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NSR database version of April 11, 2024.

Search: Author = T.Szucs

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2024TO01      Nucl.Phys. A1041, 122778 (2024)

A.Toth, Gy.Gyurky, E.Papp, T.Szucs

Experimental 7Be production cross section from the 7Li(p, n)7Be reaction at Ep = 3.5 - 13 MeV

NUCLEAR REACTIONS 7Li(p, n), E=3.5-13 MeV; measured reaction products, Eγ, Iγ; deduced σ and uncertainties. Comparison with available data. The MGC-20 cyclotron accelerator of Atomki.

doi: 10.1016/j.nuclphysa.2023.122778
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2023CS01      Nucl.Phys. A1037, 122705 (2023)

L.Csedreki, Gy.Gurky, T.Szucs

Precise resonance parameter measurement in the 12C(p, γ)13N astrophysically important reaction

NUCLEAR REACTIONS 12C(p, γ), E=0.460, 1.7 MeV; measured reaction products, Eγ, Iγ; deduced yields, resonances, resonance parameters using a simplified R-matrix model. Comparison with available data. 2.0 MV Medium-Current Plus Tandetron Accelerator at Atomki, Debrecen, Hungary.

doi: 10.1016/j.nuclphysa.2023.122705
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Data from this article have been entered in the XUNDL database. For more information, click here.


2023GY01      Phys.Rev. C 107, 025803 (2023)

Gy.Gyurky, P.Mohr, A.Angyal, Z.Halasz, G.G.Kiss, Zs.Matyus, T.N.Szegedi, T.Szucs, Zs.Fulop

Cross section measurement of the 144Sm(α, n)147Gd reaction for studying the α-nucleus optical potential at astrophysical energies

NUCLEAR REACTIONS 144Sm(α, n)147Gd, E=13-20 MeV; measured Eγ Iγ; deduced total σ(E), astrophysical S-factor, constraints on α-nucleus potential. 144Sm(α, X), E=7.5-20 MeV; analyzed experimental information on σ, deduced contribution of different channels to the σ and S-factor. 144Sm(α, γ), E=10-13 MeV; calculated S-factor, astrophysical reaction rate using derived optical model parameters. Activation method. Comparison with statistical model calculations, other experimental data and data from REACLIB AND STARLIB. Targets were irradiated at K20 cyclotron accelerator of Atomki and γ-rays from decay was measured by thin HPGe (LEPS).

doi: 10.1103/PhysRevC.107.025803
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2023GY02      Eur.Phys.J. A 59, 59 (2023)

G.Gyurky, L.Csedreki, T.Szucs, G.G.Kiss, Z.Halasz, Zs.Fulop

Cross section measurement of the 12C(p, γ)13N reaction with activation in a wide energy range

NUCLEAR REACTIONS 12C(p, γ), E=300-1900 keV; measured reaction products, Eγ, Iγ; deduced σ, resonances. Comparison with R-matrix calculation based on the AZURE2 computer code. The Tandetron accelerator of Atomki.

doi: 10.1140/epja/s10050-023-00974-0
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2023SK01      J.Phys.(London) G50, 045201 (2023)

J.Skowronski, R.M.Gesue, A.Boeltzig, G.F.Ciani, D.Piatti, D.Rapagnani, M.Aliotta, C.Ananna, F.Barile, D.Bemmerer, A.Best, C.Broggini, C.G.Bruno, A.Caciolli, M.Campostrini, F.Cavanna, P.Colombetti, A.Compagnucci, P.Corvisiero, L.Csedreki, T.Davinson, R.Depalo, A.Di Leva, Z.Elekes, F.Ferraro, A.Formicola, Z.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, G.Gyurky, G.Imbriani, M.Junker, M.Lugaro, P.Marigo, E.Masha, R.Menegazzo, V.Paticchio, R.Perrino, P.Prati, V.Rigato, L.Schiavulli, R.S.Sidhu, O.Straniero, T.Szucs, S.Zavatarelli

Advances in radiative capture studies at LUNA with a segmented BGO detector

NUCLEAR REACTIONS 12,13C, 14N, 17O, 25Mg(p, γ), 13C(α, n), E ∼ 200 keV; measured reaction products, Eγ, Iγ; deduced yields, resonance parameters, a high-efficiency detection of shorter-lived nuclides. A BGO summing detector at LUNA.

doi: 10.1088/1361-6471/acb961
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Data from this article have been entered in the XUNDL database. For more information, click here.


2023SK02      Phys.Rev. C 107, L062801 (2023)

J.Skowronski, E.Masha, D.Piatti, M.Aliotta, H.Babu, D.Bemmerer, A.Boeltzig, R.Depalo, A.Caciolli, F.Cavanna, L.Csedreki, Z.Fulop, G.Imbriani, D.Rapagnani, S.Rummler, K.Schmidt, R.S.Sidhu, T.Szucs, S.Turkat, A.Yadav

Improved S factor of the 12C(p, γ)13N reaction at E=320-620 keV and the 422 keV resonance

NUCLEAR REACTIONS 12C(p, γ)13N, E=350-670 keV; measured Eγ, Iγ, γ(θ); deduced resonance energy, resonance γ- and p-width, S-factor, astrophysical reaction rate (T=0.01-10 GK). R-matrix analysis. Relevance to HCNO nucleosynthesis.Comparison to other experimental data. Gammas detected by HPGe cluster detector. Molecular H2+ beam from 5MV Pelletron accelerator of Felsenkeller Laboratory

doi: 10.1103/PhysRevC.107.L062801
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2023TO07      Phys.Rev. C 108, 025802 (2023)

A.Toth, T.Szucs, T.N.Szegedi, Gy.Gyurky, Z.Halasz, G.G.Kiss, Zs.Fulop

Experimental determination of the 3He(α, γ)7Be reaction cross section above the 7Be proton separation threshold

NUCLEAR REACTIONS 3He(α, γ)7Be, E=11-20 Mev; measured Eγ, Iγ; deduced σ(E), possible resonance. Activation technique. R-matrix analysis. No prominent structures are observed around known 7Be level, but overall structure of the cross-section suggest a broad resonance peaking around E*=7.5 MeV of 7Be excitation energy. Comparison to previous experimental data obtained with different methods and to the data obtained for mirror reaction 3H(α, γ)7Li. Thin-window gas-cell target irradiated at the Atomki MGC-20 cyclotron. Activated target measured with HPGe detector.

doi: 10.1103/PhysRevC.108.025802
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2022GY01      Phys.Rev. C 105, L022801 (2022)

Gy.Gyurky, Z.Halasz, G.G.Kiss, T.Szucs, Zs.Fulop

Activation cross section measurement of the 14(p, γ)15O astrophysical key reaction

NUCLEAR REACTIONS 14N(p, γ), E=600-1500 keV; measured Eγ, Iγ; deduced σ(E), astrophysical S-factor. Activation method. Comparison with other experimental results.

doi: 10.1103/PhysRevC.105.L022801
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4423.


2022KI15      Phys.Rev. C 106, 015802 (2022)

G.G.Kiss, P.Mohr, Gy.Gyurky, T.Szucs, L.Csedreki, Z.Halasz, Zs.Fulop, E.Somorjai

High-precision 144Sm (α, α) 144Sm scattering at low energies and the rate of the 144Sm (α, γ) 148Gd reaction

NUCLEAR REACTIONS 144Sm(α, α), E=16.13, 18.07, 19.87 MeV; measured Eα, Iα, angular distribution; deduced σ(θ) normalized to Rutherford cross section, parameters of the optical potentials. 144Sm(α, X), 144Sm(α, γ), E(cm)=5-20 MeV; deduced σ(E), astrophysical S-factor using derived α-OMP parameters. Comparison to other experimental data and calculations performed with different OMP parameters. Array of 7 ion-implanted silicon detectors at cyclotron laboratory of ATOMKI, Debrecen.

doi: 10.1103/PhysRevC.106.015802
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2022PI05      Eur.Phys.J. A 58, 194 (2022)

D.Piatti, E.Masha, M.Aliotta, J.Balibrea-Correa, F.Barile, D.Bemmerer, A.Best, A.Boeltzig, C.Broggini, C.G.Bruno, A.Caciolli, F.Cavanna, T.Chillery, G.F.Ciani, A.Compagnucci, P.Corvisiero, L.Csedreki, T.Davinson, R.Depalo, A.di Leva, Z.Elekes, F.Ferraro, E.M.Fiore, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, M.Junker, M.Lugaro, P.Marigo, R.Menegazzo, V.Mossa, F.R.Pantaleo, V.Paticchio, R.Perrino, P.Prati, D.Rapagnani, L.Schiavulli, J.Skowronski, K.Stockel, O.Straniero, T.Szucs, M.P.Takacs, S.Zavatarelli

First direct limit on the 334 keV resonance strength in 22Ne(α, γ)26Mg reaction

NUCLEAR REACTIONS 22Ne(α, γ), E(cm)=334 keV; measured reaction products, Eγ, Iγ; deduced probability density functions of the resonance strength, resonances. Comparison with available data. The Laboratory for Underground Nuclear Astrophysics (LUNA) 400 kV accelerator, located in the deep underground INFN Laboratori Nazionali del Gran Sasso.

doi: 10.1140/epja/s10050-022-00827-2
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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
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2021CS01      Nucl.Instrum.Methods Phys.Res. A994, 165081 (2021)

