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NSR database version of May 24, 2024.

Search: Author = O.Straniero

Found 74 matches.

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2024AM02      Phys.Rev.Lett. 132, 122701 (2024)

S.Amaducci, N.Colonna, L.Cosentino, S.Cristallo, P.Finocchiaro, M.Krticka, C.Massimi, M.Mastromarco, A.Mazzone, E.A.Maugeri, A.Mengoni, I.U.Roederer, O.Straniero, S.Valenta, D.Vescovi, O.Aberle, V.Alcayne, J.Andrzejewski, L.Audouin, V.Babiano-Suarez, M.Bacak, M.Barbagallo, S.Bennett, E.Berthoumieux, J.Billowes, D.Bosnar, A.Brown, M.Busso, M.Caamano, L.Caballero-Ontanaya, F.Calvino, M.Calviani, D.Cano-Ott, A.Casanovas, F.Cerutti, E.Chiaveri, G.Cortes, M.A.Cortes-Giraldo, L.A.Damone, P.J.Davies, M.Diakaki, M.Dietz, C.Domingo-Pardo, R.Dressler, Q.Ducasse, E.Dupont, I.Duran, Z.Eleme, B.Fernandez-Dominguez, A.Ferrari, V.Furman, K.Gobel, R.Garg, A.Gawlik-Ramiega, S.Gilardoni, I.F.Goncalves, E.Gonzalez-Romero, C.Guerrero, F.Gunsing, H.Harada, S.Heinitz, J.Heyse, D.G.Jenkins, A.Junghans, F.Kappeler, Y.Kadi, A.Kimura, I.Knapova, M.Kokkoris, Y.Kopatch, D.Kurtulgil, I.Ladarescu, C.Lederer-Woods, H.Leeb, J.Lerendegui-Marco, S.J.Lonsdale, D.Macina, A.Manna, T.Martinez, A.Masi, P.Mastinu, E.Mendoza, V.Michalopoulou, P.M.Milazzo, F.Mingrone, J.Moreno-Soto, A.Musumarra, A.Negret, R.Nolte, F.Ogallar, A.Oprea, N.Patronis, A.Pavlik, J.Perkowski, C.Petrone, L.Piersanti, E.Pirovano, I.Porras, J.Praena, J.M.Quesada, D.Ramos-Doval, T.Rauscher, R.Reifarth, D.Rochman, C.Rubbia, M.Sabate-Gilarte, A.Saxena, P.Schillebeeckx, D.Schumann, A.Sekhar, A.G.Smith, N.V.Sosnin, P.Sprung, A.Stamatopoulos, G.Tagliente, J.L.Tain, A.Tarifeno-Saldivia, L.Tassan-Got, Th.Thomas, P.Torres-Sanchez, A.Tsinganis, J.Ulrich, S.Urlass, G.Vannini, V.Variale, P.Vaz, A.Ventura, V.Vlachoudis, R.Vlastou, A.Wallner, P.J.Woods, T.Wright, P.Zugec

Measurement of the 140Ce(n, γ) Cross Section at n_TOF and Its Astrophysical Implications for the Chemical Evolution of the Universe

NUCLEAR REACTIONS 140Ce(n, γ), E<200 keV; measured reaction products, En, In, Eγ, Iγ; deduced Maxwellian averaged σ, yields, resonance parameters, impact on galactic abundances. Comparison with ENDF/B-VIII.0, JENDL-5 libraries, R-matrix code SAMMY. The neutron beam time-of-flight facility (n_TOF) at CERN.

doi: 10.1103/PhysRevLett.132.122701
Citations: PlumX Metrics


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.


2023ST02      Eur.Phys.J. A 59, 17 (2023)

O.Straniero, C.Abia, I.Domínguez

The carbon star mystery: 40 years later - Theory and observations

doi: 10.1140/epja/s10050-023-00926-8
Citations: PlumX Metrics


2022AL01      J.Phys.(London) G49, 010501 (2022)

M.Aliotta, R.Buompane, M.Couder, A.Couture, R.J.deBoer, A.Formicola, L.Gialanella, J.Glorius, G.Imbriani, M.Junker, C.Langer, A.Lennarz, Y.A.Litvinov, W.-P.Liu, M.Lugaro, C.Matei, Z.Meisel, L.Piersanti, R.Reifarth, D.Robertson, A.Simon, O.Straniero, A.Tumino, M.Wiescher, Y.Xu

The status and future of direct nuclear reaction measurements for stellar burning

NUCLEAR REACTIONS 12C(α, γ), 22Ne(α, n), (α, γ), 12C(12C, X), E(cm)<7 MeV; analyzed available data; deduced σ, S-factors.

doi: 10.1088/1361-6471/ac2b0f
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


2021VE01      J.Phys.(London) G48, 015201 (2021)

