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NSR database version of April 25, 2024.

Search: Author = G.G.Rapisarda

Found 56 matches.

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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
Citations: PlumX Metrics

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


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics

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


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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


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.


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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.


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
Citations: PlumX Metrics

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


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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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


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
Citations: PlumX Metrics

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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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.


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics

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.


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.


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.


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.


2014JU02      Phys.Rev. C 90, 035805 (2014)

H.S.Jung, C.S.Lee, Y.K.Kwon, J.Y.Moon, J.H.Lee, C.C.Yun, M.J.Kim, T.Hashimoto, H.Yamaguchi, D.Kahl, S.Kubono, Y.Wakabayashi, Y.Togano, S.Choi, Y.H.Kim, Y.K.Kim, J.S.Park, E.J.Kim, C.-B.Moon, T.Teranishi, N.Iwasa, T.Yamada, S.Kato, S.Cherubini, S.Hayakawa, G.G.Rapisarda

Elastic scattering of 25Al + p to explore the resonance structure in 26Si

NUCLEAR REACTIONS 1H(25Al, p), E=71.58 MeV, [25Al secondary beam from 3He(24Mg, 25Al), E=7.5 MeV/nucleon primary reaction]; measured Ep, Ip, ΔE-E and two-dimensional TOF plots, σ(E) at CRIB-RIKEN-CNS facility. 26Si; deduced levels, resonances, J, π, l-values, proton widths using R-matrix analysis. Comparison with previous experimental studies. Discussed astrophysical implications.

doi: 10.1103/PhysRevC.90.035805
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetE2463. Data from this article have been entered in the XUNDL database. For more information, click here.


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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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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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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2012JU01      Phys.Rev. C 85, 045802 (2012)

H.S.Jung, C.S.Lee, Y.K.Kwon, J.Y.Moon, J.H.Lee, C.C.Yun, S.Kubono, H.Yamaguchi, T.Hashimoto, D.Kahl, S.Hayakawa, S.Choi, M.J.Kim, Y.H.Kim, Y.K.Kim, J.S.Park, E.J.Kim, C.-B.Moon, T.Teranishi, Y.Wakabayashi, N.Iwasa, T.Yamada, Y.Togano, S.Kato, S.Cherubini, G.G.Rapisarda

Experimental study of resonant states in 27P via elastic scattering of 26Si+p

NUCLEAR REACTIONS 1H(26Si, p), [26Si beam from 3He(24Mg, X), E=7.5 MeV/nucleon primary reaction], E=132.8 MeV; measured Ep, Ip, time-of-flight. 27P; deduced levels, resonances, J, π, l-value, widths using R-matrix analysis. 26Si(p, γ); deduced reaction rates of astrophysical interest. Comparison with shell-model calculations, and level structure of 27Mg mirror nucleus.

doi: 10.1103/PhysRevC.85.045802
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetE2372. 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.


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.


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.


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


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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1713. Data from this article have been entered in the XUNDL database. For more information, click here.


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
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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
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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
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4208.


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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD0552.


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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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4208.


2007TU04      Nucl.Phys. A787, 337c (2007)

A.Tumino, C.Spitaleri, G.G.Rapisarda, S.Cherubini, S.Blagus, M.Bogovac, V.Crucilla, Z.Elekes, Z.Fulop, M.Gulino, G.Gyurky, G.Kiss, M.La Cognata, L.Lamia, Dj.Miljanic, M.Milin, F.Mudo, A.Mukhamedzhanov, R.G.Pizzone, D.Rendic, S.Romano, M.L.Sergi, E.Somorjai

No signature of nuclear-Coulomb interference in the proton-proton elastic scattering via the Trojan Horse Method

NUCLEAR REACTIONS 2H(p, 2p), E=5, 6 MeV; measured Ep, Ip, σ(E, θ). Plane wave impulse approximation, Trojan horse method.

doi: 10.1016/j.nuclphysa.2006.12.053
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Note: The following list of authors and aliases matches the search parameter G.G.Rapisarda: , G.G.RAPISARDA