L.Csedreki, G.F.Ciani, J.Balibrea-Correa, A.Best, M.Aliotta, F.Barile, D.Bemmerer, A.Boeltzig, C.Broggini, C.G.Bruno, A.Caciolli, F.Cavanna, T.Chillery, P.Colombetti, P.Corvisiero, T.Davinson, R.Depalo, A.Di Leva, Z.Elekes, F.Ferraro, E.M.Fiore, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, Z.Janas, M.Junker, I.Kochanek, M.Lugaro, P.Marigo, E.Masha, C.Mazzocchi, R.Menegazzo, V.Mossa, F.R.Pantaleo, V.Paticchio, R.Perrino, D.Piatti, P.Prati, L.Schiavulli, K.Stockel, O.Straniero, T.Szucs, M.P.Takacs, F.Terrasi, S.Zavatarelli

Characterization of the LUNA neutron detector array for the measurement of the 13C(α, n)16O reaction

NUCLEAR REACTIONS 13C(α, n), E=300-400 keV; 51V(p, n), E=5 MeV; measured reaction products, En, In, Eγ, Iγ; deduced yields, neutron efficiencies, possiblity to measure the σ approaching its s-process Gamow peak. Comparison with Geant4 simulations.

doi: 10.1016/j.nima.2021.165081
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2021GY02      J.Phys.(London) G48, 105202 (2021)

G.Gyurky, Z.Halasz, G.G.Kiss, T.Szucs, R.Huszank, Z.Torok, Z.Fulop, T.Rauscher, C.Travaglio

Measurement of the 91Zr(p, γ)92mNb cross section motivated by type Ia supernova nucleosynthesis

NUCLEAR REACTIONS 91,96Zr(p, γ), E=1450-2800 keV; measured reaction products, Eγ, Iγ; deduced σ and uncertainties. Comparison with theoretical calculations.

doi: 10.1088/1361-6471/ac2132
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4417.


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.


2021MO22      At.Data Nucl.Data Tables 142, 101453 (2021)

P.Mohr, Z.Fulop, Gy.Gyurky, G.G.Kiss, T.Szucs, A.Arcones, M.Jacobi, A.Psaltis

Astrophysical reaction rates of α-induced reactions for nuclei with 26 ≤ Z ≤ 83 from the new Atomki-V2 α-nucleus potential

NUCLEAR REACTIONS 88Kr, 188Sm(α, X), E(cm)<15 MeV; calculated astrophysical reaction rates using new Atomki-V2 α-nucleus potential and TALYS nuclear model code.

doi: 10.1016/j.adt.2021.101453
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2021SZ02      Phys.Rev. C 104, 035804 (2021)

T.N.Szegedi, G.G.Kiss, P.Mohr, A.Psaltis, M.Jacobi, G.G.Barnafoldi, T.Szucs, Gy.Gyurky, A.Arcones

Activation thick target yield measurement of 100Mo(α, n)103Ru for studying the weak r-process nucleosynthesis

NUCLEAR REACTIONS 100Mo(α, n)103Ru, E=7.0-13.0 MeV; measured Eγ, Iγ, thick target σ(E) by activation technique at the Institute for Nuclear Research (Atomki); deduced recommended astrophysical rate at T9=1.0-5.0, elemental abundances for the MC13 trajectory using α-nucleus optical model potentials (α-OMPs) with Atomki-V2 potential to model the nucleosynthesis scenario. 95,97Ru, 95Tc; observed γ rays in the spectrum.

doi: 10.1103/PhysRevC.104.035804
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4422.


2021TU03      Phys.Rev. C 103, 045805 (2021)

S.Turkat, S.Hammer, E.Masha, S.Akhmadaliev, D.Bemmerer, M.Grieger, T.Hensel, J.Julin, M.Koppitz, F.Ludwig, C.Mockel, S.Reinicke, R.Schwengner, K.Stockel, T.Szucs, L.Wagner, K.Zuber

Measurement of the 2H(p, γ)3He S factor at 265-1094 keV

NUCLEAR REACTIONS 2H(p, γ)3He, E=400-1650 keV from the 3-MV Tandetron accelerator at Dresden; measured Eγ, Iγ using two HPGe detectors, one surrounded by BGO escape-suppression shield; deduced astrophysical S factors at 14 different incident proton energies, corrected for the assumed ab initio angular distributions of γ rays. 2H(p, γ)3He, E=1-1650 keV; analyzed S-factor data from the present experiment together with previous measurements in other energy regions, and compared with theoretical predictions. Relevance to deuterium abundance in big bang nucleosynthesis.

doi: 10.1103/PhysRevC.103.045805
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2556.


2020CI06      Eur.Phys.J. A 56, 75 (2020)

G.F.Ciani, L.Csedreki, J.Balibrea-Correa, A.Best, M.Aliotta, F.Barile, D.Bemmerer, A.Boeltzig, C.Broggini, C.G.Bruno, A.Caciolli, F.Cavanna, T.Chillery, P.Colombetti, P.Corvisiero, T.Davinson, R.Depalo, A.Di Leva, L.Di Paolo, Z.Elekes, F.Ferraro, E.M.Fiore, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, M.Junker, I.Kochanek, M.Lugaro, P.Marigo, E.Masha, R.Menegazzo, V.Mossa, F.R.Pantaleo, V.Paticchio, R.Perrino, D.Piatti, P.Prati, L.Schiavulli, K.Stockel, O.Straniero, T.Szucs, M.P.Takacs, F.Terrasi, D.Trezzi, S.Zavatarelli

A new approach to monitor 13C-targets degradation in situ for 13C(α, n)16O cross-section measurements at LUNA

doi: 10.1140/epja/s10050-020-00077-0
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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.


2020KR12      Phys.Rev. A 102, 042825 (2020)

F.M.Kroger, G.Weber, M.O.Herdrich, J.Glorius, C.Langer, Z.Slavkovska, L.Bott, C.Brandau, B.Bruckner, K.Blaum, X.Chen, S.Dababneh, T.Davinson, P.Erbacher, S.Fiebiger, T.Gassner, K.Gobel, M.Groothuis, A.Gumberidze, Gy.Gyurky, S.Hagmann, C.Hahn, M.Heil, R.Hess, R.Hensch, P.Hillmann, P.-M.Hillenbrand, O.Hinrichs, B.Jurado, T.Kausch, A.Khodaparast, T.Kisselbach, N.Klapper, C.Kozhuharov, D.Kurtulgil, G.Lane, C.Lederer-Woods, M.Lestinsky, S.Litvinov, Yu.A.Litvinov, B.Loher, F.Nolden, N.Petridis, U.Popp, M.Reed, R.Reifarth, M.S.Sanjari, H.Simon, U.Spillmann, M.Steck, J.Stumm, T.Szucs, T.T.Nguyen, A.Taremi Zadeh, B.Thomas, S.Yu.Torilov, H.Tornqvist, C.Trageser, S.Trotsenko, M.Volknandt, M.Weigand, C.Wolf, P.J.Woods, V.P.Shevelko, I.Yu.Tolstikhina, Th.Stohlker

Electron capture of Xe54+ in collisions with H2 molecules in the energy range between 5.5 and 30.9 MeV/u

NUCLEAR REACTIONS H(Xe, X), E=5.5-30.9 MeV/nucleon; measured reaction products, X-rays; deduced X-ray spectra, electron-capture σ. Comparison with available data.

doi: 10.1103/PhysRevA.102.042825
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2020MO23      Phys.Rev.Lett. 124, 252701 (2020)

P.Mohr, Z.Fulop, G.Gyurky, G.G.Kiss, T.Szucs

Successful Prediction of Total α-Induced Reaction Cross Sections at Astrophysically Relevant Sub-Coulomb Energies Using a Novel Approach

NUCLEAR REACTIONS 176W(α, γ), E<200 keV; analyzed available data; deduced astrophysical reaction rates, S-factor.

doi: 10.1103/PhysRevLett.124.252701
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2020SC07      Phys.Rev. C 101, 064303 (2020)

R.Schwengner, R.Massarczyk, R.Beyer, M.Bhike, B.A.Brown, Krishichayan, K.Sieja, W.Tornow, D.Bemmerer, M.Butterling, V.Derya, M.Dietz, F.Fiedler, U.Friman-Gayer, A.Frotscher, M.Grieger, A.Hartmann, A.R.Junghans, T.Kogler, F.Ludwig, B.Lutz, H.Pai, T.Szucs, M.P.Takacs, A.Wagner

Electric and magnetic dipole strength in 54Fe

NUCLEAR REACTIONS 54Fe(polarized γ, γ'), E=4.3-13.0 MeV; measured Eγ, Iγ, γ(θ), γ(polarization asymmetry), and integrated scattering cross sections, absolute photoabsorption σ(E) using HPGe detectors at the γELBE facility of the Helmholtz-Zentrum Dresden-Rossendorf (HZDR), and at the HIγS facility at TUNL. 54Fe; deduced levels, J, π, B(E1), B(M1). Comparison with shell-model predictions.

doi: 10.1103/PhysRevC.101.064303
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetL0262. Data from this article have been entered in the XUNDL database. For more information, click here.


