NSR Query Results
Output year order : Descending NSR database version of April 11, 2024. Search: Author = R.G.Pizzone Found 131 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
2022LA01 Phys.Lett. B 826, 136917 (2022) M.La Cognata, S.Palmerini, P.Adsley, F.Hammache, A.Di Pietro, P.Figuera, R.Alba, S.Cherubini, F.Dell'Agli, G.L.Guardo, M.Gulino, L.Lamia, D.Lattuada, C.Maiolino, A.Oliva, R.G.Pizzone, P.M.Prajapati, S.Ramano, D.Santonocito, R.Sparta, M.L.Sergi, A.Tumino Exploring the astrophysical energy range of the 27Al(p, α)24Mg reaction: A new recommended reaction rate NUCLEAR REACTIONS 2H(27Al, α24Mg)1NN, E<1.5 MeV; measured reaction products. 28Si, 24Mg; deduced σ(θ, E), strengths of the levels, astrophysical reaction rates. The indirect Trojan Horse method (THM), INFN-LNS Tandem accelerator (Catania, Italy).
doi: 10.1016/j.physletb.2022.136917
2022LA06 Phys.Rev. C 105, 044618 (2022) H.Y.Lan, W.Luo, Y.Xu, D.L.Balabanski, G.L.Guardo, M.La Cognata, D.Lattuada, C.Matei, R.G.Pizzone, T.Rauscher, J.L.Zhou Feasibility of studying astrophysically important charged-particle emission with the variable energy γ-ray system at the Extreme Light Infrastructure--Nuclear Physics facility NUCLEAR REACTIONS 29Si, 47Ti, 56Fe, 73Ge, 74Se, 84Sr, 91Zr, 95Mo, 96,98Ru, 102Pd, 106Cd, 115,117,119Sn, 132Ba, 143Nd(γ, p), (γ, np), E<30 MeV; 50V, 67Zn, 87Sr, 107Ag, 113,115In, 119Sn, 123,125Te, 149,154Sm, 155,156,157,158,160Gd, 208Pb(γ, α), (γ, nα), E<30 MeV; calculated inclusive and exclusive σ(E), population of the particular excited states, energy spectra of ejectiles. TALYS-1.9 calculations with various combinations of level densities, strength functions and optical potentials available in the code.Investigated the feasibility of studying the reactions of astrophysical interest with ELI-NP facility infrastructure. Simulated achievable yields.
doi: 10.1103/PhysRevC.105.044618
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
2022PR09 Pramana 96, 167 (2022) P.M.Prajapati, R.G.Pizzone, A.Hingu, S.Mukherjee, S.V.Suryanarayana Production and characterisation of 20, 22Ne targets NUCLEAR REACTIONS 22Ne(p, γ), E=639 keV; 20Ne(p, γ), E=1169 keV; measured reaction products; deduced neon concentration depth profiling. Nuclear resonance analysis (NRA), Rutherford backscattering (RBS), elastic recoil detection analysis (ERDA) and proton-induced X-ray emission (PIXE) methods. The 6 MV Tandetron facility at the Advanced Technologies Research Institute of the Faculty of Materials Science and Technology in Trnava. The Ion Beam Centre (IBC), Helmholtz Zentrum Dresden Rossendorf (HZDR), Dresden.
