NSR Query Results
Output year order : Descending NSR database version of April 24, 2024. Search: Author = A.Vomiero Found 11 matches. 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=4001400 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
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
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
2008SC01 Phys.Lett. B 658, 109 (2008) W.Scandale, A.Carnera, G.Della Mea, D.De Salvador, R.Milan, A.Vomiero, S.Baricordi, P.Dalpiaz, M.Fiorini, V.Guidi, G.Martinelli, A.Mazzolari, E.Milan, G.Ambrosi, P.Azzarello, R.Battiston, B.Bertucci, W.J.Burger, M.Ionica, P.Zuccon, G.Cavoto, R.Santacesaria, P.Valente, E.Vallazza, A.G.Afonin, V.T.Baranov, Y.A.Chesnokov, V.I.Kotov, V.A.Maisheev, I.A.Yazynin, S.V.Afanasiev, A.D.Kovalenko, A.M.Taratin, A.S.Denisov, Y.A.Gavrikov, Y.M.Ivanov, V.G.Ivochkin, S.V.Kosyanenko, L.P.Lapina, A.A.Petrunin, V.V.Skorobogatov, V.M.Suvorov, D.Bolognini, L.Foggetta, S.Hasan, M.Prest Double volume reflection of a proton beam by a sequence of two bent crystals
doi: 10.1016/j.physletb.2007.10.070
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
2007SC14 Phys.Rev.Lett. 98, 154801 (2007) W.Scandale, D.A.Still, A.Carnera, G.Della Mea, D.De Salvador, R.Milan, A.Vomiero, S.Baricordi, P.Dalpiaz, M.Fiorini, V.Guidi, G.Martinelli, A.Mazzolari, E.Milan, G.Ambrosi, P.Azzarello, R.Battiston, B.Bertucci, W.J.Burger, M.Ionica, P.Zuccon, G.Cavoto, R.Santacesaria, P.Valente, E.Vallazza, A.G.Afonin, V.T.Baranov, Y.A.Chesnokov, V.I.Kotov, V.A.Maisheev, I.A.Yaznin, S.V.Afansiev, A.D.Kovalenko, A.M.Taratin, A.S.Denisov, Y.A.Gavrikov, Y.M.Ivanov, V.G.Ivochkin, S.V.Kosyanenko, A.A.Petrunin, V.V.Skorobogatov, V.M.Suvorov, D.Bolognini, L.Foggetta, S.Hasan, M.Prest High-Efficiency Volume Reflection of an Ultrarelativistic Proton Beam with a Bent Silicon Crystal NUCLEAR REACTIONS Si(p, p), E=400 GeV; measured proton spectra, angular distribution as a function of crystal orientation; deduced high-efficiency volume reflection.
doi: 10.1103/PhysRevLett.98.154801
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
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
2005DE54 Nucl.Instrum.Methods Phys.Res. B240, 803 (2005) G.Della Mea, A.Patelli, S.Restello, V.Rigato, A.Vomiero 14N(α, p)17O nuclear reaction cross-section at 4.9-6.1 MeV NUCLEAR REACTIONS 14N(α, p), E=4893-6047 keV; measured σ(θ=172°). Application to nitrogen depth profiling discussed.
doi: 10.1016/j.nimb.2005.06.213
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
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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