2020WI09      Phys.Rev. C 102, 044327 (2020)

J.Wilhelmy, M.Muscher, G.Rusev, R.Schwengner, R.Beyer, M.Bhike, P.Erbacher, F.Fiedler, U.Friman-Gayer, J.Glorius, R.Greifenhagen, S.Hammer, T.Hensel, J.Isaak, A.R.Junghans, Krishichayan, B.Loher, S.E.Muller, N.Pietralla, S.Reinicke, D.Savran, P.Scholz, K.Sonnabend, T.Szucs, M.Tamkas, W.Tornow, S.Turkat, A.Wagner, A.Zilges

Dipole response of 87Rb and its impact on the 86Rb (n, γ) 87Rb cross section

NUCLEAR REACTIONS 87Rb(γ, γ'), E=8.2, 13.2 MeV bremsstrahlung beam; measured Eγ, Iγ, γ(θ) using four HPGe detectors at the γ-ELBE facility in Dresden. 87Rb(polarized γ, γ'), E=5.10, 5.30, 5.50, 5.75, 6.00, 6.25, 6.50, 6.75, 7.00, 7.25, 7.50, 7.80, 8.10, 8.40, 8.70, 9.00, 9.30, 9.60 MeV; measured Eγ, Iγ, azimuthal asymmetry using four LaBr3:Ce scintillators and four HPGe detectors at the HIγS facility of TUNL; deduced energy-integrated σ(excitation energy), γ-ray sum spectra, photoabsorption σ(E), E1-photon strength functions (PSFs), nuclear level densities (NLDs), Thomas-Reiche-Kuhn (TRK) sum rule. Comparison with QRPA calculations for PSFs, and microscopic Hartree-Fock-Bogolyubov calculations with Skyrme and Gogny forces for NLDs. 87Rb; deduced 256 discrete levels from 845 to 10005 keV, J, π, gΓ02/Γ, γ-ray branching ratios for selected levels, as listed in supplemental material. 86Rb(n, γ), kT=5-100 keV; deduced Maxwellian cross sections (MACSs) for different PSF and NLD inputs, and compared to data in KADoNiS database.

doi: 10.1103/PhysRevC.102.044327
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetL0266.


2019BE31      Phys.Lett. B 797, 134900 (2019)

A.Best, F.R.Pantaleo, A.Boeltzig, G.Imbriani, M.Aliotta, J.Balibrea-Correa, D.Bemmerer, C.Broggini, C.G.Bruno, R.Buompane, A.Caciolli, F.Cavanna, T.Chillery, G.F.Ciani, P.Corvisiero, L.Csedreki, T.Davinson, R.J.deBoer, R.Depalo, A.Di Leva, Z.Elekes, F.Ferraro, E.M.Fiore, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, M.Junker, I.Kochanek, M.Lugaro, P.Marigo, R.Menegazzo, V.Mossa, V.Paticchio, R.Perrino, D.Piatti, P.Prati, L.Schiavulli, K.Stockel, O.Straniero, F.Strieder, T.Szucs, M.P.Takacs, D.Trezzi, M.Wiescher, S.Zavatarelli

Cross section of the reaction 18O(p, γ)19F at astrophysical energies: The 90 keV resonance and the direct capture component

NUCLEAR REACTIONS 18O(p, γ), E<1 MeV; measured reaction products, Eγ, Iγ; deduced γ-ray energies, resonance parameters, σ. Comparison with available data.

doi: 10.1016/j.physletb.2019.134900
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2457. Data from this article have been entered in the XUNDL database. For more information, click here.


2019BO09      Phys.Lett. B 795, 122 (2019)

A.Boeltzig, A.Best, F.R.Pantaleo, G.Imbriani, M.Junker, M.Aliotta, J.Balibrea-Correa, D.Bemmerer, C.Broggini, C.G.Bruno, R.Buompane, A.Caciolli, F.Cavanna, T.Chillery, G.F.Ciani, P.Corvisiero, L.Csedreki, T.Davinson, R.J.deBoer, R.Depalo, A.Di Leva, Z.Elekes, F.Ferraro, E.M.Fiore, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, I.Kochanek, M.Lugaro, P.Marigo, R.Menegazzo, V.Mossa, F.Munnik, V.Paticchio, R.Perrino, D.Piatti, P.Prati, L.Schiavulli, K.Stockel, O.Straniero, F.Strieder, T.Szucs, M.P.Takacs, D.Trezzi, M.Wiescher, S.Zavatarelli

Direct measurements of low-energy resonance strengths of the 23Na(p, γ)24Mg reaction for astrophysics

NUCLEAR REACTIONS 23Na(p, γ), E<1 MeV; measured reaction products, Eγ, Iγ; deduced resonance parameters, strengths, astrophysical reaction rates. Comparison with available data.

doi: 10.1016/j.physletb.2019.05.044
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2520. Data from this article have been entered in the XUNDL database. For more information, click here.


2019BR07      Phys.Lett. B 790, 237 (2019)

C.G.Bruno, M.Aliotta, P.Descouvemont, A.Best, T.Davinson, D.Bemmerer, A.Boeltzig, C.Broggini, A.Caciolli, F.Cavanna, T.Chillery, G.F.Ciani, P.Corvisiero, R.Depalo, A.Di Leva, Z.Elekes, F.Ferraro, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, M.Junker, M.Lugaro, P.Marigo, R.Menegazzo, V.Mossa, F.R.Pantaleo, D.Piatti, P.Prati, K.Stockel, O.Straniero, F.Strieder, T.Szucs, M.P.Takacs, D.Trezzi

Improved astrophysical rate for the 18O(p, α)15N reaction by underground measurements

NUCLEAR REACTIONS 18O(p, α)15N, E=60-360 keV; measured reaction products, Ep, Ip, Eα, Iα; deduced differential yield, resonance energies, S-factor, J, π, reaction rates.

doi: 10.1016/j.physletb.2019.01.017
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2019GL01      Phys.Rev.Lett. 122, 092701 (2019)

J.Glorius, C.Langer, Z.Slavkovska, L.Bott, C.Brandau, B.Bruckner, K.Blaum, X.Chen, S.Dababneh, T.Davinson, P.Erbacher, S.Fiebiger, T.Gassner, K.Gobel, M.Groothuis, A.Gumberidze, G.Gyurky, M.Heil, R.Hess, R.Hensch, P.Hillmann, P.-M.Hillenbrand, O.Hinrichs, B.Jurado, T.Kausch, A.Khodaparast, T.Kisselbach, N.Klapper, C.Kozhuharov, D.Kurtulgil, G.Lane, C.Lederer-Woods, M.Lestinsky, S.Litvinov, Y.A.Litvinov, B.Loher, F.Nolden, N.Petridis, U.Popp, T.Rauscher, M.Reed, R.Reifarth, M.S.Sanjari, D.Savran, H.Simon, U.Spillmann, M.Steck, T.Stohlker, J.Stumm, A.Surzhykov, T.Szucs, T.T.Nguyen, A.Taremi Zadeh, B.Thomas, S.Yu.Torilov, H.Tornqvist, M.Trager, C.Trageser, S.Trotsenko, L.Varga, M.Volknandt, H.Weick, M.Weigand, C.Wolf, P.J.Woods, Y.M.Xing

Approaching the Gamow Window with Stored Ions: Direct Measurement of 124Xe(p, γ) in the ESR Storage Ring

NUCLEAR REACTIONS 124Xe(p, γ), E=5.5-8 MeV/nucleon; measured reaction products, X-rays; deduced σ, σ(θ).

doi: 10.1103/PhysRevLett.122.092701
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2443.


2019GY04      Appl.Radiat.Isot. 148, 87 (2019)

G.Gyurky, Z.Halasz, G.G.Kiss, T.Szucs, Z.Fulop

Half-life measurement of 65Ga with γ-spectroscopy

RADIOACTIVITY 65Ga(EC) [from 64Zn(p, γ), E=4.5, 6 MeV]; 61Cu(EC) [from 64Zn(p, α), E=4.5, 6 MeV]; measured decay products, Eγ, Iγ; deduced γ-ray energies, intensities, T1/2.

doi: 10.1016/j.apradiso.2019.03.021
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Data from this article have been entered in the XUNDL database. For more information, click here.


2019GY05      Phys.Rev. C 100, 015805 (2019)

Gy.Gyurky, Z.Halasz, G.G.Kiss, T.Szucs, A.Csik, Zs.Torok, R.Huszank, M.G.Kohan, L.Wagner, Zs.Fulop

Resonance strengths in the 14N(p, γ)15O astrophysical key reaction measured with activation

NUCLEAR REACTIONS 14N(p, γ)15O, E=278, 1058 keV; measured Eγ, Iγ, resonance strengths using activation method at the Institute for Nuclear Research, Debrecen. Comparison with previous experimental values. Discussion of relevance to stellar hydrogen burning.

doi: 10.1103/PhysRevC.100.015805
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2019PI05      Phys.Rev. C 99, 024601 (2019)

E.Pirovano, R.Beyer, M.Dietz, A.R.Junghans, S.E.Muller, R.Nolte, M.Nyman, A.J.M.Plompen, M.Roder, T.Szucs, M.P.Takacs

Cross section and neutron angular distribution measurements of neutron scattering on natural iron

NUCLEAR REACTIONS Fe(n, n), (n, n'), E=2-6 MeV; measured E(n), I(n), time of flight, neutron angular distributions, differential σ(θ, E), and σ(E) using liquid organic scintillator array for neutron detection at GELINA and nELBE facilities. 56Fe(n, n'), E=2-6 MeV; measured differential σ(θ, E) for the first excited state of 56Fe. Comparison with previous experimental results, and ENDF/B-VIII evaluation; compiled a list of previous experiments for Fe(n, n), 56Fe(n, n'), E=2-6 MeV retrieved from the EXFOR database.

doi: 10.1103/PhysRevC.99.024601
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset23365.


