Spitaleri, A.Coc, A.Mukhamedzhanov, V.Burjan, S.Cherubini, V.Crucilla, M.Gulino, F.Hammache, V.Z.Hons, B.Irgaziev, G.Kiss, V.Kroha, M.La Cognata, L.Lamia, R.G.Pizzone, S.M.R.Puglia, G.G.Rapisarda, S.Romano, N.de Sereville, E.Somorjai, S.Tudisco, A.Tumino Indirect measurement of 17O(p, α)14N cross section at ultra-low energies NUCLEAR REACTIONS 2H(17O, α14N), E=41 MeV; measured E(particle), I(particle, θ) using position sensitive detectors and ionization chambers; deduced neutron momentum distribution. 17O(p, α), E(cm)=0-0.7 MeV; deduced σ(θ) from 2H(17O, α14N), E=41 MeV using Trojan Horse method in PWIA approach.
doi: 10.1088/1742-6596/202/1/012021
2010SP04 Nucl.Phys. A834, 639c (2010) C.Spitaleri, S.Cherubini, M.La Cognata, L.Lamia, A.Mukhamedzhanov, R.G.Pizzone, S.Romano, M.L.Sergi, A.Tumino Trojan Horse Method: recent applications in nuclear astrophysics
doi: 10.1016/j.nuclphysa.2010.01.111
2010TU06 J.Phys.:Conf.Ser. 205, 012048 (2010) A.Tumino, C.Spitaleri, S.Cherubini, M.La Cognata, L.Lamia, R.G.Pizzone, S.M.R.Puglia, G.G.Rapisarda, S.Romano, M.L.Sergi The Trojan Horse method as an indirect approach for nuclear astrophysics studies NUCLEAR REACTIONS 6Li(p, α), E(cm)=0.01-2 MeV; compared earlier calculation of S-factor done by the authors for Trojan Horse method with data of Engstler. 2H(18O, α15N), E not given;deduced dσ for 18O(p, α), E(cm)=0-250 MeV using data of La Cognata and Trojan horse method. 2H(p, 2p), E not given; deduced 1H(p, p'), E(cm)=0.05-0.7 MeV σ using Trojan horse method with OES (on-energy-shell) model of Jackson and Blatt and recent HOES (half-off-energy-shell) by the authors.
doi: 10.1088/1742-6596/205/1/012048
2009MI23 Eur.Phys.J. A 41, 335 (2009) M.Milin, V.V.Ostashko, D.Miljanic, H.G.Bohlen, A.Di Pietro, O.Yu.Goryunov, Tz.Kokalova, M.Lattuada, A.Musumarra, W.von Oertzen, M.G.Pellegriti, S.Romano, S.Thummerer, A.Tumino, M.Zadro States in 17O excited in the 13C + 9Be → 13C + 2α + n reaction at 90 MeV NUCLEAR REACTIONS 9Be(13C, α), E=90 MeV; measured Eα, Iα, E(13C), 13Cα-coin; deduced 17O excitation energy spectrum. 17O; deduced levels, J, π. Comparison with other data.
doi: 10.1140/epja/i2009-10827-1
2009PI12 Phys.Rev. C 80, 025807 (2009) R.G.Pizzone, C.Spitaleri, A.M.Mukhamedzhanov, L.D.Blokhintsev, C.A.Bertulani, B.F.Irgaziev, M.La Cognata, L.Lamia, S.Romano Effects of distortion of the intercluster motion in 2H, 3He, 3H, 6Li, and 9Be on Trojan horse applications NUCLEAR REACTIONS 2H(p, 2p), E=5, 6 MeV; 2H(t, pt), E=35.5 MeV; 2H(3He, p3He), E=17 MeV; 2H(6Li, 3Heα), E=25 MeV; 2H(9Be, α6Li), E=22 MeV; 2H(10B, α7Be), (11B, α8Be), E=27 MeV; 2H(7Li, 2α), E=20 MeV; 2H(15N, α12C), E=60 MeV; 2H(18O, α15N), E=54 MeV; 3H(3He, d3He), (3He, p3He), E=65 MeV; 3H(3He, 2d), E=50, 65, 78 MeV; 3H(3He, pt), E=78 MeV; 3H(d, 2d), E=35 MeV; 3H(p, 2p), (p, pd), E=45.6 MeV; 3He(p, pd), E=65, 85, 100, 590 MeV; 3He(d, pt), E=17, 35, 52 MeV; 3He(d, p3He), E=18 MeV; 6Li(6Li, 2α)4He, E=2.1-44 MeV; 7Li(3He, 2α), E=11, 12, 33 MeV; 9Be(p, pα)5He, E=47, 55, 57, 160 MeV; 9Be(3He, 2α)4He, E=2.8, 3, 4 MeV; 9Be(p, dα), E=30 MeV; 9Be(7Li, α7Li), E=52 MeV; 9Be(α, 2α), E=140 MeV; calculated widths (FWHM) of momentum distributions of the spectator particles using the Trojan Horse method and compared with the experimental data.