D.Vescovi, C.Mascaretti, F.Vissani, L.Piersanti, O.Straniero

The luminosity constraint in the era of precision solar physics

NUCLEAR REACTIONS 1H, 7Be, 14N(p, X), 3,4He(3He, X), E not given; analyzed available data; calculated evolution of solar abundances, luminosity constraints.

doi: 10.1088/1361-6471/abb784
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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


2019BR08      Riv.Nuovo Cimento Soc.Ital.Fis. 42, 103 (2019)

C.Broggini, O.Straniero, M.G.F.Taiuti, G.de Angelis, G.Benzoni G.E.Bruno, S.Bufalino, G.Cardella, N.Colonna, M.Contalbrigo, G.Cosentino, S.Cristallo, C.Curceanu, E.De Filippo, R.Depalo, A.Di Leva, A.Feliciello, S.Gammino, A.Galata, M.La Cognata, R.Lea, S.Leoni, I.Lombardo, V.Manzari, D.Mascali, C.Massimi, A.Mengoni, D.Mengoni, D.R.Napoli, S.Palmerini, S.Piano, S.Pirrone, R.G.Pizzone, G.Politi, P.Prati, G.Prete, P.Russotto, G.Tagliente, G.M.Urciuoli

Experimental nuclear astrophysics in Italy

doi: 10.1393/ncr/i2019-10157-1
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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

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

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

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

doi: 10.3847/1538-4357/aac177
Citations: PlumX Metrics


2018ZI03      Phys.Rev. C 97, 065806 (2018)

J.Zickefoose, A.Di Leva, F.Strieder, L.Gialanella, G.Imbriani, N.De Cesare, C.Rolfs, J.Schweitzer, T.Spillane, O.Straniero, F.Terrasi

Measurement of th e 12C(12C, p)23Na cross section near the Gamow energy

NUCLEAR REACTIONS 12C(12C, p), E=2.00-4.00 MeV; measured Ep, Ip, thick-target yields at CIRCE, Vanvitelli accelerator facility; deduced astrophysical S-factor for p0 and p1 channels, proton-channel to total S-factor ratio, resonance strength at 2.1 MeV, and constrained potential resonance strength at 1.5 MeV. Comparison with previous experimental, and with potential model calculations.

doi: 10.1103/PhysRevC.97.065806
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2524. Data from this article have been entered in the XUNDL database. For more information, click here.


2017DI09      Phys.Rev. C 95, 045803 (2017)

A.Di Leva, G.Imbriani, R.Buompane, L.Gialanella, A.Best, S.Cristallo, M.De Cesare, A.D'Onofrio, J.G.Duarte, L.R.Gasques, L.Morales-Gallegos, A.Pezzella, G.Porzio, D.Rapagnani, V.Roca, M.Romoli, D.Schurmann, O.Straniero, F.Terrasi

Measurement of 1323 and 1487 keV resonances in 15N(α, γ)19F with the recoil separator ERNA

NUCLEAR REACTIONS 4He(15N, γ)19F, E(cm)=1323, 1487 keV; measured 19F recoils and reaction yields using the ERNA separator at CIRCE-Italy. 19F; deduced levels, resonances, Γα and Γγ, fractional contribution of resonances and direct capture (DC) component to the total reaction rate of 15N(α, γ)19F, as function of the temperature. Relevance for AGB nucleosynthesis.

doi: 10.1103/PhysRevC.95.045803
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2409. Data from this article have been entered in the XUNDL database. For more information, click here.


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
Citations: PlumX Metrics


2016AL13      Eur.Phys.J. A 52, 76 (2016)

M.Aliotta, M.Junker, P.Prati, O.Straniero, F.Strieder

Helium burning and neutron sources in the stars

doi: 10.1140/epja/i2016-16076-3
Citations: PlumX Metrics


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
Citations: PlumX Metrics

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.


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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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.


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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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.


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


2013HE10      Astrophys.J. 768, L11 (2013)

R.P.Hedrosa, C.Abia, M.Busso, S.Cristallo, I.Dominguez, S.Palmerini, B.Plez, O.Straniero

Nitrogen Isotopes in Asymptotic Giant Branch Carbon Stars and Presolar SiC Grains: A Challenge for Stellar Nucleosynthesis

doi: 10.1088/2041-8205/768/1/L11
Citations: PlumX Metrics


2012ST02      Phys.Lett. B 707, 60 (2012)

F.Strieder, B.Limata, A.Formicola, G.Imbriani, M.Junker, D.Bemmerer, A.Best, C.Broggini, A.Caciolli, P.Corvisiero, H.Costantini, A.DiLeva, Z.Elekes, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, A.Lemut, M.Marta, C.Mazzocchi, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, C.Rossi Alvarez, E.Somorjai, O.Straniero, F.Terrasi, H.P.Trautvetter

The 25Mg(p, γ)26Al reaction at low astrophysical energies

NUCLEAR REACTIONS 25Mg(p, γ)26Al, E(cm) = 92, 189 keV; measured reaction products Eγ, Iγ; deduced energy levels, branching ratios, total resonance strength, screening effects.

doi: 10.1016/j.physletb.2011.12.029
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1976.