2019SZ01      Nucl.Phys. A986, 213 (2019)

T.N.Szegedi, G.G.Kiss, I.Oksuz, T.Szucs, Gy.Gyurky, Z.Elekes, E.Somorjai, Zs.Fulop

High precision half-life measurement of 125Cs and 125Xe with γ-spectroscopy

NUCLEAR REACTIONS 124Xe(p, γ)125Cs, E=6-7.5 MeV; measured off-line activation Eγ, Iγ(t) following the β-decay; deduced T1/2. Compared with published results.

doi: 10.1016/j.nuclphysa.2019.04.002
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2019SZ02      Phys.Rev. C 99, 055804 (2019), Erratum Phys.Rev. C 105, 069901 (2022)

T.Szucs, G.G.Kiss, Gy.Gyurky, Z.Halasz, T.N.Szegedi, Zs.Fulop

Cross section of 3He(α, γ)7Be around the 7Be proton separation threshold

NUCLEAR REACTIONS 3He(α, γ)7Be, E=7.3-11.35 MeV; measured Eγ, Iγ, Eα, σ(E) using HPGe detector for offline γ spectroscopy. 3He(α, γ)7Be, E(cm)=0.2-5.0 MeV; analyzed data using constrained R-matrix fit; deduced S factors, asymptotic nuclear coefficients (ANCs), and upper limit on α-capture resonance strength using data from present experiment and previous experiments. Relevance to Big Bang nucleosynthesis and solar hydrogen burning.

doi: 10.1103/PhysRevC.99.055804
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4400.


2019SZ03      Eur.Phys.J. A 55, 174 (2019)

T.Szucs, D.Bemmerer, D.Degering, A.Domula, M.Grieger, F.Ludwig, K.Schmidt, J.Steckling, S.Turkat, K.Zuber

Background in γ-ray detectors and carbon beam tests in the Felsenkeller shallow-underground accelerator laboratory

doi: 10.1140/epja/i2019-12865-4
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2019SZ04      Phys.Rev. C 100, 065803 (2019)

T.Szucs, P.Mohr, Gy.Gyurky, Z.Halasz, R.Huszank, G.G.Kiss, T.N.Szegedi, Zs.Torok, Zs.Fulop

Cross section of α-induced reactions on 197Au at sub-Coulomb energies

NUCLEAR REACTIONS 197Au(α, 2n)199Tl, E=17.48, 17.99, 18.49, 18.99, 19.46, 19.92 MeV; 197Au(α, n)200Tl, E=13.62, 13.91, 14.92, 15.91, 16.96, 17.48, 17.99, 18.49, 18.99, 19.46, 19.92 MeV; 197Au(α, γ)201Tl, E=13.91, 14.92, 15.91, 16.96, 17.48, 17.99, 18.99, 19.46, 19.92 MeV; measured Eγ, Iγ, E(x ray), I(x ray), σ(E) by activation method at the MTA Atomki cyclotron in Debrecen; deduced Absolute x-ray intensities from the decays of 199,200,201Tl. 197Au(α, α'), E=24.7 MeV; measured σ(θ) and total σ. Comparison to the best fit statistical model calculation using the AVR A-OMP, and with previous experimental results. Prediction of cross sections in the Gamow window with smaller uncertainties. Relevance to determination of reaction rates in large-scale reaction networks for heavy-element nucleosynthesis.

doi: 10.1103/PhysRevC.100.065803
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4406.


2018BE07      Eur.Phys.J. A 54, 58 (2018)

R.Beyer, M.Dietz, D.Bemmerer, A.R.Junghans, T.Kogler, R.Massarczyk, S.Muller, K.Schmidt, R.Schwengner, T.Szucs, M.P.Takacs, A.Wagner

The γ-ray angular distribution in fast neutron inelastic scattering from iron

NUCLEAR REACTIONS 54,56Fe(n, n'), E=0.1-10 MeV; measured Eγ, Iγ(θ) of the four lowest excited states of 56Fe and on of 54Fe using five FPGe and five LaBr3 scintillators; deduced σ(θ), σ; compared with other data and data libraries; calculated Legendre polynomial coefficients fitting σ(θ) data.

doi: 10.1140/epja/i2018-12492-7
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset23411.


2018BE17      Europhys.Lett. 122, 52001 (2018)

D.Bemmerer, F.Cavanna, R.Depalo, M.Aliotta, M.Anders, A.Boeltzig, C.Broggini, C.Bruno, A.Caciolli, T.Chillery, P.Corvisiero, T.Davinson, Z.Elekes, F.Ferraro, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, R.Menegazzo, V.Mossa, F.R.Pantaleo, P.Prati, D.A.Scott, K.Stocker, O.Straniero, T.Szucs, M.P.Takacs, D.Trezzi

Effect of beam energy straggling on resonant yield in thin gas targets: The cases 22Ne(p, γ)23Na and 14N(p, γ)15O

NUCLEAR REACTIONS 22Ne, 14N(p, γ), E<300 keV; analyzed available data; deduced correction for narrow resonance yields.

doi: 10.1209/0295-5075/122/52001
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2018BE21      Eur.Phys.J. A 54, 81 (2018)

R.Beyer, A.R.Junghans, P.Schillebeeckx, I.Sirakov, T.-Y.Song, D.Bemmerer, R.Capote, A.Ferrari, A.Hartmann, R.Hannaske, J.Heyse, H.I.Kim, J.W.Kim, T.Kogler, C.W.Lee, Yo.-O.Lee, R.Massarczyk, S.E.Muller, T.P.Reinhardt, M.Roder, K.Schmidt, R.Schwengner, T.Szucs, M.P.Takacs, A.Wagner, L.Wagner, S.-C.Yang

The neutron transmission of natFe, 197Au and natW

NUCLEAR REACTIONS 197Au, W(n, x), E=0.025-0.17 MeV; calculated transmission correction factor using MCNP. Fe, 197Au, W(n, x), E=0.15-8 MeV; measured reaction products using nELBE neutron ToF; deduced σ. Compared with other data (in a wider energy interval) and published calculations using optical model.

doi: 10.1140/epja/i2018-12505-7
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset23415.


2018KI04      Phys.Rev. C 97, 055803 (2018)

G.G.Kiss, T.Szucs, P.Mohr, Zs.Torok, R.Huszank, Gy.Gyurky, Zs.Fulop

α-induced reactions on 115In: Cross section measurements and statistical model analysis

NUCLEAR REACTIONS 115In(α, γ), (α, n)118mSb, E(cm)=8.83-15.58 MeV; 115In(α, n)118Sb, E(cm)=11.10-15.58 MeV; measured Eγ, Iγ, and corrected peak rates of α-irradiated targets, reaction σ(E) using a HPGe detector for γ detection and a low-energy photon spectrometer (LEPS) for x-ray detection at Atomki, Debrecen; deduced reaction σ best fit parameters, σ at energies corresponding to the Gamow window at 2 and 3 GK. Applied best fit parameters to α+113In reaction σ. Comparison with statistical model calculations using TALYS code, and with previous experimental values.

doi: 10.1103/PhysRevC.97.055803
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4385.


2018KO12      Phys.Rev. C 97, 045803 (2018)

Z.Korkulu, N.Ozkan, G.G.Kiss, T.Szucs, Gy.Gyurky, Zs.Fulop, R.T.Guray, Z.Halasz, T.Rauscher, E.Somorjai, Zs.Torok, C.Yalcin

Investigation of α-induced reactions on Sb isotopes relevant to the astrophysical γ process

NUCLEAR REACTIONS 121,123Sn(α, n), 121Sn(α, γ), E=10.09-16 MeV; measured Eγ, Iγ from decay of reaction products, σ(E) by activation method at the MGC cyclotron accelerator of Atomki-Debrecen; deduced sensitivity of σ to variation of particle and radiative widths for 121Sn+α reactions. Comparison with previous experimental values, and with statistical model calculations using NON-SMOKER and SMARAGD codes. Discussed implications for astrophysical reaction rates in γ-process nucleosynthesis network.

doi: 10.1103/PhysRevC.97.045803
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4393.


2018SZ01      Phys.Lett. B 776, 396 (2018)

T.Szucs, G.G.Kiss, Gy.Gyurky, Z.Halasz, Zs.Fulop, T.Rauscher

Cross section of α-induced reactions on iridium isotopes obtained from thick target yield measurement for the astrophysical γ process

NUCLEAR REACTIONS 191,193Ir(α, γ), (α, n), E=13.4, 17 MeV; measured reaction products, Eγ, Iγ; deduced thick target yields, σ. Comparison with statistical-model calculations performed with the SMARAGD code.

doi: 10.1016/j.physletb.2017.11.072
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4386.


2018WA03      Phys.Rev. C 97, 015801 (2018)

L.Wagner, S.Akhmadaliev, M.Anders, D.Bemmerer, A.Caciolli, St.Gohl, M.Grieger, A.Junghans, M.Marta, F.Munnik, T.P.Reinhardt, S.Reinicke, M.Roder, K.Schmidt, R.Schwengner, M.Serfling, M.P.Takacs, T.Szucs, A.Vomiero, A.Wagner, K.Zuber

Astrophysical S factor of the 14N(p, γ)150 reaction at 0.4-1.3 MeV

NUCLEAR REACTIONS 14N(p, γ), E=4001400 keV from tandem accelerator at Helmholtz-Zentrum Dresden-Rossendorf (HZDR); measured Eγ, Iγ, γ(θ), σ(E), resonance yields. 15O; deduced levels, proton-resonances, astrophysical S factors. R-matrix analysis. Comparison with previous experimental results.

doi: 10.1103/PhysRevC.97.015801
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2439.