doi: 10.1007/s12043-022-02397-w
2022SC17 J.Phys.(London) G49, 110502 (2022) H.Schatz, A.D.Becerril Reyes, A.Best, E.F.Brown, K.Chatziioannou, K.A.Chipps, C.M.Deibel, R.Ezzeddine, D.K.Galloway, C.J.Hansen, F.Herwig, A.P.Ji, M.Lugaro, Z.Meisel, D.Norman, J.S.Read, L.F.Roberts, A.Spyrou, I.Tews, F.X.Timmes, C.Travaglio, N.Vassh, C.Abia, P.Adsley, S.Agarwal, M.Aliotta, W.Aoki, A.Arcones, A.Aryan, A.Bandyopadhyay, A.Banu, D.W.Bardayan, J.Barnes, A.Bauswein, T.C.Beers, J.Bishop, T.Boztepe, B.Cote, M.E.Caplan, A.E.Champagne, J.A.Clark, M.Couder, A.Couture, S.E.de Mink, S.Debnath, R.J.deBoer, J.den Hartogh, P.Denissenkov, V.Dexheimer, I.Dillmann, J.E.Escher, M.A.Famiano, R.Farmer, R.Fisher, C.Frohlich, A.Frebel, C.Fryer, G.Fuller, A.K.Ganguly, S.Ghosh, B.K.Gibson, T.Gorda, K.N.Gourgouliatos, V.Graber, M.Gupta, W.C.Haxton, A.Heger, W.R.Hix, W.C.G.Ho, E.M.Holmbeck, A.A.Hood, S.Huth, G.Imbriani, R.G.Izzard, R.Jain, H.Jayatissa, Z.Johnston, T.Kajino, A.Kankainen, G.G.Kiss, A.Kwiatkowski, M.La Cognata, A.M.Laird, L.Lamia, P.Landry, E.Laplace, K.D.Launey, D.Leahy, G.Leckenby, A.Lennarz, B.Longfellow, A.E.Lovell, W.G.Lynch, S.M.Lyons, K.Maeda, E.Masha, C.Matei, J.Merc, B.Messer, F.Montes, A.Mukherjee, M.R.Mumpower, D.Neto, B.Nevins, W.G.Newton, L.Q.Nguyen, K.Nishikawa, N.Nishimura, F.M.Nunes, E.O'Connor, B.W.O'Shea, W.-J.Ong, S.D.Pain, M.A.Pajkos, M.Pignatari, R.G.Pizzone, V.M.Placco, T.Plewa, B.Pritychenko, A.Psaltis, D.Puentes, Y.-Z.Qian, D.Radice, D.Rapagnani, B.M.Rebeiro, R.Reifarth, A.L.Richard, N.Rijal, I.U.Roederer, J.S.Rojo, J.S K, Y.Saito, A.Schwenk, M.L.Sergi, R.S.Sidhu, A.Simon, T.Sivarani, A.Skuladottir, M.S.Smith, A.Spiridon, T.M.Sprouse, S.Starrfield, A.W.Steiner, F.Strieder, I.Sultana, R.Surman, T.Szucs, A.Tawfik, F.Thielemann, L.Trache, R.Trappitsch, M.B.Tsang, A.Tumino, S.Upadhyayula, J.O.Valle Martinez, M.Van der Swaelmen, C.Viscasillas Vazquez, A.Watts, B.Wehmeyer, M.Wiescher, C.Wrede, J.Yoon, R.G.T.Zegers, M.A.Zermane, M.Zingale, the Horizon 2020 Collaborations Horizons: nuclear astrophysics in the 2020s and beyond
doi: https://dx.doi.org/10.1088/1361-6471/ac8890
2021CH38 Astrophys.J. 916, 79 (2021) A.Chieffi, L.Roberti, M.Limongi, M.La Cognata, L.Lamia, S.Palmerini, R.G.Pizzone, R.Sparta, A.Tumino Impact of the New Measurement of the 12C + 12C Fusion Cross Section on the Final Compactness of Massive Stars NUCLEAR REACTIONS 12C(12C, X)24Mg, E<1 MeV; analyzed available data; deduced impact on the dependence of the compactness on the initial mass with respect to previous findings by adopting the classical cross section.
doi: 10.3847/1538-4357/ac06ca
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
2020MU07 Phys.Rev. C 101, 055801 (2020) M.Munch, C.Matei, S.D.Pain, M.T.Febbraro, K.A.Chipps, H.J.Karwowski, C.Aa.Diget, A.Pappalardo, S.Chesnevskaya, G.L.Guardo, D.Walter, D.L.Balabanski, F.D.Becchetti, C.R.Brune, K.Y.Chae, J.Frost-Schenk, M.J.Kim, M.S.Kwag, M.La Cognata, D.Lattuada, R.G.Pizzone, G.G.Rapisarda, G.V.Turturica, C.A.Ur, Y.Xu Measurement of the 7Li(γ, t)4He ground-state cross section between Eγ = 4.4. and 10 MeV NUCLEAR REACTIONS 7Li(γ, t), E=4.4-10 MeV from High Intensity Gamma-ray Source (HIγS) at TUNL; measured E(t), I(t), Eα, Iα, Eγ and Iγ, αt-coin, ground state σ(E) using the SIDAR silicon detector array. 3H(α, γ), E(cm)=0-7 MeV; deduced astrophysical S-factor from R-matrix analysis. Comparison with model predictions, and with previous experimental results. Relevance to primordial Li problem and the mirror α-capture reactions.