2011MA25      Phys.Rev. C 83, 045804 (2011)

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

The 14N( p, γ )15O reaction studied with a composite germanium detector

NUCLEAR REACTIONS 14N(p, γ), E=359, 380, 399 keV; measured Eγ, Iγ, σ. 15O; deduced levels, J, π, branching ratios for four major resonances, corresponding astrophysical S factors. R-matrix analysis for capture to ground state. Relevance to (CNO) cycle of hydrogen burning.

doi: 10.1103/PhysRevC.83.045804
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1912. Data from this article have been entered in the XUNDL database. For more information, click here.


2010CR05      J.Phys.:Conf.Ser. 202, 012033 (2010)

S.Cristallo, L.Piersanti, R.Gallino, O.Straniero, F.Kappeler, I.Dominguez, P.Mohr

The long-standing problem of 176Lu/176Hf branching: A new approach with full stellar evolutionary models

NUCLEAR REACTIONS 175Lu(n, γ), E above 15 keV; calculated long-term time behaviour of 176Lu and 176Hf [product of β-decay of excited 176Lu].

doi: 10.1088/1742-6596/202/1/012033
Citations: PlumX Metrics


2010LE21      Phys.Rev. C 82, 055804 (2010), Erratum Phys.Rev. C 84, 019902 (2011)

P.J.LeBlanc, G.Imbriani, J.Gorres, M.Junker, R.Azuma, M.Beard, D.Bemmerer, A.Best, C.Broggini, A.Caciolli, P.Corvisiero, H.Costantini, M.Couder, R.deBoer, Z.Elekes, S.Falahat, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, F.Kappeler, A.Kontos, R.Kuntz, H.Leiste, A.Lemut Q.Li, B.Limata, M.Marta, C.Mazzocchi, R.Menegazzo, S.O'Brien, A.Palumbo, P.Prati, V.Roca, C.Rolfs, C.Rossi Alvarez, E.Somorjai, E.Stech, O.Straniero, F.Strieder, W.Tan, F.Terrasi, H.P.Trautvetter, E.Uberseder, M.Wiescher

Constraining the S factor of 15N(p, γ)16O at astrophysical energies

NUCLEAR REACTIONS 15N(p, γ), E=130-1800 keV; measured Ep, Ip, Eγ, Iγ, σ(E), σ(θ); deduced resonances, branching ratios, astrophysical S factors and reaction rates. Multilevel R-matrix analysis. Implications for the first and second cycles of the CNO cycles.

doi: 10.1103/PhysRevC.82.055804
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1825. Data from this article have been entered in the XUNDL database. For more information, click here.


2010LI22      Phys.Rev. C 82, 015801 (2010)

B.Limata, F.Strieder, A.Formicola, G.Imbriani, M.Junker, H.W.Becker, D.Bemmerer, A.Best, R.Bonetti, C.Broggini, A.Caciolli, P.Corvisiero, H.Costantini, A.DiLeva, Z.Elekes, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, A.Lemut, M.Marta, C.Mazzocchi, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, C.Rossi Alvarez, C.Salvo, E.Somorjai, O.Straniero, F.Terrasi, H.-P.Trautvetter, for the LUNA Collaboration

New experimental study of low-energy (p, γ) resonances in magnesium isotopes

NUCLEAR REACTIONS 24Mg(p, γ)25Al, E=214 keV; 25Mg(p, γ)26Al, E=304 keV; 26Mg(p, γ)27Al, E=326 keV; measured Eγ, Iγ, resonance strengths and thick target yield curves at LUNA facility. 25,26,27Al; deduced levels, γ-ray branching ratios of primary γ rays from capture states.

doi: 10.1103/PhysRevC.82.015801
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1854. 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


2009CA05      Eur.Phys.J. A 39, 179 (2009)

A.Caciolli, L.Agostino, D.Bemmerer, R.Bonetti, C.Broggini, F.Confortola, P.Corvisiero, H.Costantini, Z.Elekes, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, M.Junker, M.Laubenstein, A.Lemut, B.Limata, 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

Ultra-sensitive in-beam γ-ray spectroscopy for nuclear astrophysics at LUNA

doi: 10.1140/epja/i2008-10706-3
Citations: PlumX Metrics


2008CO12      Nucl.Phys. A814, 144 (2008)

H.Costantini, D.Bemmerer, F.Confortola, A.Formicola, Gy.Gyurky, P.Bezzon, R.Bonetti, C.Broggini, P.Corvisiero, Z.Elekes, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, G.Imbriani, M.Junker, M.Laubenstein, A.Lemut, B.Limata, V.Lozza, M.Marta, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, C.Rossi Alvarez, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter

The 3He(α, γ)7Be S-factor at solar energies: The prompt γ experiment at LUNA

NUCLEAR REACTIONS 3He(α, γ), E=220, 250, 400 keV; measured Eγ, Iγ, σ, branching ratio; deduced astrophysical S-factor. Prompt-γ technique, HPGe detector in the Gran Sasso underground laboratory. Comparison with other data.

doi: 10.1016/j.nuclphysa.2008.09.014
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1709.


