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NSR database version of April 11, 2024.

Search: Author = M.La Cognata

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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
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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
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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
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2022BA13      Riv.Nuovo Cimento Soc.Ital.Fis. 45, 189 (2022); Erratum Riv.Nuovo Cimento Soc.Ital.Fis. 45, 277 (2022)

A.Badala, M.La Cognata, R.Nania, M.Osipenko, S.Piantelli, R.Turrisi, L.Barion, S.Capra, D.Carbone, F.Carnesecchi, E.A.R.Casula, C.Chatterjee, G.F.Ciani, R.Depalo, A.Di Nitto, A.Fantini, A.Goasduff, G.L.Guardo, A.C.Kraan, A.Manna, L.Marsicano, N.S.Martorana, L.Morales-Gallegos, E.Naselli, A.Scordo, S.Valdre, G.Volpe

Trends in particle and nuclei identification techniques in nuclear physics experiments

doi: 10.1007/s40766-021-00028-5
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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
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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
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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
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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
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2022MA37      Universe 8, 80 (2022)

D.Mascali, D.Santonocito, S.Amaducci, L.Ando, V.Antonuccio, S.Biri, A.Bonanno, V.P.Bonanno, S.Briefi, M.Busso, L.Celona, L.Cosentino, S.Cristallo, M.Cuffiani, C.De Angelis, G.De Angelis, D.De Salvador, L.Di Donato, J.-E.Ducret, A.Eshkevar Vakili, U.Fantz, A.Galata, C.Gallo, S.Gammino, T.Isernia, H.Koivisto, K.-L.Kratz, R.Kronholm, M.La Cognata, S.Leoni, A.Locatelli, M.Maggiore, F.Maimone, L.Malferrari, G.Mancini, L.Maunoury, G.S.Mauro, M.Mazzaglia, A.Mengoni, A.Miraglia, B.Mishra, M.Musumeci, D.R.Napoli, E.Naselli, F.Odorici, L.Palladino, G.Palmisano, S.Pavone, S.Pennisi, A.Perego, A.Pidatella, R.Racz, R.Reitano, D.Rifuggiato, M.Rinaldi, A.D.Russo, F.Russo, G.Schillaci, S.Selleri, S.Simonucci, G.Sorbello, R.Sparta, S.Taioli, K.Tinschert, G.Torrisi, A.Trifiro, S.Tsikata, A.Tumino, D.Vescovi, L.Vincetti

A Novel Approach to β-Decay: PANDORA, a New Experimental Setup for Future In-Plasma Measurements

RADIOACTIVITY 94Nb, 134Cs, 176Lu(β-); calculated stellar to terrestrial T1/2 of β- decay of these isotopes as a function of temperature from 0.5-1000 MK; reviewed novel approach to measure β- decay rates of radionuclides relevant in nuclear-astrophysics under the PANDORA (Plasmas for Astrophysics, Nuclear Decay Observation and Radiation for Archaeometry) project at the INFN-LNS-Catania facility.

doi: 10.3390/universe8020080
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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
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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
Citations: PlumX Metrics


2021AD01      Phys.Rev. C 103, 015805 (2021)

P.Adsley, U.Battino, A.Best, A.Caciolli, A.Guglielmetti, G.Imbriani, H.Jayatissa, M.La Cognata, L.Lamia, E.Masha, C.Massimi, S.Palmerini, A.Tattersall, R.Hirschi

Reevaluation of the 22Ne(α, γ)26Mg and 22Ne(α, n)25Mg reaction rates

NUCLEAR REACTIONS 22Ne(α, γ); 25Mg(n, γ); 22Ne(6Li, d); 26Mg(γ, γ'), (p, p'), (d, d'), (α, α'); 11B(16O, p); evaluated experimental data. 26Mg; evaluated nuclear data for levels, resonances, J, π, resonance energies and resonance strengths for (α, γ) and (α, n) reactions, Γα, Γp, Γn. 22Ne(α, γ)26Mg, T=0.010-1.250 GK; 22Ne(α, n)25Mg, T=0.030-1.250 GK; recommended reaction rates, ratios of reaction rates, based on present evaluation and using different statistical methods. Comparison with theoretical predictions. Relevance to weak s process in evolved massive stars and in the helium flash in low-mass AGB stars.

doi: 10.1103/PhysRevC.103.015805
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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
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD1035. Data from this article have been entered in the XUNDL database. For more information, click here.


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
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset23652.


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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetE2724. Data from this article have been entered in the XUNDL database. For more information, click here.


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
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Data from this article have been entered in the XUNDL database. For more information, click here.