doi: 10.1103/PhysRevC.101.055801
2020NA31 Phys.Atomic Nuclei 83, 520 (2020) D.K.Nauruzbayev, A.K.Nurmukhanbetova, V.Z.Goldberg, M.La Cognata, A.Di Pietro, P.Figuera, S.Cherubini, M.Gulino, L.Lamia, R.G.Pizzone, R.Sparta, A.Tumino, A.Serikov, E.M.Gazeeva Strong Resonances at High Excitation Energy in 17O + Alpha Resonance Scattering NUCLEAR REACTIONS 4He(17O, α), E=54.4 MeV; measured reaction products. 21Ne; deduced σ(E), very strong resonances at high energies of 8.6 MeV.
doi: 10.1134/S1063778820040158
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
2020PI17 Eur.Phys.J. A 56, 283 (2020) R.G.Pizzone, C.A.Bertulani, L.Lamia, M.La Cognata, M.L.Sergi, R.Sparta, A.Tumino Clusters and their fundamental role for Trojan Horse Method NUCLEAR REACTIONS 6Li(d, α), E(cm)<3 MeV; 7Li(p, α), E(cm)<7 MeV; 2H(d, p), E(cm)<0.9 MeV; analyzed available data; deduced S-factors, momentum distributions within the framework of the Plane Wave Impulse Approximation (PWIA). The Trojan Horse Method (THM).
doi: 10.1140/epja/s10050-020-00285-8
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
2019BR08 Riv.Nuovo Cimento Soc.Ital.Fis. 42, 103 (2019) C.Broggini, O.Straniero, M.G.F.Taiuti, G.de Angelis, G.Benzoni G.E.Bruno, S.Bufalino, G.Cardella, N.Colonna, M.Contalbrigo, G.Cosentino, S.Cristallo, C.Curceanu, E.De Filippo, R.Depalo, A.Di Leva, A.Feliciello, S.Gammino, A.Galata, M.La Cognata, R.Lea, S.Leoni, I.Lombardo, V.Manzari, D.Mascali, C.Massimi, A.Mengoni, D.Mengoni, D.R.Napoli, S.Palmerini, S.Piano, S.Pirrone, R.G.Pizzone, G.Politi, P.Prati, G.Prete, P.Russotto, G.Tagliente, G.M.Urciuoli Experimental nuclear astrophysics in Italy
doi: 10.1393/ncr/i2019-10157-1
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
2019SP05 Eur.Phys.J. A 55, 161 (2019) C.Spitaleri, M.La Cognata, L.Lamia, R.G.Pizzone, A.Tumino Astrophysics studies with the Trojan Horse Method
doi: 10.1140/epja/i2019-12833-0
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
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
2018TU05 Few-Body Systems 59, 54 (2018) A.Tumino, A.Bonasera, G.Giuliani, M.Lattuada, M.Milin, R.G.Pizzone, C.Spitaleri, S.Tudisco Triple α Resonances and Possible Link to the Efimov Trimers NUCLEAR REACTIONS 6Li(6Li, 3α), E=3.1 MeV; analyzed available data. 12C, 8Be; deduced a strong enhancement in the α-α coincidence yields.