2008FO04      J.Phys.(London) G35, 014013 (2008)

A.Formicola, A.Best, G.Imbriani, M.Junker, D.Bemmerer, R.Bonetti, C.Broggini, A.Caciolli, F.Confortola, P.Corvisiero, H.Costantini, Z.Elekes, Zs.Fulop, G.Gervino, A.Guglielmetti, G.Gyurky, C.Gustavino, A.Lemut, B.Limata, 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

Measurement of 25Mg(p, γ)26Al resonance strengths via gamma spectrometry

NUCLEAR REACTIONS 25Mg(p, γ), E not given;measured Eγ, Iγ; deduced resonance strengths.

doi: 10.1088/0954-3899/35/1/014013
Citations: PlumX Metrics


2008GY01      J.Phys.(London) G35, 014002 (2008)

G.Gyurky, D.Bemmerer, F.Confortola, H.Costantini, A.Formicola, R.Bonetti, C.Broggini, P.Corvisiero, Z.Elekes, Z.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, G.Imbriani, M.Junker, M.Laubenstein, A.Lemut, B.Limata, V.Lozza, M.Marta, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, C.Rossi Alvarez, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter

Comparison of the LUNA 3He(α, γ)7Be activation results with earlier measurements and model calculations

NUCLEAR REACTIONS 3He(α, γ), E(cm)=92.9, 105.6, 105.7, 126.5, 147.7, 168.9, 169.5 keV; analyzed activation cross sections; calculated S-factor. Comparisons with previous experimental data.

doi: 10.1088/0954-3899/35/1/014002
Citations: PlumX Metrics


2008MA36      Phys.Rev. C 78, 022802 (2008)

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

Precision study of ground state capture in the 14N(p, γ)15O reaction

NUCLEAR REACTIONS 14N(p, γ), E=359, 380, 399 keV; measured Eγ, Iγ, σ ratios; deduced astrophysical S-factors. R-matrix analysis for capture to g.s. of 15O.

doi: 10.1103/PhysRevC.78.022802
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1693.


2008TR03      J.Phys.(London) G35, 014019 (2008)

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

Ground state capture in 14N(p, γ)15O studied above the 259 keV resonance at LUNA

NUCLEAR REACTIONS 14N(p, γ), E=360, 380, 400 keV; measured Eγ, Iγ, cross sections; deduced astrophysical S-factor. Comparisons with existing data. R-matrix analysis.

doi: 10.1088/0954-3899/35/1/014019
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1912.


2007CO17      Phys.Rev. C 75, 065803 (2007); Pub.Note: Phys.Rev. C 75, 069903 (2007)

F.Confortola, D.Bemmerer, H.Costantini, A.Formicola, Gy.Gyurky, P.Bezzon, R.Bonetti, C.Broggini, P.Corvisiero, Z.Elekes, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, G.Imbriani, M.Junker, M.Laubenstein, A.Lemut, B.Limata, V.Lozza, M.Marta, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, C.Rossi Alvarez, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, and the LUNA Collaboration

Astrophysical S factor of the 3He(α, γ)7Be reaction measured at low energy via detection of prompt and delayed γ rays

NUCLEAR REACTIONS 3He(α, γ), E=220, 250, 400 keV; measured Eγ, Iγ. Deduced cross section and S-factor.

doi: 10.1103/PhysRevC.75.065803
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1516.


2007GY01      Phys.Rev. C 75, 035805 (2007)

Gy.Gyurky, F.Confortola, H.Costantini, A.Formicola, D.Bemmerer, R.Bonetti, C.Broggini, P.Corvisiero, Z.Elekes, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, G.Imbriani, M.Junker, M.Laubenstein, A.Lemut, B.Limata, V.Lozza, M.Marta, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, C.Rossi Alvarez, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, and the LUNA Collaboration

3He(α, γ)7Be cross section at low energies

NUCLEAR REACTIONS 3He(α, γ), E=250, 300, 350, 400 keV; measured Eγ, Iγ, σ; deduced astrophysical S-factor.

doi: 10.1103/PhysRevC.75.035805
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1520.