2021SP02      Eur.Phys.J. A 57, 20 (2021)

C.Spitaleri, S.Typel, C.A.Bertulani, A.M.Mukhamedzhanov, T.Kajino, M.Lattuada, A.Cvetinovic, S.Messina, G.L.Guardo, N.Soic, M.Milin, S.S.Perrotta, C.Li, P.Colovic, G.D'Agata, D.Dell'Aquila, C.G.Fatuzzo, M.Gulino, S.Q.Hou, M.La Cognata, D.Lattuada, D.Nurkic, R.Popocovski, N.Skukan, S.Szilner, O.Trippella, M.Uroic, N.Vukman

The 3He + 5He → α+α reaction below the Coulomb barrier via the Trojan Horse Method

NUCLEAR REACTIONS 9Be(3He, 2α), E=4 MeV; 3He(5He, α), E(cm)<1 Mev; measured reaction products, Eα, Iα; deduced two α-particles σ(θ, E), σ(θ). Comparison with theoretical calculations, Trojan Horse Method (THM).

doi: 10.1140/epja/s10050-020-00324-4
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD1037.


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
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2021SP06      Phys.Lett. B 820, 136477 (2021)

R.Sparta, A.Di Pietro, P.Figuera, O.Tengblad, A.M.Moro, I.Martel, J.P.Fernandez-Garcia, J.Lei, L.Acosta, M.J.G.Borge, G.Bruni, J.Cederkall, T.Davinson, J.D.Ovejas, L.M.Fraile, D.Galaviz, J.H.Jensen, B.Jonson, M.La Cognata, A.Perea, A.M.Sanchez-Benitez, N.Soic, S.Vinals

Probing proton halo effects in the 8B+64Zn collision around the Coulomb barrier

NUCLEAR REACTIONS 64Zn(8B, 8B), (8B, X)7Be, E=4.9 MeV/nucleon; measured reaction products. 8B; deduced σ(θ, E). Comparison with continuum-discretized coupled-channels (CDCC) calculations.

doi: 10.1016/j.physletb.2021.136477
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2598. Data from this article have been entered in the XUNDL database. For more information, click here.


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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetL0260. Data from this article have been entered in the XUNDL database. For more information, click here.


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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD8026.


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
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset14716.


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
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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
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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
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD0956. Data from this article have been entered in the XUNDL database. For more information, click here.


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
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset31824. Data from this article have been entered in the XUNDL database. For more information, click here.


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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2432. Data from this article have been entered in the XUNDL database. For more information, click here.


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
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset23726.


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
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2018CR02      Astrophys.J. 859, 105 (2018)

S.Cristallo, M.La Cognata, C.Massimi, A.Best, S.Palmerini, O.Straniero, O.Trippella, M.Busso, G.F.Ciani, F.Mingrone, L.Piersanti, D.Vescovi

The Importance of the 13C(α, n)16O Reaction in Asymptotic Giant Branch Stars

NUCLEAR REACTIONS 13C(α, n), E not given; analyzed available data; deduced impact of reaction rate variations on variations of the element surface distributions.

doi: 10.3847/1538-4357/aac177
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2426. Data from this article have been entered in the XUNDL database. For more information, click here.


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
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2018LA10      Acta Phys.Pol. B49, 657 (2018)

M.La Cognata

Experimental Studies of Nuclear Reactions of Astrophysical Relevance by Means of the Trojan Horse Method Applied to Resonant Reactions

NUCLEAR REACTIONS 13C(α, n)16O, E(cm)=0.05-1.3 MeV; analyzed, calculated Trojan Horse Method (THM) σ data obtained at two INFN laboratories, Catania and Legnaro; calculated R-matrix astrophysical S-factor using the resonance deduced from Trojan Horse Method (THM) σ of quasi-free scattering 19F(p, α)16O, E(cm)<=300 keV; 19F(d, αn)16O using Half-off-Energy-Shell (HOES) to compare THM σ to the corresponding direct σ.

doi: 10.5506/aphyspolb.49.657
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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
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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
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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
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Data from this article have been entered in the XUNDL database. For more information, click here.


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
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Data from this article have been entered in the XUNDL database. For more information, click here.


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
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset23332. Data from this article have been entered in the XUNDL database. For more information, click here.


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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2434.


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
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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
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD0839.


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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD0837.


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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2437. Data from this article have been entered in the XUNDL database. For more information, click here.


2017TR03      Astrophys.J. 837, 41 (2017)

O.Trippella, M.La Cognata

Concurrent Application of ANC and THM to assess the 13C(α, n)16O Absolute Cross Section at Astrophysical Energies and Possible Consequences for Neutron Production in Low-mass AGB Stars

NUCLEAR REACTIONS 13C(α, n), E(cm)<1 MeV; analyzed available data; deduced σ, S-factors, astrophysical reaction rates, asymptotic normalization coefficients.

doi: 10.3847/1538-4357/aa5eb5
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2359.