doi: 10.1007/s00601-018-1374-y
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
2017GU05 Phys.Rev. C 95, 025807 (2017) G.L.Guardo, C.Spitaleri, L.Lamia, M.Gulino, M.La Cognata, X.Tang, R.deBoer, X.Fang, V.Goldberg, J.Mrazek, A.Mukhamedzhanov, M.Notani, R.G.Pizzone, G.G.Rapisarda, M.L.Sergi, M.Wiescher Assessing the near threshold cross section of the 17O(n, α)14C reaction by means of the Trojan horse method NUCLEAR REACTIONS 2H(17O, α14C), E=43.5 MeV; measured reaction products, particle spectra, (particle)(particle)-coin, angular distributions using two telescopes of ionization chambers (IC) and silicon position-sensitive detector (PSD) at LNS-Catania and NSL-Notre Dame accelerator facilities; deduced normalized reaction yields, experimental momentum distribution, quasifission (QF) cross sections and best fit from R-matrix analysis. 18O; deduced levels, resonances, J, π, and Trojan horse method (THM) analysis of Γn, Γα and total widths. 17O(n, α)14C, T9=0.01-10; deduce astrophysical reaction rates by THM method.
doi: 10.1103/PhysRevC.95.025807
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
2017LA12 Astrophys.J. 846, 65 (2017) M.La Cognata, R.G.Pizzone, J.Jose, M.Hernanz, S.Cherubini, M.Gulino, G.G.Rapisarda, and C.Spitaleri A Trojan Horse Approach to the Production of 18F in Novae NUCLEAR REACTIONS 18F(p, α), E(cm)<1 MeV; analyzed available data using R-matrix formalism; deduced S-factors changes.
doi: 10.3847/1538-4357/aa845f
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
2017LI10 Phys.Rev. C 95, 035804 (2017); Pub.Note Phys.Rev. C 95, 039905 (2017) C.Li, Q.Wen, A.Tumino, Y.Fu, J.Zhou, S.Zhou, Q.Meng, C.Spitaleri, R.G.Pizzone, L.Lamia Beam-energy dependence and updated test of the Trojan-horse nucleus invariance via a measurement of the 2H(d, p)3H reaction at low energies NUCLEAR REACTIONS 2H(d, pt)4He, E=11 MeV; measured proton and triton spectra, astrophysical S(E) factors at Beijing National Tandem Accelerator Laboratory of the CIAE; deduced mass spectrum of the three outgoing particles. Trojan-horse method.
doi: 10.1103/PhysRevC.95.035804
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
2017TO14 Phys.Rev. C 96, 044317 (2017) D.Torresi, C.Wheldon, Tz.Kokalova, S.Bailey, A.Boiano, C.Boiano, M.Fisichella, M.Mazzocco, C.Parascandolo, D.Pierroutsakou, E.Strano, M.Zadro, M.Cavallaro, S.Cherubini, N.Curtis, A.Di Pietro, J.P.Fernandez-Garcia, P.Figuera, T.Glodariu, J.Grebosz, M.La Cognata, M.La Commara, M.Lattuada, D.Mengoni, R.G.Pizzone, C.Signorini, C.Stefanini, L.Stroe, C.Spitaleri Evidence for 15O + α resonance structures in 19Ne via direct measurement NUCLEAR REACTIONS 4He(15O, α), E=28.5 MeV, [secondary 15O beam from 1H(15N, 15O), E=80 MeV primary reaction at LNL-XTU, Legnaro tandem Van de Graaff accelerator; measured Eα, Iα using a double-sided silicon strip detector (DSSSD), absolute differential cross sections. 19Ne; deduced levels, resonances, J, π, Γα, total Γ, partial decay branches, reduced α-widths, 15O+α rotational band, cluster structure using R-matrix analysis with AZURE2 code. Comparison with previous experimental results, and with potential model calculation using the well-known 16O+α cluster band configurations. Relevance to α branching ratio in the astrophysical reaction rate for high-spin near-threshold resonances.
doi: 10.1103/PhysRevC.96.044317
2016PI01 Eur.Phys.J. A 52, 24 (2016) R.G.Pizzone, B.T.Roeder, M.McCleskey, L.Trache, R.E.Tribble, C.Spitaleri, C.A.Bertulani, S.Cherubini, M.Gulino, I.Indelicato, M.La Cognata, L.Lamia, G.G.Rapisarda, R.Sparta Trojan Horse measurement of the 18F(p, α)15O astrophysical S(E)-factor NUCLEAR REACTIONS 2H(18F, nα), E=52 MeV; measured α-particles using TESCA, 15O using X1-PSD detectors; deduced deuteron breakup momentum distribution. 18F(p, α), E not given; deduced reaction rate vs nuclear temperature, σ(θ), S-factor for individual levels vs E(cm) using Trojan Horse method.