doi: 10.1103/PhysRevC.80.025807
2008LA06 J.Phys.(London) G35, 014014 (2008) M.La Cognata, C.Spitaleri, R.E.Tribble, T.Al-Abdullah, A.Banu, S.Cherubini, V.Crucilla, C.Fu, V.Goldberg, M.Gulino, L.Lamia, A.Mukhamedzhanov, R.G.Pizzone, S.M.R.Puglia, G.G.Rapisarda, S.Romano, M.L.Sergi, G.Tabacaru, L.Trache, S.Tudisco, A.Tumino, S.Typel, Y.Zhai Indirect measurement of the 18O(p, α)15N reaction rate through the THM NUCLEAR REACTIONS 2H(18O, α15N)n, E=54 MeV; measured charged particle spectra, angular and momentum distributions, cross sections; 18O(p, α)15N, E(cm)=0-1.5 MeV; deduced S-factor, reaction rate. Trojan Horse Method.
doi: 10.1088/0954-3899/35/1/014014
2008LA08 Phys.Lett. B 664, 157 (2008) M.La Cognata, A.Del Zoppo, P.Figuera, A.Musumarra, R.Alba, S.Cherubini, N.Colonna, L.Cosentino, V.Crucilla, A.Di Pietro, M.Gulino, L.Lamia, M.G.Pellegriti, R.G.Pizzone, S.M.R.Puglia, G.G.Rapisarda, C.Rolfs, S.Romano, M.L.Sergi, C.Spitaleri, S.Tudisco, A.Tumino On the magnitude of the 8Li + 4He → 11B + n reaction cross section at the Big-Bang temperature NUCLEAR REACTIONS 4He(8Li, n), E(cm)=1.05 MeV; 4He(9Be, n), E(cm)=1.45 MeV; measured En, In, σ. Comparison with other data.
doi: 10.1016/j.physletb.2008.05.026
2008LA13 Phys.Rev.Lett. 101, 152501 (2008) M.La Cognata, C.Spitaleri, A.M.Mukhamedzhanov, B.Irgaziev, R.E.Tribble, A.Banu, S.Cherubini, A.Coc, V.Crucilla, V.Z.Goldberg, M.Gulino, G.G.Kiss, L.Lamia, J.Mrazek, R.G.Pizzone, S.M.R.Puglia, G.G.Rapisarda, S.Romano, M.L.Sergi, G.Tabacaru, L.Trache, W.Trzaska, A.Tumino Measurement of the 20 and 90 keV Resonances in the 18O(p, α)15N Reaction via the Trojan Horse Method NUCLEAR REACTIONS 2H(18O, nα), E=54 MeV; measured σ(θ, E). 18O(p, α), E=0-250 keV; deduced σ(θ). 19F; deduced low lying resonance strengths. Discussed astrophysical implications.
doi: 10.1103/PhysRevLett.101.152501
2008LA17 Few-Body Systems 44, 353 (2008) M.La Cognata, C.Spitaleri, S.Cherubini, M.Gulino, L.Lamia, R.G.Pizzone, S.M.R.Puglia, G.G.Rapisarda, S.Romano, M.L.Sergi, A.Tumino Pole approximation in the quasi-free t+p scattering and the t(p, d)d reaction via the t+d interaction NUCLEAR REACTIONS 2H(t, pt), (t, 2d), E=35.5 MeV; measured cross sections. 3H(p, p), (p, d); deduced cross sections.