2016DE02      Phys.Lett. B 753, 449 (2016)

A.Del Zoppo, M.La Cognata

First time evidence of pronounced plateaus right above the Coulomb barrier in 8Li + 4He fusion

NUCLEAR REACTIONS 4He(8Li, X)12B, E(cm)=0.6-5 MeV; measured reaction products; deduced heavy-ion fusion, near-barrier σ, barrier height, intrinsic width and moment of inertia parameter sets. MINUIT data fitting procedure, comparison with available data.

doi: 10.1016/j.physletb.2015.12.055
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2016LA06      Acta Phys.Pol. B47, 681 (2016)

M.La Cognata, C.Spitaleri, S.Cherubini, M.Gulino, O.Trippella, A.Tumino

Using the Trojan Horse Method to Investigate Resonances Above and Below the Threshold in Nuclear Reactions of Astrophysical Interest

NUCLEAR REACTIONS 13C, 19F(α, n), E(cm)<1 MeV; calculated S-factors. R-matrix, Trojan horse method (THM) resonance parameters.

doi: 10.5506/APhysPolB.47.681
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2016LO02      J.Phys.(London) G43, 045109 (2016)

I.Lombardo, D.Dell'Aquila, F.Conte, L.Francalanza, M.La Cognata, L.Lamia, R.La Torre, G.Spadaccini, C.Spitaleri, M.Vigilante

New investigations of the 10B(p, α0)7Be reaction at bombarding energies between 0.6 and 1 MeV

NUCLEAR REACTIONS 10B(p, α)7Be, E=0.6-1 MeV; measured reaction products, Ep, Ip. 11C; deduced σ(θ), S-factor, energy levels, J, π. Comparison with available data.

doi: 10.1088/0954-3899/43/4/045109
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2317. Data from this article have been entered in the XUNDL database. For more information, click here.


2016MA82      Nuovo Cim. C 39, 360 (2016)

C.Matei, D.L.Balabanski, O.Tesileanu, Y.Xu, M.La Cognata, C.Spitaleri

Nuclear astrophysics measurements with ELISSA at ELI-NP

NUCLEAR REACTIONS 3H(α, γ), E(cm)<9 MeV; Calculated S-factor. Comparison with available data.

doi: 10.1393/ncc/i2016-16360-4
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2214. Data from this article have been entered in the XUNDL database. For more information, click here.


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
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2016WE02      Phys.Rev. C 93, 035803 (2016); Pub Note Phys.Rev. C 93, 039902 (2016)

Q.-G.Wen, C.-B.Li, S.-H.Zhou, B.Irgaziev, Y.-Y.Fu, C.Spitaleri, M.La Cognata, J.Zhou, Q.-Y.Meng, L.Lamia, M.Lattuada

Experimental study to explore the 8Be-induced nuclear reaction via the Trojan horse method

NUCLEAR REACTIONS 9Be(d, nα)6Li, E=22.4 MeV; measured α and 6Li spectra, Eα versus θα plots at HI-13 accelerator of CIAE-Beijing; deduced experimental neutron momentum distribution inside 9Be. Deuterated polyethylene target CD2. Trojan horse method for a 3-body reaction with assumption of 9Be as 8Be+n cluster structure. Comparison with theoretical calculations treating 8Be-n interaction with a Woods-Saxon potential.

doi: 10.1103/PhysRevC.93.035803
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetE2506. Data from this article have been entered in the XUNDL database. For more information, click here.


2015FI10      Eur.Phys.J. A 51, 185 (2015)

D.Filipescu, A.Anzalone, D.L.Balabanski, S.S.Belyshev, F.Camera, M.La Cognata, P.Constantin, L.Csige, P.V.Cuong, M.Cwiok, V.Derya, W.Dominik, M.Gai, S.Gales, I.Gheorghe, B.S.Ishkhanov, A.Krasznahorkay, A.A.Kuznetsov, C.Mazzocchi, V.N.Orlin, N.Pietralla, M.Sin, C.Spitaleri, K.A.Stopani, O.Tesileanu, C.A.Ur, I.Ursu, H.Utsunomiya, V.V.Varlamov, H.R.Weller, N.V.Zamfir, A.Zilges

Perspectives for photonuclear research at the Extreme Light Infrastructure - Nuclear Physics (ELI-NP) facility

doi: 10.1140/epja/i2015-15185-9
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2015GR03      Phys.Rev. C 91, 014601 (2015)

J.Grineviciute, L.Lamia, A.M.Mukhamedzhanov, C.Spitaleri, M.La Cognata

Low-energy R-matrix fits for the 6Li (d, α) 4He S factor

NUCLEAR REACTIONS 6Li(d, α)4He, E(cm)=0.01-1.1 MeV; analyzed 2+ subthreshold resonance energy, partial width of the α+α channel, bare astrophysical S(E) factor by single-, two-, and three-level R-matrix fits to the experimental data; deduced electron screening potential. Indirect Trojan horse method.

