NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = R.Gallino Found 53 matches. 2023GA10 Eur.Phys.J. A 59, 66 (2023) Franz and his friends: 35-years of s-process studies by the Karlsruhe-Torino collaboration
doi: 10.1140/epja/s10050-023-00934-8
2023PI08 Eur.Phys.J. A 59, 302 (2023) M.Pignatari, R.Gallino, R.Reifarth The s process in massive stars, a benchmark for neutron capture reaction rates
doi: 10.1140/epja/s10050-023-01206-1
2022LI64 Eur.Phys.J. A 58, 216 (2022) N.Liu, T.Stephan, S.Cristallo, D.Vescovi, R.Gallino, L.R.Nittler, C.M.O.D.Alexander, A.M.Davis Presolar silicon carbide grains of types Y and Z: their strontium and barium isotopic compositions and stellar origins
doi: 10.1140/epja/s10050-022-00838-z
2014BI20 Astrophys.J. 787, 1 (2014) S.Bisterzo, C.Travaglio, R.Gallino, M.Wiescher, F.Kappeler Galactic chemical evolution and solar s-process abundances: dependence on the 13C-pocket structure NUCLEAR REACTIONS 80,82,83,84,86Kr, Kr, 85,87Rb, Rb, 86,87,88Sr, Sr, 89Y, Y, 90,91,92,94,96Zr, Zr, 93Nb, Nb, 94,95,96,97,98,100Mo, Mo, 99,100,101,102,104Ru, Ru, 103Rh, Rh, 104,105,106,108,110Pd, Pd, 107,109Ag, Ag, 108,110,111,112,113,114,116Cd, Cd, 113,115In, In, 114,115,116,117,118,119,120,122,124Sn, Sn, 121,123Sb, Sb, 122,123,124,125,126,128Te, Te, 127I, I, 128,129,130,131,132,134Xe, Xe, 133Cs, Cs, 134,135,136,137,138Ba, Ba, 139La, La, 140,142Ce, Ce, 141Pr, Pr, 142,143,144,145,146,148Nd, Nd, 147,148,149,150,152,154Sm, Sm, 151,153Eu, Eu, 152,154,155,156,157,158,160Gd, Gd, 159Tb, Tb, 160,161,162,163,164Dy, Dy, 165Ho, Ho, 164,166,167,168,170Er, Er, 169Tm, Tm, 170,171,172,173,174,176Yb, Yb, 175,176Lu, Lu, 176,177,178,179,180Hf, Hf, 180,181Ta, Ta, 180,182,183,184,186W, W, 185,187Re, Re, 186,187,188,189,190,192Os, Os, 191,193Ir, Ir, 192,194,195,196,198Pt, Pt, 197Au, Au, 198,199,200,201,202,204Hg, Hg, 203,205Tl, Tl, 204,206,207,208Pb, Pb, 209Bi, Bi(n, γ), E ∼ 30 keV; analyzed available data; deduced s-process abundances.
doi: 10.1088/0004-637x/787/1/10
2014HE25 Phys.Rev. C 90, 045804 (2014); Erratum Phys.Rev. C 92, 019902 (2015) M.Heil, R.Plag, E.Uberseder, R.Gallino, S.Bisterzo, A.Juseviciute, F.Kappeler, C.Lederer, A.Mengoni, M.Pignatari Stellar neutron capture cross sections of 20, 21, 22Ne NUCLEAR REACTIONS 20,21,22Ne(n, γ), E=5-800 keV; measured transmission data, σ(E) via prompt γ-ray cascades, and using the TOF technique at the Karlsruhe Van de Graaff accelerator. 21,22,23Ne; deduced energies of neutron resonances, resonance parameters, widths, capture kernels, stellar cross sections (MACS) at kT=30 keV, relative s-abundance distributions. R-matrix analysis using SAMMY code. Comparison with previous experimental results and data in KADONIS database. Discussed 22Ne and 20Ne as significant neutron poisons for the s process in stars.