doi: 10.1007/s00601-008-0325-4
2008LA18 Nuovo Cim. B 31, 423 (2008) L.Lamia, C.Spitaleri, N.Carlin, S.Cherubini, M.G.Del Santo, M.Gulino, M.La Cognata, M.G.Munhoz, R.G.Pizzone, S.M.R.Puglia, G.G.Rapisarda, S.Romano, M.L.Sergi, A.Szanto de Toledo, S.Tudisco, A.Tumino Indirect study of (p, α) and (n, α) reactions induced on boron isotopes NUCLEAR REACTIONS 2H(11B, nα), (10B, pα), E=27 MeV; measured Eα, Iα, fragment spectra, cross sections. 11B(p, α), 10B(n, α); deduced S-factors.
doi: 10.1393/ncc/i2009-10303-2
2008MU15 Phys.Rev. C 78, 015804 (2008) A.M.Mukhamedzhanov, P.Bem, V.Burjan, C.A.Gagliardi, V.Z.Goldberg, Z.Hons, M.La Cognata, V.Kroha, J.Mrazek, J.Novak, S.Piskor, R.G.Pizzone, A.Plunkett, S.Romano, E.Simeckova, C.Spitaleri, L.Trache, R.E.Tribble, F.Vesely, J.Vincour New astrophysical S factor for the 15N(p, γ)16O reaction via the asymptotic normalization coefficient (ANC) method NUCLEAR REACTIONS 15N(3He, d), E=25.74 MeV; measured deuteron spectra, asymptotic normalization coefficients, angular distributions. 15N(p, γ), (p, α); deduced astrophysical S-factors, resonance parameters.
doi: 10.1103/PhysRevC.78.015804
2008RO05 J.Phys.(London) G35, 014008 (2008) S.Romano, C.Spitaleri, S.Cherubini, V.Crucilla, M.Gulino, M.La Cognata, L.Lamia, R.G.Pizzone, S.M.R.Puglia, G.G.Rapisarda, M.L.Sergi, S.Tudisco, A.Tumino, R.E.Tribble, V.Z.Goldberg, A.M.Mukhamedzhanov, G.Tabacaru, L.Trache, V.Kroha, V.Burjan, Z.Hons, J.Mrazek, E.Somorjai, Z.Elekes, Z.Fulop, G.Gyurky, G.Kiss, A.Szanto de Toledo, N.Carlin, M.M.De Moura, M.G.Del Santo, M.G.Munhoz, R.Liguori Neto, F.A.Souza, A.A.P.Suaide, E.Szanto The Trojan horse method in nuclear astrophysics: recent results NUCLEAR REACTIONS 7Li(p, α)α, E(cm)=0-7 MeV; 10B(p, α)7Be, E(cm)=0-400 keV; p(p, p)p, E ≈ 0-0.6 MeV; analyzed cross section, S-factors.Trojan Horse Method.
doi: 10.1088/0954-3899/35/1/014008
2008TU07 Phys.Rev. C 78, 064001 (2008) A.Tumino, C.Spitaleri, A.Mukhamedzhanov, G.G.Rapisarda, L.Campajola, S.Cherubini, V.Crucilla, Z.Elekes, Z.Fulop, L.Gialanella, M.Gulino, G.Gyurky, G.Kiss, M.La Cognata, L.Lamia, A.Ordine, R.G.Pizzone, S.Romano, M.L.Sergi, E.Somorjai Off-energy-shell p-p scattering at sub-Coulomb energies via the Trojan horse method NUCLEAR REACTIONS 2H(p, 2p), E=5 MeV; measured Ep, Ip, pp-coin, momentum distributions, two- and three-body σ. Trojan Horse Method.
doi: 10.1103/PhysRevC.78.064001
2007LA25 Nucl.Phys. A787, 309c (2007) L.Lamia, S.Romano, N.Carlin, S.Cherubini, V.Crucilla, M.M.De Moura, M.G.Del Santo, M.G.Munhoz, M.Gulino, R.Liguori Neto, M.La Cognata, F.Mudo, R.G.Pizzone, S.M.R.Puglia, M.L.Sergi, F.A.Souza, C.Spitaleri, A.A.P.Suaide, E.Szanto, A.Szanto de Toledo, S.Tudisco, A.Tumino Boron depletion: indirect measurement of the 10B(p, α)7Be S(E)-factor NUCLEAR REACTIONS 2H(10B, nα), E=27 MeV; measured Eα, Iα, σ; deduced astrophysical S-factor. Trojan horse method, three-body process.