2006BE41      Phys.Rev.Lett. 97, 122502 (2006)

D.Bemmerer, F.Confortola, H.Costantini, A.Formicola, Gy.Gyurky, R.Bonetti, C.Broggini, P.Corvisiero, Z.Elekes, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, G.Imbriani, M.Junker, M.Laubenstein, A.Lemut, B.Limata, V.Lozza, M.Marta, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, C.Rossi Alvarez, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, and the LUNA Collaboration

Activation Measurement of the 3He(α, γ)7Be Cross Section at Low Energy

NUCLEAR REACTIONS 3He(α, γ), E=300, 350, 400 keV; measured σ; deduced astrophysical S-factors. Activation technique.

doi: 10.1103/PhysRevLett.97.122502
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1399.


2006BE44      Eur.Phys.J. A 27, Supplement 1, 161 (2006)

D.Bemmerer, F.Confortola, A.Lemut, R.Bonetti, C.Broggini, P.Corvisiero, H.Costantini, J.Cruz, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, A.P.Jesus, M.Junker, B.Limata, R.Menegazzo, P.Prati, V.Roca, D.Rogalla, C.Rolfs, M.Romano, C.Rossi Alvarez, F.Schumann, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, and the LUNA Collaboration

CNO hydrogen burning studied deep underground

doi: 10.1140/epja/i2006-08-024-7
Citations: PlumX Metrics


2006BE50      Nucl.Phys. A779, 297 (2006)

D.Bemmerer, F.Confortola, A.Lemut, R.Bonetti, C.Broggini, P.Corvisiero, H.Costantini, J.Cruz, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, A.Jesus, M.Junker, B.Limata, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, D.Rogalla, M.Romano, C.Rossi-Alvarez, F.Schumann, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, and the LUNA Collaboration

Low energy measurement of the 14N(p, γ)15O total cross section at the LUNA underground facility

NUCLEAR REACTIONS 14N(p, γ), E=70-228 keV; measured Eγ, σ; deduced astrophysical S-factor, resonance strength.

doi: 10.1016/j.nuclphysa.2006.09.001
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1458.


2006CO13      Eur.Phys.J. A 27, Supplement 1, 177 (2006)

H.Costantini, D.Bemmerer, P.Bezzon, R.Bonetti, C.Broggini, M.L.Casanova, F.Confortola, P.Corvisiero, J.Cruz, Z.Elekes, A.Formicola, Zs.Fulop, G.Gervino, C.Gustavino, A.Guglielmetti, Gy.Gyurky, G.Imbriani, A.P.Jesus, M.Junker, A.Lemut, M.Marta, R.Menegazzo, P.Prati, E.Roca, C.Rolfs, M.Romano, C.Rossi Alvarez, F.Schumann, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter

Towards a high-precision measurement of the 3He(α, γ)7Be cross section at LUNA

NUCLEAR REACTIONS 3He(α, γ), E=280, 327, 373 keV; calculated expected counting rate for activation experiment.

doi: 10.1140/epja/i2006-08-026-5
Citations: PlumX Metrics


2006LE13      Phys.Lett. B 634, 483 (2006)

A.Lemut, D.Bemmerer, F.Confortola, R.Bonetti, C.Broggini, P.Corvisiero, H.Costantini, J.Cruz, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, A.P.Jesus, M.Junker, B.Limata, R.Menegazzo, P.Prati, V.Roca, D.Rogalla, C.Rolfs, M.Romano, C.Rossi Alvarez, F.Schumann, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, and the LUNA Collaboration

First measurement of the 14N(p, γ)15O cross section down to 70 keV

NUCLEAR REACTIONS 14N(p, γ), E=70-228 keV; measured Eγ, Iγ, σ; deduced astrophysical S-factor and thermonuclear reaction rate. 14N(p, γ), E=259 keV; measured Eγ, Iγ; deduced resonance strength. Comparison with other data, discussed astrophysical consequences.

doi: 10.1016/j.physletb.2006.02.021
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1364.


2006ST35      Nucl.Phys. A777, 311 (2006)

O.Straniero, R.Gallino, S.Cristallo

s process in low-mass asymptotic giant branch stars

doi: 10.1016/j.nuclphysa.2005.01.011
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2005BE28      Eur.Phys.J. A 24, 313 (2005)

D.Bemmerer, F.Confortola, A.Lemut, R.Bonetti, C.Broggini, P.Corvisiero, H.Costantini, J.Cruz, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, A.P.Jesus, M.Junker, B.Limata, R.Menegazzo, P.Prati, V.Roca, D.Rogalla, C.Rolfs, M.Romano, C.Rossi Alvarez, F.Schumann, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, A.Vomiero

Feasibility of low-energy radiative-capture experiments at the LUNA underground accelerator facility

doi: 10.1140/epja/i2004-10135-4
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2005CO16      Nucl.Phys. A758, 383c (2005)

H.Costantini, C.Angulo, D.Bemmerer, R.Bonetti, C.Broggini, F.Confortola, P.Corvisiero, J.Cruz, P.Descouvemont, A.Formicola, Z.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, G.Gyurky, G.Imbriani, A.P.Jesus, M.Junker, A.Lemut, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, M.Romano, C.Rossi Alvarez, F.Schumann, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, A.Vomiero, S.Zavatarelli

Recent results of the 14N(p, γ)15O measurement at LUNA

NUCLEAR REACTIONS 14N(p, γ), E=low; measured Eγ, Iγ; deduced S-factors.

doi: 10.1016/j.nuclphysa.2005.05.069
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1458.