doi: 10.1140/epja/i2016-16024-3
2016SP03 Eur.Phys.J. A 52, 77 (2016) C.Spitaleri, M.La Cognata, L.Lamia, A.M.Mukhamedzhanov, R.G.Pizzone Nuclear astrophysics and the Trojan Horse Method NUCLEAR REACTIONS 2H(d, p), (d, n), E(cm)=0.003-3 MeV;6,7Li(p, α), E(cm)=0.01-1 MeV;13C(α, n), E(cm)=0-1.2 MeV;19F(p, α0), E(cm)=0-1.0 MeV; compiled S-factor data, fitting THM (Trojan Horse Method) and calculations. 6,7Li(p, α), T=0.001-10 GK; compiled, compared THM and NACRE reaction rates.
doi: 10.1140/epja/i2016-16077-2
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
2015LA20 Astrophys.J. 811, 99 (2015) L.Lamia, C.Spitaleri, E.Tognelli, S.Degl'Innocenti, R.G.Pizzone, P.G.Prada Moroni Astrophysical impact of the updated 9Be (p, α)6Li and 10B(p, α)7Be reaction rates as deduced by THM NUCLEAR REACTIONS 9Be, 10B(p, α), E(cm)<0.5 MeV; calculated σ, S-factors, reaction rates using Trojan Horse Method. Comparison with NACRE library.
doi: 10.1088/0004-637X/811/2/99
2015LI34 Phys.Rev. C 92, 025805 (2015) C.Li, Q.Wen, Y.Fu, J.Zhou, S.Zhou, Q.-Y.Meng, C.Spitaleri, A.Tumino, R.G.Pizzone, L.Lamia Measurement of the 2H (d, p) 3H reaction at astrophysical energies via the Trojan-horse method NUCLEAR REACTIONS 2H(6Li, pt)4He, E=9.5 MeV; measured proton and triton spectra using position-sensitive detectors at HI-13 Tandem Accelerator Laboratory of the CIAE; deduced Q3-value spectrum, E1-E2 kinematic plot, momentum distribution of α inside 6Li. 2H(d, p)3H; deduced astrophysical S(E) factor and screening potential Ue using Trojan-horse method applied to the quasifree process. Relevance to nucleosynthesis in standard Big Bang and stellar evolution, as well as in future fusion reactor designs.
doi: 10.1103/PhysRevC.92.025805
2015SE08 Phys.Rev. C 91, 065803 (2015) M.L.Sergi, C.Spitaleri, M.La Cognata, L.Lamia, R.G.Pizzone, G.G.Rapisarda, X.D.Tang, B.Bucher, M.Couder, P.Davies, R.deBoer, X.Fang, L.Lamm, C.Ma, M.Notani, S.O'Brien, D.Roberson, W.Tan, M.Wiescher, B.Irgaziev, A.Mukhamedzhanov, J.Mrazek, V.Kroha Improvement of the high-accuracy 17O(p, α)14N reaction-rate measurement via the Trojan Horse method for application to 17O nucleosynthesis NUCLEAR REACTIONS 2H(17O, α14N)n, E=41, 43.5 MeV; measured particle spectra, (14N)α-coin at LNS-Catania and NSL-Notre Dame accelerator facilities; deduced Q-value spectra, yields as function of 14N and α emission angles, E(14N-α) versus E(α-n) plots, neutron momentum distributions, (14N)α-coincidence yields for different neutron momentum ranges, differential σ(E) of the Trojan-Horse reaction. 18F; deduced parameters for the two resonance levels, resonance strengths for the 65-keV resonance. 17O(p, α)14N; deduced reaction rates via Trojan Horse Method (THM). 18F; compiled resonance energies, J, π, Γp, Γα, Γγ for 24 resonances from -3.12 keV to 1684.5 keV. Relevance to destruction of 17O and the formation of 18F in stellar sites.