doi: 10.1016/j.nuclphysa.2006.12.049
2007LA37 Phys.Rev. C 76, 065804 (2007) M.La Cognata, S.Romano, C.Spitaleri, S.Cherubini, V.Crucilla, M.Gulino, L.Lamia, R.G.Pizzone, A.Tumino, R.Tribble, C.Fu, V.Z.Goldberg, A.M.Mukhamedzhanov, D.Schmidt, G.Tabacaru, L.Trache, B.F.Irgaziev Astrophysical S(E) factor of the 15N(p, α)12C reaction at sub-Coulomb energies via the Trojan horse method NUCLEAR REACTIONS 2H(15N, nα), E=60 MeV; measured 12C energies, particle coincidences, momentum. 15N(p, α)12C, E(cm)=19.2-576.0 MeV; deduced angular distributions, excitation functions, astrophysical S-factors using Trojan horse method.
doi: 10.1103/PhysRevC.76.065804
2007MU10 Nucl.Phys. A787, 321c (2007) A.M.Mukhamedzhanov, L.D.Blokhintsev, S.Brown, V.Burjan, S.Cherubini, V.Z.Goldberg, M.Gulino, B.F.Irgaziev, E.Johnson, K.Kemper, V.Kroha, M.La Cognata, L.Lamia, A.Momotyuk, R.G.Pizzone, B.Roeder, G.Rogachev, S.Romano, C.Spitaleri, R.E.Tribble, A.Tumino Indirect Techniques in Nuclear Astrophysics. Asymptotic Normalization Coefficient and Trojan Horse NUCLEAR REACTIONS 13C(α, n), E=0-0.9 MeV; calculated astrophysical S-factor. Asymptotic normalization coefficient method. Comparison with data. 6Li(d, α), 7Li(p, α), E=0-800 keV; calculated astrophysical S-factor. Trojan horse method.
doi: 10.1016/j.nuclphysa.2006.12.051
2007OS03 Ukr.J.Phys. 52, 525 (2007) V.Ostashko, M.Lattuada, O.Goryunov, A.Di Pietro, D.Miljanic, M.Zadro, A.Musumara, M.-G.Pellegriti, S.Romano, S.Tudisco, A.Tumino, P.Figuera 8Be nucleus resonances at the excitation energy Ex < 35 MeV in the three-particle reaction 9Be + 13C → 14C + α + α NUCLEAR REACTIONS 9Be(13C, α14C), E=89.45 MeV; measured particle energies and coincidences. 8Be deduced levels.
2007OS05 Iader.Fiz.Enerh. 8 no.1, 45 (2007) V.Ostashko, M.Lattuada, M.Milin, O.Goryunov, A.Di Pietro, D.Miljanic, M.Zadro, A.Musumara, M.-G.Pellegriti, S.Romano, S.Tudisco, A.Tumino, P.Figuera Investigation of α-3He resonances at relative energy 1<Ex<20 in three particles processes 9Be + 13C → 15C + α + 3He NUCLEAR REACTIONS 9Be(13C, 15C), E=89.45 MeV; measured reaction products. 7Be;deduced energies of resonances.
doi: 10.15407/jnpae
2007TU02 Phys.Rev.Lett. 98, 252502 (2007) A.Tumino, C.Spitaleri, A.Mukhamedzhanov, G.G.Rapisarda, S.Cherubini, V.Crucilla, Z.Elekes, Z.Fulop, M.Gulino, G.Gyurky, G.Kiss, M.La Cognata, L.Lamia, F.Mudo, R.G.Pizzone, S.Romano, M.L.Sergi, E.Somorjai Suppression of the Coulomb Interaction in the Off-Energy-Shell p - p Scattering form the p + d → p + p + m Reaction NUCLEAR REACTIONS 2H(p, 2p), E=5 MeV; measured cross sections. Analyzed data using the Trojan Horse Method to deduce off-energy shell effects on p-p scattering.