2005CR04      Nucl.Phys. A758, 509c (2005)

S.Cristallo, O.Straniero, R.Gallino

S-process nucleosynthesis in low mass AGB Stars: do we really need an improved determination of the 13C(α, n)16O reaction rate?

doi: 10.1016/j.nuclphysa.2005.05.181
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2005GA39      Nucl.Phys. A758, 485c (2005)

R.Gallino, D.Delaude, L.Husti, S.Cristallo, O.Straniero, S.Ryan

Predictions of s-process Lead in low-metallicity stars compared with spectroscopic observations

doi: 10.1016/j.nuclphysa.2005.05.089
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2005IM02      Eur.Phys.J. A 25, 455 (2005)

G.Imbriani, H.Costantini, A.Formicola, A.Vomiero, C.Angulo, D.Bemmerer, R.Bonetti, C.Broggini, F.Confortola, P.Corvisiero, J.Cruz, P.Descouvemont, Z.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, A.P.Jesus, M.Junker, J.N.Klug, A.Lemut, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, M.Romano, C.Rossi-Alvarez, F.Schumann, D.Schurmann, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter

S-factor of 14N(p, γ)15O at astrophysical energies

NUCLEAR REACTIONS 14N(p, γ), E(cm)=119-367 keV; measured Eγ, Iγ, excitation functions; deduced astrophysical S-factors. R-matrix analysis.

doi: 10.1140/epja/i2005-10138-7
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1195.


2005NI17      Nucl.Phys. A758, 348c (2005)

L.R.Nittler, R.Gallino, M.Lugaro, O.Straniero, I.Dominguez, E.Zinner

Si and C Isotopes in Presolar Silicon Carbide Grains From AGB Stars

doi: 10.1016/j.nuclphysa.2005.05.064
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2005PR20      J.Phys.(London) G31, S1537 (2005)

P.Prati, D.Bemmerer, R.Bonetti, C.Broggini, F.Confortola, P.Corvisiero, H.Costantini, J.Cruz, A.Formicola, Z.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, G.Gyurky, G.Imbriani, A.P.Jesus, M.Junker, A.Lemut, R.Menegazzo, V.Roca, C.Rolfs, M.Romano, C.Rossi Alvarez, F.Schumann, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter

Recent results from the LUNA facility at Gran Sasso

NUCLEAR REACTIONS 14N(p, γ), E=low; measured Eγ, Iγ; deduced astrophysical S-factor. Solid and gas targets.

doi: 10.1088/0954-3899/31/10/027
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2004CO27      Nuovo Cim. C 27, 423 (2004)

F.Confortola, D.Bemmerer, R.Bonetti, C.Broggini, P.Corvisiero, H.Costantini, J.Cruz, A.Formicola, Z.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, G.Gyurky, G.Imbriani, A.P.Jesus, M.Junker, A.Lemut, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, M.Romano, C.Rossi Alvarez, F.Schumann, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, S.Zavatarelli

The 14N(p, γ)15O measurement at low energy

NUCLEAR REACTIONS 14N(p, γ), E=low; measured astrophysical S-factors. Solid and gas targets.

doi: 10.1393/ncc/i2005-10009-5
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2004FO02      Phys.Lett. B 591, 61 (2004)

A.Formicola, G.Imbriani, H.Costantini, C.Angulo, D.Bemmerer, R.Bonetti, C.Broggini, P.Corvisiero, J.Cruz, P.Descouvemont, Z.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, G.Gyurky, A.P.Jesus, M.Junker, A.Lemut, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, M.Romano, C.Rossi Alvarez, F.Schumann, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, A.Vomiero, S.Zavatarelli

Astrophysical S-factor of 14N(p, γ)15O

NUCLEAR REACTIONS 14N(p, γ), E=140-400 keV; measured Eγ, Iγ, capture σ; deduced astrophysical S-factor. R-matrix analysis.

doi: 10.1016/j.physletb.2004.03.092
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1195.