doi: 10.1103/PhysRevC.91.014601
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2015LA12      Astrophys.J. 805, 128 (2015)

M.La Cognata, S.Palmerini, C.Spitaleri, I.Indelicato, A.M.Mukhamedzhanov, I.Lombardo, O.Trippella

Updated THM astrophysical factor of the 19F(p, α)16O reaction and direct data at astrophysical energies

NUCLEAR REACTIONS 19F(p, α)16O, E(cm)=600-800 keV; analyzed available data; deduced renormalized data, form factor. Trojan Horse Method (THM).

doi: 10.1088/0004-637X/805/2/128
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2015LO07      Phys.Lett. B 748, 178 (2015)

I.Lombardo, D.Dell Aquila, A.Di Leva, I.Indelicato, M.La Cognata, M.La Commara, A.Ordine, V.Rigato, M.Romoli, E.Rosato, G.Spadaccini, C.Spitaleri, A.Tumino, M.Vigilante

Toward a reassessment of the 19F(p, α0)16O reaction rate at astrophysical temperatures

NUCLEAR REACTIONS 19F(p, α), E(cm)=0.2-0.6 MeV; measured reaction products, Eα, Iα; deduced σ(θ), S-factor. Comparison with available data.

doi: 10.1016/j.physletb.2015.06.073
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2278. Data from this article have been entered in the XUNDL database. For more information, click here.


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
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Data from this article have been entered in the XUNDL database. For more information, click here.


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
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1765. Data from this article have been entered in the XUNDL database. For more information, click here.


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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD0651.


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
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2013FI08      Phys.Rev. C 88, 011303 (2013)

M.Fisichella, A.Musumarra, F.Farinon, C.Nociforo, A.Del Zoppo, P.Figuera, M.La Cognata, M.G.Pellegriti, V.Scuderi, D.Torresi, E.Strano

Determination of the half-life of 213Fr with high precision

RADIOACTIVITY 213Fr(α)[from 208Pb(11B, 6n), E=72 MeV]; measured Eα, half-life using the life-time experiment (LITE) facility at INFN-LNS. 211At, 211Po(α); observed α lines. Discussed electron screening effects on decay probability. Comparison with previous measurements.

doi: 10.1103/PhysRevC.88.011303
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Data from this article have been entered in the XUNDL database. For more information, click here.


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
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2147.


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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2146.


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
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetE2369. Data from this article have been entered in the XUNDL database. For more information, click here.


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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1973.


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
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2012LA20      Phys.Scr. T150, 014019 (2012)

M.La Cognata, A.Del Zoppo

Role of exotic cluster structures in astrophysics: the case of 8Li(α, n)11B

NUCLEAR REACTIONS 8Li(α, n)11B, E(cm)=0.3-2 MeV; analyzed experimental data; deduced σ, branching, reaction rates ratios. Cluster structures.

doi: 10.1088/0031-8949/2012/T150/014019
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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
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Data from this article have been entered in the XUNDL database. For more information, click here.


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
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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
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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
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1961. Data from this article have been entered in the XUNDL database. For more information, click here.


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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD0674.


2011MU03      Phys.Rev. C 83, 044604 (2011)

A.M.Mukhamedzhanov, M.La Cognata, V.Kroha

Astrophysical S factor for the 15N( p, γ )16O reaction

NUCLEAR REACTIONS 15N(p, γ), E=0-1.7 MeV; analyzed Notre Dame-LUNA experimental data; deduced astrophysical S factors and resonance parameters, widths using R-matrix approach.

doi: 10.1103/PhysRevC.83.044604
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD0649. Data from this article have been entered in the XUNDL database. For more information, click here.


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
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD0651.


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
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset23158. Data from this article have been entered in the XUNDL database. For more information, click here.


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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1660.


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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1973.


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
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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
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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
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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
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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
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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
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1864. Data from this article have been entered in the XUNDL database. For more information, click here.


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
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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
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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
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2009LA13      Phys.Rev. C 80, 012801 (2009)

M.La Cognata, V.Z.Goldberg, A.M.Mukhamedzhanov, C.Spitaleri, R.E.Tribble

Improved determination of the astrophysical S(0) factor of the 15N(p, α)12C reaction

NUCLEAR REACTIONS 15N(p, α)12C, E(cm)<0.8 MeV; analyzed experimental data; deduced astrophysical S factors and effect of finite energy resolution on S-factors using R-matrix fits to experimental and Trojan Horse data.

doi: 10.1103/PhysRevC.80.012801
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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
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