doi: 10.1103/PhysRevLett.98.252502
2007TU04 Nucl.Phys. A787, 337c (2007) A.Tumino, C.Spitaleri, G.G.Rapisarda, S.Cherubini, S.Blagus, M.Bogovac, V.Crucilla, Z.Elekes, Z.Fulop, M.Gulino, G.Gyurky, G.Kiss, M.La Cognata, L.Lamia, Dj.Miljanic, M.Milin, F.Mudo, A.Mukhamedzhanov, R.G.Pizzone, D.Rendic, S.Romano, M.L.Sergi, E.Somorjai No signature of nuclear-Coulomb interference in the proton-proton elastic scattering via the Trojan Horse Method NUCLEAR REACTIONS 2H(p, 2p), E=5, 6 MeV; measured Ep, Ip, σ(E, θ). Plane wave impulse approximation, Trojan horse method.
doi: 10.1016/j.nuclphysa.2006.12.053
2006AG11 Nucl.Instrum.Methods Phys.Res. A565, 406 (2006) C.Agodi, R.Alba, L.Calabretta, S.Cherubini, L.Cosentino, A.Del Zoppo, A.Di Pietro, P.Figuera, M.Gulino, A.Musumarra, M.G.Pellegriti, R.Pizzone, C.Rolfs, S.Romano, C.Spitaleri, S.Tudisco, A.Tumino In flight production of a 8Li radioactive beam for Big Bang nucleosynthesis investigations at LNS Catania NUCLEAR REACTIONS 2H, C(7Li, X)4He/7Li/8Li/7Be/8B/11B, E=23 MeV; measured yields. 4He(8Li, n), E(cm) ≈ 1.25 MeV; measured σ.
doi: 10.1016/j.nima.2006.06.053
2006LA18 Eur.Phys.J. A 27, Supplement 1, 249 (2006) M.La Cognata, S.Romano, C.Spitaleri, R.Tribble, L.Trache, S.Cherubini, C.Fu, L.Lamia, A.Mukhamedzhanov, R.G.Pizzone, C.Rolfs, G.Tabacaru, A.Tumino Indirect measurement of the 15N(p, α)12C reaction cross section through the Trojan-Horse Method NUCLEAR REACTIONS 2H(15N, nα), E=60 MeV; measured particle spectra, correlations; deduced quasi-free contribution. 15N(p, α), E(cm) ≈ 0-600 keV; deduced astrophysical S-factor.
doi: 10.1140/epja/i2006-08-039-0
2006MU15 Eur.Phys.J. A 27, Supplement 1, 205 (2006) A.M.Mukhamedzhanov, L.D.Blokhintsev, B.A.Brown, V.Burjan, S.Cherubini, C.A.Gagliardi, B.F.Irgaziev, V.Kroha, F.M.Nunes, F.Pirlepesov, R.G.Pizzone, S.Romano, C.Spitaleri, X.D.Tang, L.Trache, R.E.Tribble, A.Tumino Indirect techniques in nuclear astrophysics: Asymptotic Normalization Coefficient and Trojan Horse NUCLEAR REACTIONS 14N(3He, d), E=26.3 MeV; measured σ(θ). 14N(p, γ), E ≈ 100-600 keV; deduced astrophysical S-factor. 11C, 13N(p, γ), E not given; analyzed resonant and nonresonant amplitudes. Asymptotic normalization coefficient and Trojan horse techniques discussed.
doi: 10.1140/epja/i2006-08-032-7
2006OS06 Iader.Fiz.Enerh. 7 no.2, 34 (2006) V.Ostashko, M.Lattuada, M.Milin, O.Goryunov, A.Di Pietro, D.Miljanic, M.Zadro, A.Musumara, M.-G.Pellegriti, S.Romano, S.Tudisco, A.Tumino, P.Figuera, H.Bohlen, W.von Oertzen, T.Kokalova, S.Shumerer Cluster structure of 9Be from many-particles reactions NUCLEAR REACTIONS 9Be(13C, α), (13C, 2α), E=89.45 MeV; measured reaction products, Eα, Iα, particleα-coin. 9Be; deduced resonance energies, possible J, π, cluster structure - α-5He and n-8Be of 9nuclei.