doi: 10.1103/PhysRevC.90.045804
2011KA13 Rev.Mod.Phys. 83, 157 (2011) F.Kappeler, R.Gallino, S.Bisterzo, W.Aoki The s process: Nuclear physics, stellar models, and observations
doi: 10.1103/RevModPhys.83.157
2011TA17 Phys.Rev. C 84, 015801 (2011) G.Tagliente, P.M.Milazzo, K.Fujii, U.Abbondanno, G.Aerts, H.Alvarez, F.Alvarez-Velarde, S.Andriamonje, J.Andrzejewski, L.Audouin, G.Badurek, P.Baumann, F.Becvar, F.Belloni, E.Berthoumieux, S.Bisterzo, F.Calvino, M.Calviani, D.Cano-Ott, R.Capote, C.Carrapico, P.Cennini, V.Chepel, E.Chiaveri, N.Colonna, G.Cortes, A.Couture, J.Cox, M.Dahlfors, S.David, I.Dillmann, C.Domingo-Pardo, W.Dridi, I.Duran, C.Eleftheriadis, M.Embid-Segura, A.Ferrari, R.Ferreira-Marques, W.Furman, R.Gallino, I.Goncalves, E.Gonzalez-Romero, F.Gramegna, C.Guerrero, F.Gunsing, B.Haas, R.Haight, M.Heil, A.Herrera-Martinez, E.Jericha, F.Kappeler, Y.Kadi, D.Karadimos, D.Karamanis, M.Kerveno, E.Kossionides, M.Krticka, C.Lamboudis, H.Leeb, A.Lindote, I.Lopes, M.Lozano, S.Lukic, J.Marganiec, S.Marrone, T.Martnez, C.Massimi, P.Mastinu, A.Mengoni, C.Moreau, M.Mosconi, F.Neves, H.Oberhummer, S.O'Brien, J.Pancin, C.Papachristodoulou, C.Papadopoulos, C.Paradela, N.Patronis, A.Pavlik, P.Pavlopoulos, L.Perrot, M.T.Pigni, R.Plag, A.Plompen, A.Plukis, A.Poch, J.Praena, C.Pretel, J.Quesada, T.Rauscher, R.Reifarth, M.Rosetti, C.Rubbia, G.Rudolf, P.Rullhusen, J.Salgado, C.Santos, L.Sarchiapone, I.Savvidis, C.Stephan, J.L.Tain, L.Tassan-Got, L.Tavora, R.Terlizzi, G.Vannini, P.Vaz, A.Ventura, D.Villamarin, M.C.Vincente, V.Vlachoudis, R.Vlastou, F.Voss, S.Walter, M.Wiescher, K.Wisshak Neutron capture on 94Zr: Resonance parameters and Maxwellian-averaged cross sections NUCLEAR REACTIONS 94Zr(n, γ), E=0.001-60 keV; measured E(n), I(n), capture yield using CERN n_TOF neutron source; deduced resonance parameters ER, gamma and neutron widths, capture kernels; calculated Maxwellian-averaged capture cross sections. 95Zr; deduced resonances, J, l-values, R-matrix analysis. Comparison with previous studies. Discussed astrophysical implications.
doi: 10.1103/PhysRevC.84.015801
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
2010PI15 Astrophys.J. 710, 1557 (2010) M.Pignatari, R.Gallino, M.Heil, M.Wiescher, F.Kappeler, F.Herwig, S.Bisterzo The Weak s-Process in Massive Stars and its Dependence on the Neutron Capture Cross Sections NUCLEAR REACTIONS 74Ge, 75As, 78Se, 36S, 80Kr(n, γ), E ∼ 30 keV; analyzed available data; deduced Maxwellian averaged σ.
doi: 10.1088/0004-637x/710/2/1557
2009DI04 Phys.Rev. C 79, 065805 (2009) I.Dillmann, C.Domingo-Pardo, M.Heil, F.Kappeler, A.Wallner, O.Forstner, R.Golser, W.Kutschera, A.Priller, P.Steier, A.Mengoni, R.Gallino, M.Paul, C.Vockenhuber Determination of the stellar (n, γ) cross section of 40Ca with accelerator mass spectrometry NUCLEAR REACTIONS 40Ca(n, γ), E<106 keV; measured σ, σ(E) using activation technique and accelerator mass spectrometry; deduced Maxwellian averaged cross sections. Neutrons from 7Li(p, n)7Be reaction at E(p)=1912 keV. 197Au(n, γ), E<106 keV; measured σ and used as a standard. Comparison with previous experimental data and theoretical predictions.