2017GY01      Phys.Rev. C 95, 035805 (2017)

Gy.Gyurky, A.Ornelas, Zs.Fulop, Z.Halasz, G.G.Kiss, T.Szucs, R.Huszank, I.Hornyak, I.Rajta, I.Vajda

Cross section measurement of the astrophysically important 17O(p, γ)18F reaction in a wide energy range

NUCLEAR REACTIONS 17O(p, γ)18F, E=500-1800 keV; measured Eγ, Iγ, half-life of 18F decay, σ(E) by activation method using Van de Graaff accelerator of Atomki; analyzed using R-matrix fit; deduced S factors. Comparison with previous experimental data. Relevance to hydrogen burning processes in different stages of stellar evolution.

doi: 10.1103/PhysRevC.95.035805
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4367.


2017TR01      Astropart.Phys. 89, 57 (2017)

D.Trezzi, M.Anders, M.Aliotta, A.Bellini, D.Bemmerer, A.Boeltzig, C.Broggini, C.G.Bruno, A.Caciolli, F.Cavanna, P.Corvisiero, H.Costantini, T.Davinson, R.Depalo, Z.Elekes, M.Erhard, F.Ferraro, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, M.Junker, A.Lemut, M.Marta, C.Mazzocchi, R.Menegazzo, V.Mossa, F.Pantaleo, P.Prati, C.Rossi Alvarez, D.A.Scott, E.Somorjai, O.Straniero, T.Szucs, M.Takacs

Big Bang 6Li nucleosynthesis studied deep underground (LUNA collaboration)

NUCLEAR REACTIONS 2H(α, γ), E(cm)=80, 93, 120, 133 keV; measured reaction products, Eγ, Iγ; deduced σ, S-factor, thermonuclear reaction rates. Comparison with available data.

doi: 10.1016/j.astropartphys.2017.01.007
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2016BE14      Eur.Phys.J. A 52, 72 (2016)

A.Best, A.Caciolli, Zs.Fulop, Gy.Gyurky, M.Laubenstein, E.Napolitani, V.Rigato, V.Roca, T.Szucs

Underground nuclear astrophysics: Why and how

doi: 10.1140/epja/i2016-16072-7
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2016DE34      Phys.Rev. C 94, 055804 (2016)

R.Depalo, F.Cavanna, M.Aliotta, M.Anders, D.Bemmerer, A.Best, A.Boeltzig, C.Broggini, C.G.Bruno, A.Caciolli, G.F.Ciani, P.Corvisiero, T.Davinson, A.Di Leva, Z.Elekes, F.Ferraro, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, M.Junker, R.Menegazzo, V.Mossa, F.R.Pantaleo, D.Piatti, P.Prati, O.Straniero, T.Szucs, M.P.Takacs, D.Trezzi

Direct measurement of low-energy 22Ne(p, γ)23Na resonances

NUCLEAR REACTIONS 22Ne(p, γ), E=70-300 keV; measured Eγ, Iγ, γγ-coin at the LUNA 400 kV accelerator, deep underground at the Gran Sasso National Laboratories (LNGS). 23Na; deduced levels, resonance energies and strengths, J, π, thermonuclear reaction rates. Comparison with previous experimental data.

doi: 10.1103/PhysRevC.94.055804
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2324. Data from this article have been entered in the XUNDL database. For more information, click here.


2016HA33      Phys.Rev. C 94, 045801 (2016)

Z.Halasz, E.Somorjai, Gy.Gyurky, Z.Elekes, Zs.Fulop, T.Szucs, G.G.Kiss, N.T.Szegedi, T.Rauscher, J.Gorres, M.Wiescher

Experimental study of the astrophysical γ-process reaction 124Xe(α, γ)128Ba

NUCLEAR REACTIONS 124Xe(α, γ)128Ba, 124Xe(α, n)127Ba, E=11-15 MeV; measured Eγ, Iγ, σ(E) by activation method using a thin window gas cell. Comparison with Hauser-Feshbach statistical model calculations, 124Xe+α optical potential, astrophysical gamma-process, and supernova models.

doi: 10.1103/PhysRevC.94.045801
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4365.


2016OR09      Phys.Rev. C 94, 055807 (2016)

A.Ornelas, P.Mohr, Gy.Gyurky, Z.Elekes, Zs.Fulop, Z.Halasz, G.G.Kiss, E.Somorjai, T.Szucs, M.P.Takacs, D.Galaviz, R.T.Guray, Z.Korkulu, N.Ozkan, C.Yalcin

alpha scattering and alpha-induced reaction cross sections of 64Zn at low energies

NUCLEAR REACTIONS 64Zn(α, α), (α, α'), E=12.05, 16.12 MeV; measured scattered particle spectra, Eα, Iα, elastic σ(θ), inelastic σ(E) at the Atomki cyclotron facility; deduced total σ, parameters of optical potential, phase shifts and reflection coefficients using σ(θ) elastic data at Eα=13.4-50.5 MeV from previous studies and the present work, rise of the elastic cross sections at very backward angles considered as so-called anomalous large-angle elastic scattering (ALAS). 64Zn(α, γ), (α, p), (α, n), E=16.12 MeV; measured Eγ, Iγ, σ using activation technique. Comparison with theoretical calculations based on different global α-nucleus optical potentials, and Hartree-Fock BCS γ-ray strength for (α, γ) channel.

doi: 10.1103/PhysRevC.94.055807
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4366.


2015BR09      Eur.Phys.J. A 51, 94 (2015)

C.G.Bruno, D.A.Scott, A.Formicola, M.Aliotta, T.Davinson, M.Anders, A.Best, D.Bemmerer, C.Broggini, A.Caciolli, F.Cavanna, P.Corvisiero, R.Depalo, A.Di Leva, Z.Elekes, Zs.Fulop, G.Gervino, C.J.Griffin, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, M.Junker, R.Menegazzo, E.Napolitani, P.Prati, E.Somorjai, O.Straniero, F.Strieder, T.Szucs, D.Trezzi, for the LUNA Collaboration

Resonance strengths in the 17, 18O(p, α)14, 15N reactions and background suppression underground - Commissioning of a new setup for charged-particle detection at LUNA

NUCLEAR REACTIONS 17,18O(p, α), E=151, 193 keV; measured Eα, Iα; deduced resonance strength, energy, thick target yield as a by-product of commissioning of new setup.

doi: 10.1140/epja/i2015-15094-y
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2275. Data from this article have been entered in the XUNDL database. For more information, click here.


2015CA27      Phys.Rev.Lett. 115, 252501 (2015); Erratum Phys.Rev.Lett. 120, 239901 (2018)

F.Cavanna, R.Depalo, M.Aliotta, M.Anders, D.Bemmerer, A.Best, A.Boeltzig, C.Broggini, C.G.Bruno, A.Caciolli, P.Corvisiero, T.Davinson, A.di Leva, Z.Elekes, F.Ferraro, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, M.Junker, R.Menegazzo, V.Mossa, F.R.Pantaleo, P.Prati, D.A.Scott, E.Somorjai, O.Straniero, F.Strieder, T.Szucs, M.P.Takacs, D.Trezzi, for the LUNA Collaboration

Three New Low-Energy Resonances in the 22Ne(p, γ)23Na Reaction

NUCLEAR REACTIONS 20,21,22Ne(p, γ), E=70-300 keV; measured reaction products, Eγ, Iγ; deduced resonance energies and strengths, thermonuclear reaction rates. Comparison with available data.

doi: 10.1103/PhysRevLett.115.252501
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4330. Data from this article have been entered in the XUNDL database. For more information, click here.


2015KI04      J.Phys.(London) G42, 055103 (2015)

G.G.Kiss, T.Szucs, T.Rauscher, Zs.Torok, L.Csedreki, Z.Fulop, G.Gyurky, Z.Halasz

Measurement of (α, n) reaction cross sections of erbium isotopes for testing astrophysical rate predictions

NUCLEAR REACTIONS 162Er(α, n), (α, γ), E<17 MeV; analyzed available data; deduced optical potential, theoretical σ. Comparison of statistical model predictions with experimental data.

doi: 10.1088/0954-3899/42/5/055103
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4341.


2015ME07      Phys.Rev. C 92, 035803 (2015)

B.Mei, T.Aumann, S.Bishop, K.Blaum, K.Boretzky, F.Bosch, C.Brandau, H.Brauning, T.Davinson, I.Dillmann, C.Dimopoulou, O.Ershova, Z.Fulop, H.Geissel, J.Glorius, G.Gyurky, M.Heil, F.Kappeler, A.Kelic-Heil, C.Kozhuharov, C.Langer, T.Le Bleis, Y.Litvinov, G.Lotay, J.Marganiec, G.Munzenberg, F.Nolden, N.Petridis, R.Plag, U.Popp, G.Rastrepina, R.Reifarth, B.Riese, C.Rigollet, C.Scheidenberger, H.Simon, K.Sonnabend, M.Steck, T.Stohlker, T.Szucs, K.Summerer, G.Weber, H.Weick, D.Winters, N.Winters, P.Woods, Q.Zhong

First measurement of the 96Ru(p, γ)97Rh cross section for the p process with a storage ring

NUCLEAR REACTIONS 1H(96Ru, γ)97Rh, E=9, 10, 11 MeV/nucleon; measured particle spectra in different charge states, x-ray and γ spectra, σ(E) using stored heavy ions in storage ring ESR at GSI; deduced astrophysical S factors and stellar reaction rates over a range of T9=0.5-19. Comparison with predictions from standard NON-SMOKER code and TALYS-1.4 code using different γ-ray strength functions from HFB, Brink-Axel Lorentzian (BAL), and Kopecky-Uhl, and different density models of constant temperature (CT), BSFG, generalized superfluid (GS), and Hartree-Fock-Bogolyubov (HFB). Recommended REACLIB parameters for the reactivity of 96Ru(p, γ)97Rh, and 97Rh(γ, p)96Ru reactions. Relevance to p-process network calculations.

doi: 10.1103/PhysRevC.92.035803
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2272.