2004KA26      Phys.Rev. C 69, 055802 (2004)

F.Kappeler, C.Arlandini, M.Heil, F.Voss, K.Wisshak, R.Reifarth, O.Straniero, R.Gallino, S.Masera, C.Travaglio

Stellar neutron capture on 180Tam. II. Defining the s-process contribution to nature's rarest isotope

NUCLEAR REACTIONS 180mTa(n, γ), E=low; analyzed capture σ; deduced s-process contribution to solar abundance.

doi: 10.1103/PhysRevC.69.055802
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2003AR21      Nucl.Phys. A718, 536c (2003)

E.Arnone, R.Gallino, D.L.Lambert, O.Straniero

Nucleosynthesis in FG Sge

doi: 10.1016/S0375-9474(03)00836-4
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2003GA27      Nucl.Phys. A718, 181c (2003)

R.Gallino, E.Arnone, S.Cristallo, S.Masera, C.Travaglio, D.L.Lambert, M.Lugaro, F.Kappeler, H.Van Winckel, M.Reyniers, O.Straniero, A.M.Davis

Minute steps on the quest of the s-process

doi: 10.1016/S0375-9474(03)00711-5
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2001AL25      Nucl.Phys. A690, 790 (2001)

M.Aliotta, F.Raiola, G.Gyurky, A.Formicola, R.Bonetti, C.Broggini, L.Campajola, P.Corvisiero, H.Costantini, A.D'Onofrio, Z.Fulop, G.Gervino, L.Gialanella, A.Guglielmetti, C.Gustavino, G.Imbriani, M.Junker, P.G.Moroni, A.Ordine, P.Prati, V.Roca, D.Rogalla, C.Rolfs, M.Romano, F.Schumann, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, S.Zavatarelli

Electron Screening Effect in the Reactions 3He(d, p)4He and d(3He, p)4He

NUCLEAR REACTIONS 3He(d, p), E(cm)=5-60 keV; 2H(3He, p), E(cm)=10-40 keV; measured proton spectra, excitation functions, S(E); deduced electron screening contributions.

doi: 10.1016/S0375-9474(01)00366-9
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetA0228.


2001CR05      Nucl.Phys. A688, 217c (2001)

S.Cristallo, O.Straniero, R.Gallino, F.Herwig, A.Chieffi, M.Limongi, M.Busso

The Formation of the 13C Pocket in Asymptotic Giant Branch Stars and Related Nucleosynthesis

doi: 10.1016/S0375-9474(01)00701-1
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2001DO11      Nucl.Phys. A688, 21c (2001)

I.Dominguez, P.Hoflich, O.Straniero

Type Ia Supernovae: Differences due to progenitors within delayed detonation explosions

doi: 10.1016/S0375-9474(01)00661-3
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2001DO12      Nucl.Phys. A688, 399c (2001)

I.Dominguez, C.Abia, O.Straniero, A.Chieffi, M.Limongi

The Role of Z = 0 AGB Stars on the Early Chemical Enrichment

doi: 10.1016/S0375-9474(01)00736-9
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2001IM01      Nucl.Phys. A688, 249c (2001)

G.Imbriani, O.Straniero, F.Terrasi, M.Limongi, A.Chieffi

Influence of the 12C(α, γ)16O Reaction Rate on the Evolution of a 15 M(sun)

NUCLEAR REACTIONS 12C(α, γ), E=low; analyzed σ; deduced stellar evolution features.

doi: 10.1016/S0375-9474(01)00708-4
Citations: PlumX Metrics


2001RA21      Eur.Phys.J. A 10, 487 (2001)

F.Raiola, G.Gyurky, M.Aliotta, A.Formicola, R.Bonetti, C.Broggini, L.Campajola, P.Corvisiero, H.Costantini, A.D'Onofrio, Z.Fulop, G.Gervino, L.Gialanella, A.Guglielmetti, C.Gustavino, G.Imbriani, M.Junker, R.W.Kavanagh, P.G.P.Moroni, A.Ordine, P.Prati, V.Roca, D.Rogalla, C.Rolfs, M.Romano, F.Schumann, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, S.Zavatarelli

Stopping Power of Low-Energy Deuterons in 3He Gas

NUCLEAR REACTIONS 3He(d, p), E=10-100 keV; measured proton spectra; deduced deuteron stpping power in He gas.

doi: 10.1007/s100500170107
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2001ST27      Nucl.Phys. A696, 219 (2001)

F.Strieder, L.Gialanella, G.Gyurky, F.Schumann, R.Bonetti, C.Broggini, L.Campajola, P.Corvisiero, H.Costantini, A.D'Onofrio, A.Formicola, Z.Fulop, G.Gervino, U.Greife, A.Guglielmetti, C.Gustavino, G.Imbriani, M.Junker, P.G.P.Moroni, A.Ordine, P.Prati, V.Roca, D.Rogalla, C.Rolfs, M.Romano, E.Somorjai, O.Straniero, F.Terrasi, H.P.Trautvetter, S.Zavatarelli

Absolute Cross Section of 7Be(p, γ)8B

NUCLEAR REACTIONS 7Be(p, γ), E(cm)=0.32-2.61 MeV; measured delayed Eα, σ(E); deduced astrophysical S-factor. Comparison with previous results.

doi: 10.1016/S0375-9474(01)01121-6
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetA0414.