doi: 10.1103/PhysRevC.91.065803
2015SP01 Phys.Rev. C 91, 024612 (2015) C.Spitaleri, A.Tumino, M.Lattuada, R.G.Pizzone, S.Tudisco, DJ.Miljanic, S.Blagus, M.Milin, N.Skukan, N.Soic Quasifree mechanism in the 6Li + 6Li → 3α reaction at low energy NUCLEAR REACTIONS 6Li(6Li, X)3α, E=2.5, 3.1 MeV; measured particle spectra, (particle)(particle)-, αα-coin, differential cross sections, correlation curves, momentum distribution, αα-angular correlation spectra; deduced evidence for quasifree mechanism and for an a-particle spectator either in the target or in the projectile. Analysis by plane wave impulse approximation. 8Be; deduced level, J, π, width.
doi: 10.1103/PhysRevC.91.024612
2015TU06 Phys.Lett. B 750, 59 (2015) A.Tumino, A.Bonasera, G.Giuliani, M.Lattuada, M.Milin, R.G.Pizzone, C.Spitaleri, S.Tudisco Triple α resonances in the 6Li + 6Li → 3α reaction at low energy NUCLEAR REACTIONS 6Li(6Li, α)8Be, E=3.1 MeV; measured reaction products, Eα, Iα; deduced σ(θ, E), possible Efimov states. The hyperspherical formalism for the low-energy three-body problem.
doi: 10.1016/j.physletb.2015.08.052
2014CA31 Phys.Rev. C 90, 034601 (2014) R.J.Casperson, J.T.Burke, N.D.Scielzo, J.E.Escher, E.McCleskey, M.McCleskey, A.Saastamoinen, A.Spiridon, A.Ratkiewicz, A.Blanc, M.Kurokawa, R.G.Pizzone Measurement of the 240Am (n, f) cross section using the surrogate-ratio method NUCLEAR REACTIONS 243Am, 238U(p, F)3H, 243Am, 238U(p, p'), (p, d), E=38.4 MeV; measured particle and fission fragment spectra, (particle)(fission fragment)-coin using STARLiTeR array of Si detectors at Texas A and M facility. 235U, 240Am(n, F), E=200 keV-14 MeV; deduced σ(E) using results for surrogate reactions 243Am, 238U(p, F)3H. Comparison with previous experimental results. Comparison with several evaluated libraries shows disagreement and a need for re-evaluation.
doi: 10.1103/PhysRevC.90.034601
2014PI08 Few-Body Systems 55, 1001 (2014) R.G.Pizzone, C.Spitaleri, M.L.Sergi, L.Lamia, A.Tumino, C.A.Bertulani, L.Blokhintsev, V.Burjan, V.Kroha, M.La Cognata, J.Mrazek, A.M.Mukhamedzhanov, R.Sparta Trojan Horse Particle Invariance: An Extensive Study
doi: 10.1007/s00601-014-0829-z
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
2013GU02 Phys.Rev. C 87, 012801 (2013) M.Gulino, C.Spitaleri, X.D.Tang, G.L.Guardo, L.Lamia, S.Cherubini, B.Bucher, V.Burjan, M.Couder, P.Davies, R.deBoer, X.Fang, V.Z.Goldberg, Z.Hons, V.Kroha, L.Lamm, M.La Cognata, C.Li, C.Ma, J.Mrazek, A.M.Mukhamedzhanov, M.Notani, S.O'Brien, R.G.Pizzone, G.G.Rapisarda, D.Roberson, M.L.Sergi, W.Tan, I.J.Thompson, M.Wiescher Suppression of the centrifugal barrier effects in the off-energy-shell neutron + 17O interaction NUCLEAR REACTIONS 2H(17O, α14C), E=41, 43.5 MeV; measured α and 14C particle spectra, (14C)α-coin, angular distributions, yields using position-sensitive silicon detectors (PSD) at LNS, Catania, and at NSL, Notre Dame. CD2 target; deduced momentum distributions, Q value. DWBA analysis. 17O(n, α)14C, E(cm)=0-350 keV; deduced yields, angular distributions, neutron from quasifree breakup of deuteron. 18O; deduced resonances, J, π, and excitation functions. Trojan Horse method (THM), and suppression of centrifugal barrier. Comparison with previous studies. Relevance to neutron-induced reactions in nuclear reactors, and nucleosynthesis in astrophysics.