2015SZ01      Eur.Phys.J. A 51, 33 (2015)

T.Szucs, D.Bemmerer, T.P.Reinhardt, K.Schmidt, M.P.Takacs, A.Wagner, L.Wagner, D.Weinberger, K.Zube

Cosmic-ray-induced background intercomparison with actively shielded HPGe detectors at underground locations

doi: 10.1140/epja/i2015-15033-0
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2015SZ02      Phys.Rev. C 92, 014315 (2015)

T.Szucs, D.Bemmerer, A.Caciolli, Zs.Fulop, R.Massarczyk, C.Michelagnoli, T.P.Reinhardt, R.Schwengner, M.P.Takacs, C.A.Ur, A.Wagner, L.Wagner

Determination of γ-ray widths in 15N using nuclear resonance fluorescence

NUCLEAR REACTIONS 11B, 15N(γ, γ'), E<12.6 MeV; measured Eγ, Iγ, γ(θ), integrated scattering cross sections using NRF technique at superconducting electron accelerator ELBE-HZDR. 11B, 15N; deduced levels, J, π, multipolarities, mixing ratios, γ branching ratios, partial gamma widths to the ground state, resonance strengths of 527-and 634-keV proton resonances, and proton reduced width of 10.804-MeV level in 15N. Comparison with previous experimental data.

doi: 10.1103/PhysRevC.92.014315
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Data from this article have been entered in the XUNDL database. For more information, click here.


2015SZ03      Phys.Rev. C 92, 044328 (2015)

T.Szucs, P.Mohr

Addendum to "Determination of γ-ray widths in 15N using nuclear resonance fluorescence"

NUCLEAR REACTIONS 15N(γ, γ'), E<12.6 MeV; analyzed experimental data in authors' previous work 2015Sz02, resonance strengths from 14C(p, γ)15N, and γ-ray branching ratios; deduced levels, J, π, absolute widths Γp, Γγ, Γγ, 0, and Γ of 3/2 levels at 10702 and 10804 keV. Comparison with evaluated data in ENSDF.

doi: 10.1103/PhysRevC.92.044328
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Data from this article have been entered in the XUNDL database. For more information, click here.


2015TA27      Phys.Rev. D 91, 123526 (2015)

M.P.Takacs, D.Bemmerer, T.Szucs, K.Zuber

Constraining big bang lithium production with recent solar neutrino data

doi: 10.1103/PhysRevD.91.123526
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4331.


2015TA28      Phys.Rev. D 91, 123526 (2015)

M.P.Takacs, D.Bemmerer, T.Szucs, K.Zuber

Constraining big bang lithium production with recent solar neutrino data

NUCLEAR REACTIONS 3He(α, γ), E=0.0 eV-1 GeV; measured products, 7Be, Eγ, Iγ; deduced σ, σ(E). Data were imported from EXFOR entry D4331.

doi: 10.1103/PhysRevD.91.123526
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2015YA07      Phys.Rev. C 91, 034610 (2015)

C.Yalcin, Gy.Gyurky, T.Rauscher, G.G.Kiss, N.Ozkan, R.T.Guray, Z.Halasz, T.Szucs, Zs.Fulop, J.Farkas, Z.Korkulu, E.Somorjai

Test of statistical model cross section calculations for α-induced reactions on 107Ag at energies of astrophysical interest

NUCLEAR REACTIONS 107Ag(α, γ)111In, E=8.16-13 MeV; 107Ag(α, n)110In, E=9-13 MeV; measured Eγ, Iγ, σ(E) by activation method. Comparison with statistical model calculation using SMARAGD computer code, and with previous experimental results.

doi: 10.1103/PhysRevC.91.034610
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4328.


2014AN05      Phys.Rev.Lett. 113, 042501 (2014)

M.Anders, D.Trezzi, R.Menegazzo, M.Aliotta, A.Bellini, D.Bemmerer, C.Broggini, A.Caciolli, P.Corvisiero, H.Costantini, T.Davinson, Z.Elekes, M.Erhard, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, M.Junker, A.Lemut, M.Marta, C.Mazzocchi, P.Prati, C.Rossi Alvarez, D.A.Scott, E.Somorjai, O.Straniero, T.Szucs, for the LUNA Collaboration

First Direct Measurement of the 2H(α, γ)6Li Cross Section at Big Bang Energies and the Primordial Lithium Problem

NUCLEAR REACTIONS 2H(α, γ), E=400 keV; measured reaction products, Eγ, Iγ; deduced S-factor, σ. Comparison with available data.

doi: 10.1103/PhysRevLett.113.042501
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2188.


2014CA47      Eur.Phys.J. A 50, 179 (2014)

F.Cavanna, R.Depalo, M.-L.Menzel, M.Aliotta, M.Anders, D.Bemmerer, C.Broggini, C.G.Bruno, A.Caciolli, P.Corvisiero, T.Davinson, A.di Leva, Z.Elekes, F.Ferraro, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, M.Junker, R.Menegazzo, P.Prati, C.Rossi Alvarez, D.A.Scott, E.Somorjai, O.Straniero, F.Strieder, T.Szucs, D.Trezzi, for the LUNA Collaboration

A new study of the 22Ne(p, γ)23Na reaction deep underground: Feasibility, setup and first observation of the 186 keV resonance

NUCLEAR REACTIONS 22Ne(p, γ), E=120-400 keV; measured Eγ, Iγ at LUNA. 23Na deduced γ transitions, 186 keV resonance.

doi: 10.1140/epja/i2014-14179-5
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2237. Data from this article have been entered in the XUNDL database. For more information, click here.


2014DI01      Phys.Rev. C 89, 015803 (2014), Erratum Phys.Rev. C 90, 019902 (2014)

A.Di Leva, D.A.Scott, A.Caciolli, A.Formicola, F.Strieder, M.Aliotta, M.Anders, D.Bemmerer, C.Broggini, P.Corvisiero, Z.Elekes, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, J.Jose, M.Junker, M.Laubenstein, R.Menegazzo, E.Napolitani, P.Prati, V.Rigato, V.Roca, E.Somorjai, C.Salvo, O.Straniero, T.Szucs, F.Terrasi, D.Trezzi

Underground study of the 17O(p, γ)18F reaction relevant for explosive hydrogen burning

NUCLEAR REACTIONS 17O(p, γ)18F, E(cm)=160-370 keV; measured Eγ, Iγ, on- and off-resonance γ spectra, γ-branching ratios from decay of resonances, half-life using activation method at underground LUNA accelerator at Gran Sasso National Laboratory; deduced S factors for secondary transitions, total S factor, resonance strength, astrophysical S factor and reaction rates. 18F; deduced levels, analysis of astrophysically important 183-keV resonance. Comparison with previous experimental results. 15N, 18,19F, 18O; evaluated abundances by Nova model calculations.

RADIOACTIVITY 18F(β+)[from 17O(p, γ), E(cm)=160-370 keV]; measured Eγ, Iγ, half-life.

doi: 10.1103/PhysRevC.89.015803
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2098. Data from this article have been entered in the XUNDL database. For more information, click here.


2014DI07      Nucl.Data Sheets 120, 171 (2014)

I.Dillmann, T.Szucs, R.Plag, Z.Fulop, F.Kappeler, A.Mengoni, T.Rauscher

The Karlsruhe Astrophysical Database of Nucleosynthesis in Stars Project - Status and Prospects

COMPILATION A=1-210; compiled astrophysical σ for s-, p-, and γ-processes. Comparison with theoretical calculations.

doi: 10.1016/j.nds.2014.07.038
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2014FO06      Nucl.Instrum.Methods Phys.Res. A742, 258 (2014)

A.Formicola, C.G.Bruno, A.Caciolli, F.Cavanna, R.Depalo, A.Di Leva, D.A.Scott, D.Trezzi, M.Aliotta, M.Anders, D.Bemmerer, C.Broggini, P.Corvisiero, Z.Elekes, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, M.Junker, R.Menegazzo, P.Prati, E.Somorjai, O.Straniero, F.Strieder, T.Szucs

Cross-section measurements at astrophysically relevant energies: The LUNA experiment

NUCLEAR REACTIONS 17O(p, γ), E(cm)=183 keV; measured reaction products, Eγ, Iγ; deduced σ, resonance strength, S-factor. Comparison with available data.

doi: 10.1016/j.nima.2013.11.082
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2014GY01      Nucl.Phys. A922, 112 (2014)

Gy.Gyurky, M.Vakulenko, Zs.Fulop, Z.Halasz, G.G.Kiss, E.Somorjai, T.Szucs

Cross section and reaction rate of 92Mo(p, γ)93Tc determined from thick target yield measurements

NUCLEAR REACTIONS 92Mo(p, γ), E=1700-3100 keV; measured thick target Eγ, Iγ(time). 93g,93mTc deduced peaks, thick target yields, σ, S-factor, thermonuclear reaction rates, T1/2; calculated σ, S-factor using TALYS. Compared also with some other recent data.

doi: 10.1016/j.nuclphysa.2013.12.003
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4312.