2001WI22      Phys.Rev.Lett. 87, 251102 (2001)

K.Wisshak, F.Voss, C.Arlandini, F.Becvar, O.Straniero, R.Gallino, M.Heil, F.Kappeler, M.Krticka, S.Masera, R.Reifarth, C.Travaglio

Neutron Capture on 180Tam: Clue for an s-process origin of nature's rarest isotope

NUCLEAR REACTIONS 180mTa(n, γ), E=10-100 keV; measured capture σ; deduced astrophysical average capture σ.

doi: 10.1103/PhysRevLett.87.251102
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22801.


2000CO17      Phys.Lett. 482B, 43 (2000)

H.Costantini, A.Formicola, M.Junker, R.Bonetti, C.Broggini, L.Campajola, P.Corvisiero, A.D'Onofrio, A.Fubini, G.Gervino, L.Gialanella, U.Greife, A.Guglielmetti, C.Gustavino, G.Imbriani, A.Ordine, P.G.Prada Moroni, P.Prati, V.Roca, D.Rogalla, C.Rolfs, M.Romano, F.Schumann, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, S.Zavatarelli

Stopping Power, Electron Screening and the Astrophysical S(E) Factor of d(3He, p)4He

NUCLEAR REACTIONS 2H(3He, p), E=11-35 keV; measured σ; deduced electron screening effect, stopping power, astrophysical S factor. Gas target.

doi: 10.1016/S0370-2693(00)00513-X
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetA0342.


2000FO14      Eur.Phys.J. A 8, 443 (2000)

A.Formicola, M.Aliotta, G.Gyurky, F.Raiola, R.Bonetti, C.Broggini, L.Campajola, P.Corvisiero, H.Costantini, A.D'Onofrio, Z.Fulop, G.Gervino, L.Gialanella, A.Guglielmetti, C.Gustavino, G.Imbriani, M.Junker, A.Ordine, P.Prati, V.Roca, D.Rogalla, C.Rolfs, M.Romano, F.Schumann, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, S.Zavatarelli

Energy Loss of Deuterons in 3He Gas: A threshold effect

NUCLEAR REACTIONS 3He(d, p), E=15-100 keV; measured proton yield; deduced stopping power by normalizing yield to known cross section. Nuclear astrophysics implications discussed.

doi: 10.1007/s100530050054
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1999AR31      Astrophys.J. 525, 886 (1999)

C.Arlandini, F.Kappeler, K.Wisshak, R.Gallino, M.Lugaro, M.Busso, O.Straniero

Neutron Capture in Low-Mass Asymptotic Giant Branch Stars: Cross Sections and Abundance Signatures

COMPILATION 140,141,142Ce, 141,142Pr, 142,143,144Nd(n, γ); compiled experimental nuclear reaction σ data; deduced sensitive test for models of s-process nucleosynthesis.

doi: 10.1086/307938
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1998ST20      Eur.Phys.J. A 3, 1 (1998)

F.Strieder, F.Schumann, L.Gialanella, U.Greife, D.Rogalla, C.Rolfs, H.P.Trautvetter, Zs.Fulop, G.Gyurky, E.Somorjai, R.W.Kavanagh, L.Campajola, A.D'Onofrio, A.Ordine, V.Roca, M.Romano, F.Terrasi, C.Arpesella, A.D'Alessandro, C.Gustavino, M.Junker, O.Straniero, P.Corvisiero, M.Dessalvi, P.Prati, S.Zavatarelli, C.Broggini, G.Gervino, A.Fubini, E.Bellotti, R.Bonetti, A.Guglielmetti

Loss of 8Li Recoil Nuclei in 7Li(d, p)8Li and Implications on the 7Be(p, γ)8B Cross Section

NUCLEAR REACTIONS 7Li(d, p), E=0.4-1.8 MeV; measured yields; deduced recoil loss for several backing materials. 7Be(p, γ), E not given; deduced possible corrections to σ. Astrophysical implications.

doi: 10.1007/s100500050141
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1997GA19      Nucl.Phys. A621, 423c (1997)

R.Gallino, C.Arlandini, M.Lugaro, M.Busso, O.Straniero

The New s-Process in Low Mass TP-AGB Stars

doi: 10.1016/S0375-9474(97)00284-4
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1997LI20      Nucl.Phys. A621, 453c (1997)

M.Limongi, A.Chieffi, O.Straniero

The Evolutionary History of a 25M(solar) Star

doi: 10.1016/S0375-9474(97)00289-3
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1996CA17      Z.Phys. A354, 237 (1996)

V.Castellani, G.Fiorentini, B.Ricci, O.Straniero

The Fate of Li and Be in Stars and the Laboratory

NUCLEAR REACTIONS 6,7Li, 9Be(p, X), E not given; calculated reactivity N(A)<σv> vs temperature, other aspects; deduced Li, Be fate in stars and reproducibility in laboratory related futures.

doi: 10.1007/s002180050040
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