doi: 10.1103/PhysRevC.87.012801
2013LA13 Astrophys.J. 768, 65 (2013) L.Lamia, C.Spitaleri, R.G.Pizzone, E.Tognelli, A.Tumino, S.Degl'Innocenti, P.G.Prada Moroni, M.La Cognata, L.Pappalardo, M.L.Sergi An Updated 6Li(p, α)3He Reaction Rate at Astrophysical Energies with the Trojan Horse Method NUCLEAR REACTIONS 6Li(p, α), E(cm)<1 MeV; analyzed available S-factors, reaction rates; deduced importance of this reaction for 6Li destruction in astrophysical environment.
doi: 10.1088/0004-637X/768/1/65
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
2013SO11 Phys.Rev. C 87, 054329 (2013) L.G.Sobotka, W.W.Buhro, R.J.Charity, J.M.Elson, M.F.Jager, J.Manfredi, M.H.Mahzoon, A.M.Mukhamedzhanov, V.Eremenko, M.McCleskey, R.G.Pizzone, B.T.Roeder, A.Spiridon, E.Simmons, L.Trache, M.Kurokawa, P.Navratil Proton decay of excited states in 12N and 13O and the astrophysical 11C(p, γ)12N reaction rate NUCLEAR REACTIONS 9Be(13O, X), E=30.3 MeV/nucleon, [13O secondary beam from 1H(14N, X), E=38 MeV/nucleon primary reaction]; measured particle spectra, E(p), I(p), widths using MARS spectrometer at Texas AM cyclotron facility. Invariant mass method. R-matrix analysis. 11C, 12N, 13O; deduced levels, J, π, one-proton and two-proton decay branching ratios. 11C(p, γ)12N; deduced astrophysical reaction rates and S(E) factors.
doi: 10.1103/PhysRevC.87.054329
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
2012CH04 Phys.Rev. C 85, 015805 (2012) J.Chen, A.A.Chen, G.Amadio, S.Cherubini, H.Fujikawa, S.Hayakawa, J.J.He, N.Iwasa, D.Kahl, L.H.Khiem, S.Kubono, S.Kurihara, Y.K.Kwon, M.La Cognata, J.Y.Moon, M.Niikura, S.Nishimura, J.Pearson, R.G.Pizzone, T.Teranishi, Y.Togano, Y.Wakabayashi, H.Yamaguchi Strong 25Al+p resonances via elastic proton scattering with a radioactive 25Al beam NUCLEAR REACTIONS 1H(25Al, p), [25Al secondary beam from 2H(24Mg, n), E=7.5 MeV/nucleon primary reaction], E=3.4 MeV/nucleon; measured Ep, Ip, energy loss, σ(E, θ). 26Si; deduced levels, resonances, J, π, proton widths. R-matrix analysis of excitation function data. RIKEN-CNS facility. Comparison of energy levels with results from other reaction studies.
doi: 10.1103/PhysRevC.85.015805
2012JA11 Phys.Rev. C 86, 011304 (2012);Erratum Phys.Rev. C 86, 059902 (2012) M.F.Jager, R.J.Charity, J.M.Elson, J.Manfredi, H.Mohammad, L.G.Sobotka, M.McCleskey, R.G.Pizzone, B.T.Roeder, A.Spiridon, E.Simmons, L.Trache, M.Kurokawa Two-proton decay of 12O and its isobaric analog state in 12N NUCLEAR REACTIONS 9Be(13O, 12O), (13O, 12N), [13O secondary beam from 1H(14N, X), E=38 MeV/nucleon primary reaction], E=30.3 MeV/nucleon]; measured excitation energy spectra for p+11C, p+12C, 2p+10C, 2p+10B events. Two proton decay modes of g.s. of 12O and excited states of 12O and 12N. 12O, 12N; deduced levels, J, π, widths, IAS of 12O g.s. in 12N. 10B; deduced level, IAS in 10B from 2p decay of IAS in 12N. 13N; deduced level, J, π. RADIOACTIVITY 12O(2p)[9Be(13O, 12O), E=30.3 MeV/nucleon](2p); measured total excitation energy spectra for decay of g.s. of 12O. ATOMIC MASSES 12O, 12N; analyzed isobaric multiplet mass equation (IMME) for A=12 quintet; deduced mass excesses using the invariant mass method.