2014GY02      Phys.Rev. C 90, 052801 (2014)

G.Gyurky, Z.Fulop, Z.Halasz, G.G.Kiss, T.Szucs

Direct study of the α-nucleus optical potential at astrophysical energies using the 64Zn(p, α)61Cu reaction

NUCLEAR REACTIONS 64Zn(p, α)61Cu, 64Zn(p, γ)65Ga, E=3.5-8 MeV; measured Eγ, Iγ, σ(E) by activation method; deduced experimental S factors and Gamow window for 61Cu+α system. Comparison with statistical model calculations using NON-SMOKER, TALYS and TALYS-modified with 61Cu+α optical potential. Astrophysical γ process.

doi: 10.1103/PhysRevC.90.052801
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4319.


2014KI05      Phys.Lett. B 735, 40 (2014)

G.G.Kiss, T.Szucs, T.Rauscher, Zs.Torok, Zs.Fulop, Gy.Gyurky, Z.Halasz, E.Somorjai

Alpha induced reaction cross section measurements on 162Er for the astrophysical γ process

NUCLEAR REACTIONS 162Er(α, γ), (α, n), E(cm)=12.19-16.09 MeV; measured reaction products, Eγ, Iγ, X-rays; deduced σ, needs for optical potential modifications. Comparison with Hauser-Feshbach calculations.

doi: 10.1016/j.physletb.2014.06.011
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4318.


2014SZ03      Nucl.Data Sheets 120, 191 (2014)

T.Szucs, I.Dillmann, R.Plag, Zs.Fulop

KADoNiS-p: The Astrophysical p-Process Database

COMPILATION A=1-140; compiled astrophysical σ for p-process. TALYS theoretical calculations.

doi: 10.1016/j.nds.2014.07.043
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2013AN07      Eur.Phys.J. A 49, 28 (2013)

M.Anders, D.Trezzi, A.Bellini, M.Aliotta, D.Bemmerer, C.Broggini, A.Caciolli, H.Costantini, P.Corvisiero, T.Davinson, Z.Elekes, M.Erhard, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, M.Junker, A.Lemut, M.Marta, C.Mazzocchi, R.Menegazzo, P.Prati, C.Rossi Alvarez, D.Scott, E.Somorjai, O.Straniero, T.Szucs, LUNA Collaboration

Neutron-induced background by an α-beam incident on a deuterium gas target and its implications for the study of the 2H(α, γ)6Li reaction at LUNA

NUCLEAR REACTIONS 2H(α, γ), E=280, 400 keV; measured Eγ, Iγ; deduced yields vs Eγ, existence of cosmological 6Li plateau.

doi: 10.1140/epja/i2013-13028-5
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2013BO09      Nucl.Phys. A908, 1 (2013)

C.Bordeanu, Gy.Gyurky, Z.Halasz, T.Szucs, G.G.Kiss, Z.Elekes, J.Farkas, Zs.Fulop, E.Somorjai

Activation measurement of the 3He(α, γ)7Be reaction cross section at high energies

NUCLEAR REACTIONS 3He(α, γ), E=4.0-6.3 MeV; measured off-line 7Be activation Eγ, Iγ; deduced σ, S-factor. Compared with data and published calculations.

doi: 10.1016/j.nuclphysa.2013.03.012
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4289.


2013KI11      Phys.Rev. C 88, 045804 (2013)

G.G.Kiss, P.Mohr, Zs.Fulop, T.Rauscher, Gy.Gyurky, T.Szucs, Z.Halasz, E.Somorjai, A.Ornelas, C.Yalcin, R.T.Guray, N.Ozkan

High precision 113In(α, α)113In elastic scattering at energies near the Coulomb barrier for the astrophysical γ process

NUCLEAR REACTIONS 113In(α, α), E=16.15-19.15 MeV; measured E(α), I(α), σ(E, θ) at ATOMKI facility in Debrecen; deduced global α+nucleus optical model parameters. Comparison with reduced σ for 89Y+α, 92Mo+α, 106,110,116Cd+α, 112,124Sn+α and 144Sm+α reactions. 113In(α, γ)117Sb, 113In(α, n)116Sb, E=8-15 MeV; deduced astrophysical S(E) factor, σ ratio. Relevance to γ process for production of p nuclei in supernova explosions.

doi: 10.1103/PhysRevC.88.045804
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4297.


2013NE16      Nucl.Phys. A916, 149 (2013)

L.Netterdon, P.Demetriou, J.Endres, U.Giesen, G.G.Kiss, A.Sauerwein, T.Szucs, K.O.Zell, A.Zilges

Investigation of α-induced reactions on the p nucleus 168Yb

NUCLEAR REACTIONS 168Yb(α, γ), (α, n), E=12.9-15.1 MeV; measured activation and post-β-decay Eγ, Iγ using HPGe; calculated σ using TALYS-1.4 code with RIPL3 parameters. 171,172Hf deduced (α, γ) and (α, n) σ 171Lu deduced normalization factor.

doi: 10.1016/j.nuclphysa.2013.08.002
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2178. Data from this article have been entered in the XUNDL database. For more information, click here.


2013SC16      Phys.Rev. C 88, 025803 (2013)

K.Schmidt, S.Akhmadaliev, M.Anders, D.Bemmerer, K.Boretzky, A.Caciolli, D.Degering, M.Dietz, R.Dressler, Z.Elekes, Z.Fulop, G.Gyurky, R.Hannaske, A.R.Junghans, M.Marta, M.-L.Menzel, F.Munnik, D.Schumann, R.Schwengner, T.Szucs, A.Wagner, D.Yakorev, K.Zuber

Resonance triplet at Ea=4.5 MeV in the 40Ca(α, γ)44Ti reaction

NUCLEAR REACTIONS 40Ca(α, γ), E=4.5 MeV; measured Eγ, Iγ, yields. 44Ti; deduced levels, triplet of resonances near 4.5 MeV, resonance strengths, γ-decay branching ratios, α widths, astrophysical reaction rates. Comparison with previous data. Target composition determined by elastic recoil detection (ERD) method and by nuclear reactions.

doi: 10.1103/PhysRevC.88.025803
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2161. Data from this article have been entered in the XUNDL database. For more information, click here.


2012GY01      Appl.Radiat.Isot. 70, 278 (2012)

Gy.Gyurky, J.Farkas, Z.Halasz, T.Szucs

Half-life measurement of 66Ga with γ-spectroscopy

RADIOACTIVITY 66Ga(EC) [from 66Zn(p, n), E=11.3 MeV]; measured decay products, Eγ, Iγ; deduced T1/2 and uncertainties.

doi: 10.1016/j.apradiso.2011.08.004
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2012GY02      J.Phys.:Conf.Ser. 337, 012009 (2012)

Gy.Gyurky, J.Farkas, Z.Halasz, Zs.Fulop, E.Somorjai, T.Szucs, P.Mohr, A.Wallner

Experimental study of α-induced reactions on 64Zn for the astrophysical γ-process

NUCLEAR REACTIONS 64Zn(α, n), (α, p), (α, γ), (α, α), E=4-8.8 MeV; measured Eγ, Iγ; deduced (α, p) σ using activation method; calculated (α, p) σ using NON-SMOKER and TALYS.

doi: 10.1088/1742-6596/337/1/012009
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4274.


2012GY03      Phys.Rev. C 86, 041601 (2012)

Gy.Gyurky, P.Mohr, Zs.Fulop, Z.Halasz, G.G.Kiss, T.Szucs, E.Somorjai

Relation between total cross sections from elastic scattering and α-induced reactions: The example of 64Zn

NUCLEAR REACTIONS 64Zn(α, γ), (α, p), (α, n), E(cm)=5.8-12.4 MeV; measured Eγ, Iγ, σ(E); deduced total reaction σ by comparison with σ for 64Zn(α, α) reaction, astrophysical S factor. Comparison with statistical model predictions.

doi: 10.1103/PhysRevC.86.041601
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4274.


2012HA07      Phys.Rev. C 85, 025804 (2012)

Z.Halasz, Gy.Gyurky, J.Farkas, Zs.Fulop, T.Szucs, E.Somorjai, T.Rauscher

Investigation of α-induced reactions on 130Ba and 132Ba and their importance for the synthesis of heavy p nuclei

NUCLEAR REACTIONS 130Ba(α, γ)134Ce, E=12.0-16.5 MeV; 130Ba(α, n)133Ce, 132Ba(α, n)135Ce, E=12.5-16.5 MeV; measured Eγ, Iγ, cross sections, isomeric and total cross sections for 133Ce by activation method. 130Ba(α, γ)134Ce, 132Ba(α, γ)136Ce, 134Ce(γ, α)130Ba, 136Ce(γ, α)132Ba, T9=2-10; deduced astrophysical (stellar) reaction rates. Comparison with prediction of statistical model calculations using NONSMOKER, SMARAGD, and TALYS computer codes.

doi: 10.1103/PhysRevC.85.025804
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4271.