doi: 10.15407/jnpae
2006RO33 Eur.Phys.J. A 27, Supplement 1, 221 (2006) S.Romano, L.Lamia, C.Spitaleri, C.Li, S.Cherubini, M.Gulino, M.La Cognata, R.G.Pizzone, A.Tumino Study of the 9Be(p, α)6Li reaction via the Trojan Horse Method NUCLEAR REACTIONS 2H(9Be, nα), E=22 MeV; measured particle spectra, σ(θ). 9Be(p, α), E(cm) ≈ 0-1 MeV; deduced excitation function. Comparison with direct data.
doi: 10.1140/epja/i2006-08-034-5
2006TU08 Eur.Phys.J. A 27, Supplement 1, 243 (2006) A.Tumino, C.Spitaleri, M.L.Sergi, V.Kroha, V.Burjan, S.Cherubini, Zs.Fulop, M.La Cognata, L.Lamia, J.Novac, R.G.Pizzone, S.Romano, E.Somorjai, S.Tudisco, J.Vincour Validity test of the Trojan Horse Method applied to the 7Li + p → α + α reaction via the 3He break-up NUCLEAR REACTIONS 7Li(3He, 2α), E=33 MeV; measured Eα, αα-coin; deduced quasi-free contribution. 7Li(p, α), E(cm) ≈ 0-7 MeV; deduced σ.
doi: 10.1140/epja/i2006-08-038-1
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
2005MU27 J.Phys.(London) G31, S1413 (2005) A.M.Mukhamedzhanov, E.O.Alt, L.D.Blokhintsev, S.Cherubini, B.F.Irgaziev, A.S.Kadyrov, D.Miljanic, A.Musumarra, M.G.Pellegriti, F.Pirlepesov, C.Rolfs, S.Romano, C.Spitaleri, N.K.Timofeyuk, R.E.Tribble, A.Tumino Few-body problems in nuclear astrophysics
doi: 10.1088/0954-3899/31/10/005
2005PI12 Phys.Rev. C 71, 058801 (2005) R.G.Pizzone, C.Spitaleri, S.Cherubini, M.La Cognata, L.Lamia, D.Miljanic, A.Musumarra, S.Romano, A.Tumino, S.Tudisco, S.Typel Influence of the α-d motion in 6Li on Trojan horse applications NUCLEAR REACTIONS 6Li(6Li, 2α), E ≈ 2-44 MeV; 3He(6Li, pα), E=5, 6 MeV; analyzed data. 6Li deduced α-d momentum distribution. 6Li(d, α), E(cm) ≈ 0-0.6 MeV; calculated astrophysical S-factor, role of target nucleus α-d momentum distribution.
doi: 10.1103/PhysRevC.71.058801
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
2004BB25 Iader.Fiz.Enerh. 5 no.1, 7 (2004) Z.Bazrak, D.Vincheguera, O.Y.Goryunov, S.Zilner, M.Lattuada, V.V.Ostashko, S.Tudisco, A.Tumino, S.Romano, C.Spitaleri, P.Figuera High energy excitation region of 24Mg in the 12C(16O, 16O, 8Be)α reaction study NUCLEAR REACTIONS 12C(16O, 3α), E=109 MeV; measured reaction products, (particle)(particle)-coin. 24Mg; deduced resonance energies, possible J.
doi: 10.15407/jnpae
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
2004GO03 Phys.Rev. C 69, 024602 (2004) V.Z.Goldberg, G.V.Rogachev, W.H.Trzaska, J.J.Kolata, A.Andreyev, C.Angulo, M.J.G.Borge, S.Cherubini, G.Chubarian, G.Crowley, P.Van Duppen, M.Gorska, M.Gulino, M.Huyse, P.Jesinger, K.-M.Kallman, M.Lattuada, T.Lonnroth, M.Mutterer, R.Raabe, S.Romano, M.V.Rozhkov, B.B.Skorodumov, C.Spitaleri, O.Tengblad, A.Tumino Investigation of the α-cluster structure of 22Ne and 22Mg NUCLEAR REACTIONS 4He(18O, 18O), E < 80 MeV; 4He(18Ne, 18Ne), E < 53 MeV; measured σ(θ), excitation functions. 22Ne deduced resonance energies, J, π, widths, α-cluster features. 22Mg deduced level energies, J, α-cluster features. Thick-target inverse kinematics method.