doi: 10.1103/PhysRevC.79.065805
2009MA35 Phys.Rev. C 79, 065802 (2009) J.Marganiec, I.Dillmann, C.Domingo Pardo, F.Kappeler, R.Reifarth, R.Gallino, M.Pignatari, P.Grabmayr Neutron capture cross sections of 74Ge, 76Ge, and 75As at 25 keV NUCLEAR REACTIONS 74,76Ge, 75As(n, γ), E<106 keV; measured Eγ, Iγ, σ; deduced Maxwellian averaged σ for thermal energies from 5 to 100 keV. Neutrons from 7Li(p, n), E=1912 keV reaction. 197Au(n, γ), E<106 keV; measured σ and used as a standard. Estimated background contributions for γ-ray studies of double β decay of 76Ge.
doi: 10.1103/PhysRevC.79.065802
2009MO10 Phys.Rev. C 79, 045804 (2009) P.Mohr, S.Bisterzo, R.Gallino, F.Kappeler, U.Kneissl, N.Winckler Properties of the 5- state at 839 keV in 176Lu and the s-process branching at A=176 NUCLEAR STRUCTURE 176Lu; analyzed partial level scheme, coupling between low- and high-K states; calculated reaction rates for photoactivation process and for transitions from high K ground state to low K isomers in 176Lu. Implications for 176Lu/176Hf as thermometer for astrophysical s-process.
doi: 10.1103/PhysRevC.79.045804
2008DO05 J.Phys.(London) G35, 014020 (2008) C.Domingo-Pardo, U.Abbondanno, G.Aerts, H.Alvarez, F.Alvarez-Velarde, S.Andriamonje, J.Andrzejewski, P.Assimakopoulos, L.Audouin, G.Badurek, P.Baumann, F.Becvar, E.Berthoumieux, S.Bisterzo, F.Calvino, M.Calviani, D.Cano-Ott, R.Capote, C.Carrapico, P.Cennini, V.Chepel, N.Colonna, G.Cortes, A.Couture, J.Cox, M.Dahlfors, S.David, I.Dillmann, W.Dridi, I.Duran, C.Eleftheriadis, M.Embid-Segura, L.Ferrant, A.Ferrari, R.Ferreira-Marques, K.Fujii, W.Furman, R.Gallino, I.Goncalves, E.Gonzalez-Romero, F.Gramegna, C.Guerrero, F.Gunsing, B.Haas, R.Haight, M.Heil, A.Herrera-Martinez, M.Igashira, E.Jericha, Y.Kadi, F.Kappeler, D.Karadimos, D.Karamanis, M.Kerveno, P.Koehler, E.Kossionides, M.Krticka, C.Lamboudis, H.Leeb, A.Lindote, I.Lopes, M.Lozano, S.Lukic, J.Marganiec, S.Marrone, C.Massimi, P.Mastinu, A.Mengoni, P.M.Milazzo, M.Mosconi, F.Neves, H.Oberhummer, S.O'Brien, J.Pancin, C.Papachristodoulou, C.Papadopoulos, C.Paradela, N.Patronis, A.Pavlik, P.Pavlopoulos, L.Perrot, M.T.Pigni, R.Plag, A.Plompen, A.Plukis, A.Poch, C.Pretel, J.Quesada, T.Rauscher, R.Reifarth, C.Rubbia, G.Rudolf, P.Rullhusen, J.Salgado, C.Santos, L.Sarchiapone, I.Savvidis, C.Stephan, G.Tagliente, J.L.Tain, L.Tassan-Got, L.Tavora, R.Terlizzi, G.Vannini, P.Vaz, A.Ventura, D.Villamarin, M.C.Vincente, V.Vlachoudis, R.Vlastou, F.Voss, S.Walter, M.Wiescher, K.Wisshak The measurement of the 206Pb(n, γ) cross section and stellar implications NUCLEAR REACTIONS 206Pb(n, γ), E=0.001-1000 keV; measured Eγ, Iγ, capture cross sections. Deduced maxwellian averaged sections.