doi: 10.1103/PhysRevC.86.011304
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
2012LA08 Phys.Rev. C 85, 025805 (2012) L.Lamia, M.La Cognata, C.Spitaleri, B.Irgaziev, R.G.Pizzone Influence of the d-state component of the deuteron wave function on the application of the Trojan horse method NUCLEAR REACTIONS 2H(11B, α8Be), (18O, α15N), E not given; calculated neutron momentum distribution. 11Be, 18O(p, α), E not given; analyzed discrepancy ϵ. Trojan horse method. Contribution of s-wave and d-wave components in deuteron wave function. Comparison with experimental data.
doi: 10.1103/PhysRevC.85.025805
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
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
2011RO60 Nucl.Instrum.Methods Phys.Res. A 634, 71 (2011) B.T.Roeder, M.Mccleskey, L.Trache, A.A.Alharbi, A.Banu, S.Cherubini, T.Davinson, V.Z.Goldberg, M.Gulino, R.G.Pizzone, E.Simmons, R.Sparta, A.Spiridon, C.Spitaleri, J.P.Wallace, R.E.Tribble, P.J.Woods The Texas-Edinburgh-Catania Silicon Array (TECSA): A detector for nuclear astrophysics and nuclear structure studies with rare isotope beams NUCLEAR REACTIONS 2H(14C, p), 14C(d, p), E=163.8 MeV; measured products, 15C, Eπ, Iπ; deduced σ(θ). Data were imported from EXFOR entry C1826.
doi: 10.1016/j.nima.2011.01.035
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
2010LA12 Nucl.Phys. A834, 658c (2010) M.La Cognata, C.Spitaleri, A.Mukhamedzhanov, V.Goldberg, B.Irgaziev, L.Lamia, R.G.Pizzone, M.L.Sergi, R.E.Tribble DWBA momentum distribution and its effect on THM NUCLEAR REACTIONS 2H(18O, α15N), E(cm)≈5.4 MeV; calculated wave function momentum distribution using DWBA. Comparison with data.
doi: 10.1016/j.nuclphysa.2010.01.116
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
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
2010SE11 Nucl.Phys. A834, 676c (2010) M.L.Sergi, C.Spitaleri, A.Coc, A.Mukhamedzhanov, S.V.Burjan, M.Gulino, F.Hammache, Z.Hons, B.Irgaziev, G.G.Kiss, V.Kroha, M.La Cognata, L.Lamia, R.G.Pizzone, N.de Sereville, E.Somorjai The 65 keV resonance in the 17O(p, α)14N thermonuclear reaction NUCLEAR REACTIONS 2H(17O, α14N), E=41 MeV; measured σ, σ(θ). 17O(p, α), E=0-0.7 MeV; deduced σ(θ). 18F; deduced levels using Trojan Horse Method.
doi: 10.1016/j.nuclphysa.2010.01.122
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
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
2008WE08 Phys.Rev. C 78, 035805 (2008) Q.-G.Wen, C.-B.Li, S.-H.Zhou, Q.-Y.Meng, J.Zhou, X.-M.Li, S.-Y.Hu, Y.-Y.Fu, C.Spitaleri, A.Tumino, R.G.Pizzone, G.G.Rapisarda Trojan horse method applied to 9Be(p, α)6Li at astrophysical energies NUCLEAR REACTIONS 2H(9Be, nα), E=22.35 MeV; measured Qp value, angular distributions, momentum distributions. 9Be(p, α); deduced astrophysical S-factor, σ, electron screening potential energy. Trojan Horse method.
doi: 10.1103/PhysRevC.78.035805
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
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
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