doi: 10.1103/PhysRevC.69.024602
2004PE21 Prog.Theor.Phys.(Kyoto), Suppl. 154, 349 (2004) M.G.Pellegriti, C.Spitaleri, A.Musumarra, L.Calabretta, S.Cherubini, A.Di Pietro, P.Figuera, R.G.Pizzone, S.Romano, S.Tudisco, A.Tumino Coulomb Suppression Effects in the Proton-Proton Elastic Scattering Extracted from the 2H(p, pp)n Reaction NUCLEAR REACTIONS 2H(p, 2p), E=6 MeV; measured Ep, pp-coin. 1H(p, p), E=0.3-0.8 MeV; deduced σ, Coulomb supression effects. Trojan horse method.
doi: 10.1143/PTPS.154.349
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
2004SO35 Fizika(Zagreb) B 13, 433 (2004) N.Soic, S.Blagus, M.Bogovac, W.Catford, S.Cherubini, N.Clarke, E.Costanzo, L.Donadille, S.Fazinic, M.Freer, B.Fulton, B.Greenhalgh, K.Jones, M.Lattuada, P.Leask, D.Mahboub, M.Milin, D.Miljanic, D.Rendic, S.Romano, C.Spitaleri, T.Tadic, D.Watson, D.Weisser, M.Zadro Experimental evidence for molecular structures in light nuclei NUCLEAR REACTIONS 7Li(7Li, 2α), E=8, 30 MeV; 9Be(7Li, 7Li), (7Li, α6Li), (7Li, α7Li), E=52 MeV; 7Li(9Be, α9Be), (9Be, α10Be), E=70 MeV; measured excitation energy spectra. 9,10Be, 13,14C deduced excited states, cluster structures.
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
2003GO38 Acta Phys.Hung.N.S. 18, 215 (2003) V.Z.Goldberg, W.H.Trzaska, G.V.Rogachev, J.J.Kolata, A.Andreyev, C.Angulo, M.J.G.Borge, S.Cherubini, G.Chubarian, G.Crowley, A.S.Fomichev, M.Gorska, M.Gulino, M.S.Golovkov, M.Huyse, K.-M.Kallman, M.Lattuada, T.Lonnroth, M.Mutterer, R.Raabe, A.M.Rodin, S.Romano, M.V.Rozhkov, B.B.Skorodumov, C.Spitaleri, O.Tengblad, G.M.Ter-Akopian, A.Tumino, P.Van Duppen, R.Wolski New Perspectives in the Studies of Resonance Scattering
doi: 10.1556/APH.18.2003.2-4.15
2003PI13 Nucl.Phys. A718, 496c (2003) R.G.Pizzone, C.Spitaleri, M.Lattuada, A.Musumarra, M.G.Pellegriti, S.Romano, A.Tumino, S.Cherubini, P.Figuera, D.Miljanic, C.Rolfs, S.Typel, H.H.Wolter, V.Castellani, S.Degl'Innocenti, A.Imperio Bare astrophysical S(E)-factor for the 6Li(d, α)4He and 7Li(p, α)4He reactions at astrophysical energies NUCLEAR REACTIONS 6Li(d, α), 7Li(p, α), E(cm) ≈ 10-1000 keV; analyzed astrophysical S-factors, electron screening potential energy.
doi: 10.1016/S0375-9474(03)00868-6
2003PI14 Nucl.Phys. B(Proc.Supp.) S118, 455 (2003) R.G.Pizzone, C.Spitaleri, M.Lattuada, A.Musumarra, M.G.Pellegriti, C.Rolfs, D.Miljanic, A.Di Pietro, P.Figuera, S.Romano, S.Tudisco, A.Tumino, S.Typel, H.H.Wolter, V.Castellani, S.Degl'Innocenti, A.Imperio The 7Li(p, α)4He fusion reaction studied via the Trojan Horse Method and its astrophysical implications NUCLEAR REACTIONS 7Li(d, 2α), E not given; measured not given. 7Li(p, α), E=low; deduced astrophysical S-factor, electron screening potential.
doi: 10.1016/S0920-5632(03)01356-2
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