doi: 10.1088/0954-3899/35/1/014020
2008HE01 Phys.Rev. C 77, 015808 (2008) M.Heil, F.Kappeler, E.Uberseder, R.Gallino, M.Pignatari Neutron capture cross sections for the weak s process in massive stars NUCLEAR REACTIONS 58Fe, 59Co, 64Ni, 63,65Cu(n, γ), E=25 keV; measured neutron capture cross sections, Eγ; 59Fe, 60Co, 65Ni, 64,66Cu, 198Au; deduced nucleosynthesis yields in stars.
doi: 10.1103/PhysRevC.77.015808
2008HE10 Phys.Rev. C 78, 025802 (2008) M.Heil, F.Kappeler, E.Uberseder, R.Gallino, S.Bisterzo, M.Pignatari Stellar (n, γ) cross sections for Br and Rb: Matching the weak and main s-process components NUCLEAR REACTIONS 79,81Br, 85,87Rb(n, γ), E=0-120 keV; measured Eγ, Iγ, σ. 78,80,82Se, 79,81Br, 80,82,83,84,86Kr; 85,87Rb, 86,87,88Sr, 89Y, 90Zr; deduced total s-process abundances.
doi: 10.1103/PhysRevC.78.025802
2008HE17 Astrophys.J. 673, 434 (2008) M.Heil, N.Winckler, S.Dababneh, F.Kappeler, K.Wisshak, S.Bisterzo, R.Gallino, A.M.Davis, T.Rauscher 176Lu/176Hf: A Sensitive Test of s-Process Temperature and Neutron Density in AGB Stars NUCLEAR REACTIONS 175Lu(n, γ), E=spectrum; measured Eγ, Iγ, cross sections, isomeric ratio.
doi: 10.1086/523892
2008SN01 Ann.Rev.Astron.Astrophys. 46, 241 (2008) C.Sneden, J.J.Cowan, R.Gallino Neutron-Capture Elements in the Early Galaxy NUCLEAR REACTIONS 69,71Ga, 70,72,73,74,76Ge, 75As, 76,77,78,80,82Se, 79,81Br, 80,82,83,84,86Kr, 85,87Rb, 86,87,88Sr, 89Y, 90,91,92,94,96Zr, 93Nb, 95,96,97,98,100Mo, 99,100,101,102,104Ru, 103Rh, 104,105,106,108,110Pd, 107,109Ag, 110,111,112,113,114,116Cd, 115In, 116,117,118,119,120,122,124Sn, 121,123Sb, 122,123,124,125,126,128,130Te, 127I, 128,129,130,131,132,134Xe, 133Cs, 134,135,136,137,138Ba, 139La, 140,142Ce, 141Pr, 142,143,144,145,146,148,150Nd, 147,148,149,150,152,154Sm, 151,153Eu, 152,154,155,156,157,158,160Gd, 159Tb, 160,161,162,163,164Dy, 165Ho, 164,166,167,168,170Er, 169Tm, 170,171,172,173,174,176Yb, 175,176Lu, 176,177,178,179,180Hf, 181Ta, 182,183,184,186W, 185,187Re, 186,187,188,189,190,192Os, 191,193Ir, 192,194,195,196,198Pt, 197Au, 198,199,200,201,202,204Hg, 203,205Tl, 204,206,207,208Pb, 209Bi, 232Th, 235,238U(n, γ), E ∼ 30 keV; analyzed available data; deduced s- and r-process abundances.
doi: 10.1146/annurev.astro.46.060407.145207
2007HE14 Prog.Part.Nucl.Phys. 59, 174 (2007) M.Heil, F.Kappeler, E.Uberseder, R.Gallino, M.Pignatari The s process in massive stars
doi: 10.1016/j.ppnp.2006.12.013
2007MO01 Phys.Rev. C 75, 012802 (2007) Survival of nature's rarest isotope 180Ta under stellar conditions NUCLEAR REACTIONS 180mTa(γ, γ'), E=low; analyzed σ, T1/2 in stellar environment.