2012HA36      J.Phys.:Conf.Ser. 337, 012063 (2012)

Z.Halasz, J.Farkas, Zs.Fulop, Gy.Gyurky, E.Somorjai, T.Szucs, M.P.Takacs

Towards in-beam (α, γ) cross section measurements for the astrophysical γ-process

NUCLEAR REACTIONS 116Sn(α, γ), E=10.7 MeV; measured in-beam Eγ, Iγ. Very preliminary.

doi: 10.1088/1742-6596/337/1/012063
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2012KI14      Phys.Rev. C 86, 035801 (2012)

G.G.Kiss, T.Szucs, Zs.Torok, Z.Korkulu, Gy.Gyurky, Z.Halasz, Zs.Fulop, E.Somorjai, T.Rauscher

Investigation of α-induced reactions on 127I for the astrophysical γ process

NUCLEAR REACTIONS 127I(α, γ), (α, n)130Cs/131Cs, E(cm)=9.50-15.15 MeV; measured Eγ, Iγ, x rays, σ(E) using activation method; deduced astrophysical S factor, stellar reaction rates. Comparison with Hauser-Feshbach statistical model calculations. Relevance to origin of the neutron-deficient p nuclides.

RADIOACTIVITY 130Cs(EC); measured precise Iγ of 536.1-keV transition.

doi: 10.1103/PhysRevC.86.035801
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4273.


2012RA16      Phys.Rev. C 86, 015804 (2012)

T.Rauscher, G.G.Kiss, T.Szucs, Zs.Fulop, C.Frohlich, Gy.Gyurky, Z.Halasz, Zs.Kertesz, E.Somorjai

Astrophysical analysis of the measurement of (α, γ) and (α, n) cross sections of 169Tm

NUCLEAR REACTIONS 169Tm(α, γ)173Lu, E=12.6-17.5 MeV; 169Tm(α, n)172Lu, E=11.5-17.5 MeV; measured x-ray spectra, yields using LEPS detector, σ; deduced astrophysical S factors as function of energy, reaction rates. Comparison with global α+nucleus potentials calculations using statistical model computer code SMARAGD.

doi: 10.1103/PhysRevC.86.015804
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4272.


2012SZ02      Eur.Phys.J. A 48, 8 (2012)

T.Szucs, D.Bemmerer, T.Cowan, D.Degering, Z.Elekes, Z.Fulop, G.Gyurky, A.Junghans, M.Kohler, M.Marta, R.Schwengner, A.Wagner, K.Zuber

Shallow-underground accelerator sites for nuclear astrophysics: Is the background low enough?

doi: 10.1140/epja/i2012-12008-7
Citations: PlumX Metrics


2012SZ03      J.Phys.:Conf.Ser. 337, 012032 (2012)

T.Szucs, D.Bemmerer, T.Cowan, K.Zuber

A possible underground accelerator in the Dresden Felsenkeller

doi: 10.1088/1742-6596/337/1/012032
Citations: PlumX Metrics


2012SZ04      J.Phys.:Conf.Ser. 337, 012033 (2012)

T.Szucs, I.Dillmann, R.Plag, Zs.Fulop

The KADoNiS databases - progress and future plans

doi: 10.1088/1742-6596/337/1/012033
Citations: PlumX Metrics


2011FA01      Eur.Phys.J. A 47, 7 (2011)

J.Farkas, Gy.Gyurky, Z.Halasz, T.Szucs, Zs.Fulop, E.Somorjai

Half-life measurement of 133mCe with γ-spectrometry

NUCLEAR REACTIONS 130Ba(α, n)133mCe, E=14, 14.5, 15, 15.5 MeV; measured Eγ, Iγ(t) using activation technique. 133mCe deduced T1/2.

doi: 10.1140/epja/i2011-11007-6
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Data from this article have been entered in the XUNDL database. For more information, click here.


2011KI01      Phys.Lett. B 695, 419 (2011)

G.G.Kiss, T.Rauscher, T.Szucs, Zs.Kertesz, Zs.Fulop, Gy.Gyurky, C.Frohlich, J.Farkas, Z.Elekes, E.Somorjai

Determining reaction cross sections via characteristic X-ray detection: α-induced reactions on 169Tm for the astrophysical γ-process

NUCLEAR REACTIONS 169Tm(α, γ), (α, n), E=11.5-17.5 MeV; measured Eγ, Iγ, x-rays; deduced yield, σ, S-factors. Comparison with theoretical calculations.

doi: 10.1016/j.physletb.2010.11.052
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4244.


2011KI21      Nucl.Phys. A867, 52 (2011)

G.G.Kiss, T.Szucs, Gy.Gyurky, Zs.Fulop, J.Farkas, Zs.Kertesz, E.Somorjai, M.Laubenstein, C.Frohlich, T.Rauscher

Activation method combined with characteristic X-ray counting: A possibility to measure (α, γ) cross sections on heavy p-nuclei

NUCLEAR REACTIONS 169Tm(α, γ), (α, n), E=11.5-17.5 MeV; measured Eγ, Iγ, X-rays using HPGe and LEPS detectors; deduced σ using activation method.

doi: 10.1016/j.nuclphysa.2011.07.003
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4248.


2010GY02      J.Phys.(London) G37, 115201 (2010)

Gy.Gyurky, Z.Elekes, J.Farkas, Zs.Fulop, Z.Halasz, G.G.Kiss, E.Somorjai, T.Szucs, R.T.Guray, N.Ozkan, C.Yalcin, T.Rauscher

Alpha-induced reaction cross section measurements on 151Eu for the astrophysical γ-process

NUCLEAR REACTIONS 151Eu(α, γ), (α, n), E=11.5-17.5 MeV; measured Eγ, Iγ; deduced T1/2, σ, S-factors, using activation method. Statistical model calculations using NON-SMOKER model. Relevance to astrophysical γ process.

doi: 10.1088/0954-3899/37/11/115201
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4241.


2010GY03      J.Phys.:Conf.Ser. 202, 012004 (2010)

Gy.Gyurky, Z.Elekes, J.Farkas, Z.S.Fulop, G.G.Kiss, E.Somorjai, T.Szucs, R.T.Guray, N.Ozkan, C.Yalcin, T.Rauscher

Alpha-induced reactions for the astrophysical p-process: The case of 151Eu

NUCLEAR REACTIONS 151Eu(α, γ), (α, n), E=11.5-17.5 MeV; measured Eγ, Iγ; deduced σ, S-factors using activation technique; calculated S-factors using NON-SMOKER code with different α optical model potentials.

doi: 10.1088/1742-6596/202/1/012004
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2010MA26      Phys.Rev. C 81, 055807 (2010)

M.Marta, E.Trompler, D.Bemmerer, R.Beyer, C.Broggini, A.Caciolli, M.Erhard, Z.Fulop, E.Grosse, G.Gyurky, R.Hannaske, A.R.Junghans, R.Menegazzo, C.Nair, R.Schwengner, T.Szucs, S.Vezzu, A.Wagner, D.Yakorev

Resonance strengths in the 14N(p, γ)15O and 15N(p, αγ)12C reactions

NUCLEAR REACTIONS 14N(p, γ)15O, E=278, 1058 keV; 15N(p, α)12C, E=430, 897 keV; measured γ-ray spectra, yield, angular distributions, branching ratio, and resonance strengths. 15O; deduced resonances. Comparison with previous measurements.

doi: 10.1103/PhysRevC.81.055807
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1851. Data from this article have been entered in the XUNDL database. For more information, click here.


2010SZ04      Eur.Phys.J. A 44, 513 (2010)

T.Szucs, D.Bemmerer, C.Broggini, A.Caciolli, F.Confortola, P.Corvisiero, Z.Elekes, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, M.Junker, A.Lemut, M.Marta, C.Mazzocchi, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, C.Rossi Alvarez, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, for the LUNA Collaboration

An actively vetoed Clover γ-detector for nuclear astrophysics at LUNA

NUCLEAR REACTIONS 24Mg(p, γ), E=223 keV; measured Eγ, Iγ. 25Al; deduced levels, J, π, branching ratios.

doi: 10.1140/epja/i2010-10967-1
Citations: PlumX Metrics


2010ZH54      J.Phys.:Conf.Ser. 202, 012011 (2010)

Q.Zhong, T.Aumann, S.Bishop, K.Blaum, K.Boretzky, F.Bosch, H.Brauning, C.Brandau, T.Davinson, I.Dillmann, O.Ershova, H.Geissel, G.Gyurky, M.Heil, F.Kappeler, A.Kelic, C.Kozhuharov, C.Langer, T.Le Bleis, Y.A.Litvinov, G.Lotay, J.Marganiec, N.Petridis, R.Plag, U.Popp, R.Reifarth, B.Riese, C.Rigollet, C.Scheidenberger, H.Simon, T.Stohlker, T.Szucs, G.Weber, H.Weick, D.F.A.Winters, N.Winters, P.J.Woods

96Ru(p, γ)97Rh measurement at the GSI storage ring

NUCLEAR REACTIONS 1H(96Ru, γ), (96Ru, α), (96Ru, n), E=9, 10, 11 MeV/nucleon; measured Rh ions using DSSSD (double sided Si strip detector) mounted in a pocket inside ESR; deduced σ upper limit at 11 MeV/nucleon; calculatedσ using NON-SMOKER. Analysis continues.

doi: 10.1088/1742-6596/202/1/012011
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2009GY01      Nucl.Phys. A828, 1 (2009)

Gy.Gyurky, G.Rastrepina, Z.Elekes, J.Farkas, Zs.Fulop, G.G.Kiss, E.Somorjai, T.Szucs

Precise half-life measurement of the 10 h isomer in 154Tb

RADIOACTIVITY 154Tb(IT), (β+), (EC) [from 151Eu(α, n), E=13.5, 14.5, 15, 15.5, 17 MeV]; measured Eγ, Iγ using HPGe detector; deduced T1/2 of 1st isomeric state.

doi: 10.1016/j.nuclphysa.2009.06.023
Citations: PlumX Metrics

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


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