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NSR database version of April 27, 2024.

Search: Author = A.Cvetinovic

Found 14 matches.

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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.


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.


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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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.


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.


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.


2015CV01      Appl.Radiat.Isot. 104, 160 (2015)

A.Cvetinovic, A.Likar, M.Lipoglavsek, A.Mihelic, T.Petrovic, J.Vesic, B.Vodenik

Precise measurement of the half-life of 61Cu

RADIOACTIVITY 61Cu(β+), (EC) [from 60Ni(p, γ)]; measured decay products, Eγ, Iγ; deduced T1/2, level energies, J, π. Comparison with theoretical calculations.

doi: 10.1016/j.apradiso.2015.07.005
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Data from this article have been entered in the XUNDL database. For more information, click here.


2015CV02      Phys.Rev. C 92, 065801 (2015)

A.Cvetinovic, M.Lipoglavsek, S.Markelj, J.Vesic

Molecular screening in nuclear reactions

NUCLEAR REACTIONS 1H(7Li, α)4He, E=0.4-2 MeV; 1H(11B, 2α)4He, E=1.79 MeV; 1H(19F, αγ)16O, E=6.47 MeV; measured Eα, Iα, Eγ, Iγ, integrated enhancement factors, γ-ray yields S-factor, resonance strength in different hydrogen-containing targets; deduced electron screening potential.

doi: 10.1103/PhysRevC.92.065801
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2015VE03      Acta Phys.Pol. B46, 467 (2015)

J.Vesic, A.Cvetinovic, T.Petrovic, M.Lipoglavsek

Effect of Electron Screening on Nuclear Reaction Rates

NUCLEAR REACTIONS 2H(p, γ), E=0.24-0.44 MeV; measured reaction products, Eγ, Iγ; deduced σ, lack of sensitivity for the value of the electron screening potential.

doi: 10.5506/APhysPolB.46.467
Citations: PlumX Metrics


2014VE03      Eur.Phys.J. A 50, 153 (2014)

J.Vesic, A.Cvetinovic, M.Lipoglavsek, T.Petrovic

Influence of electronic environment on nuclear reaction rates

NUCLEAR REACTIONS 1H(7Li, α), E=0.34-2.07 MeV; measured reaction products for hydrogen-implanted Ni, Zn, Pt, Pd targets; deduced screening potential, astrophysical S-factor. 55Mn(p, n), (p, γ), E=1500-1595 keV; measured reaction products; deduced thick target γ yield ratio for Mn and MnO targets, neutron number near 1.54 MeV resonance. 115Cd(p, n), E=1560-2600 keV; measured Eγ, Iγ, nγ-coin for Cd and CdO; deduced neutron number per 299 keV γ transition. 51V(p, γ)(p, n), E=700-1600 keV; measured thick target Eγ, Iγ, nγ-coin for V and VO2 targets; deduced ratio of 1434 keV γ yields. 115In(p, n), E=1750-2500 keV; measured neutrons, X-ray, nX-coin for In and In2O3 targets; deduced neutron number per 24 keV X-ray.

doi: 10.1140/epja/i2014-14153-3
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2013GA25      Eur.Phys.J. A 49, 70 (2013)

J.Gajevic, A.Cvetinovic, A.Likar, M.Lipoglavsek, P.Pelicon, T.Petrovic, A.Sanchez Ortiz

Electron screening in nickel

ATOMIC PHYSICS Ni(p, γ), (p, X), E=0.86-3.08 MeV; measured thick target Eγ, Iγ using HPGe, backscattered protons, X-rays from PIXE using SiLi from metallic Ni and NiO; deduced isotope yields, levels, γ transitions, branching ratios, electron screening potential, electron density vs intranuclear distance.

doi: 10.1140/epja/i2013-13070-3
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