doi: 10.1103/PhysRevC.75.012802
2007VO02 Phys.Rev. C 75, 015804 (2007) C.Vockenhuber, I.Dillmann, M.Heil, F.Kappeler, N.Winckler, W.Kutschera, A.Wallner, M.Bichler, S.Dababneh, S.Bisterzo, R.Gallino Stellar (n, γ) cross sections of 174Hf and radioactive 182Hf NUCLEAR REACTIONS 174,180,182Hf(n, γ), E=spectrum; measured capture σ; deduced Maxwellian averaged σ, stellar enhancement factors. Comparison with model predictions.
doi: 10.1103/PhysRevC.75.015804
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
2006WA35 Nucl.Phys. A777, 5 (2006) G.J.Wasserburg, M.Busso, R.Gallino, K.M.Nollett Short-lived nuclei in the early Solar System: Possible AGB sources
doi: 10.1016/j.nuclphysa.2005.07.015
2006WI01 Phys.Rev. C 73, 015802 (2006) K.Wisshak, F.Voss, F.Kappeler, M.Krticka, S.Raman, A.Mengoni, R.Gallino Stellar neutron capture cross section of the unstable s-process branching point 151Sm NUCLEAR REACTIONS Sm, 151Sm(n, γ), E=3-225 keV; measured capture σ; deduced Maxwellian averaged σ. Astrophysical implications discussed.
doi: 10.1103/PhysRevC.73.015802
2006WI11 Phys.Rev. C 73, 045807 (2006) K.Wisshak, F.Voss, F.Kappeler, L.Kazakov, F.Becvar, M.Krticka, R.Gallino, M.Pignatari Fast neutron capture on the Hf isotopes: Cross sections, isomer production, and stellar aspects NUCLEAR REACTIONS 176,177,178,179,180Hf(n, γ), E=3-225 keV; measured Eγ, Iγ, capture σ; deduced Maxwellian-averaged σ. Astrophysical implications discussed.
doi: 10.1103/PhysRevC.73.045807
2006WI20 Astrophys.J. 647, 685 (2006) N.Winckler, S.Dababneh, M.Heil, F.Kappeler, R.Gallino, M.Pignatari Lanthanum: An s- and r-Process Indicator NUCLEAR REACTIONS 139La(n, γ), E=5.1 keV; measured reaction products, Eγ, Iγ; deduced Maxwellian-averaged σ and its uncertainties.
doi: 10.1086/505026
2005BI19 Nucl.Phys. A758, 284c (2005) S.Bisterzo, L.Pompeia, R.Gallino, M.Pignatari, K.Cunha, A.Heger, V.Smith Cu and Zn in different stellar populations: Inferring their astrophysical origin
doi: 10.1016/j.nuclphysa.2005.05.049
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
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
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
2005PI19 Nucl.Phys. A758, 541c (2005) M.Pignatari, R.Gallino, F.Kappeler, M.Wiescher Effects of uncertainties of the 22Ne(α, n)25Mg and 13C(α, n)16O reaction rates in the s-process yields NUCLEAR REACTIONS 13C, 22Ne(α, n), E=low; analyzed astrophysical reaction rates.
doi: 10.1016/j.nuclphysa.2005.05.098
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
2004PA06 Phys.Rev. C 69, 025803 (2004) N.Patronis, S.Dababneh, P.A.Assimakopoulos, R.Gallino, M.Heil, F.Kappeler, D.Karamanis, P.E.Koehler, A.Mengoni, R.Plag Neutron capture studies on unstable 135Cs for nucleosynthesis and transmutation NUCLEAR REACTIONS 135Cs(n, γ), E=30, 500 keV; measured capture σ. 133,134,135,136,137Cs(n, γ), E=low; deduced Maxwellian averaged σ. Activation technique, comparison with previous results. RADIOACTIVITY 136Cs(β-) [from 135Cs(n, γ)]; measured T1/2.
doi: 10.1103/PhysRevC.69.025803
2004RA29 Phys.Rev. C 70, 065803 (2004) U.Ratzel, C.Arlandini, F.Kappeler, A.Couture, M.Wiescher, R.Reifarth, R.Gallino, A.Mengoni, C.Travaglio Nucleosynthesis at the termination point of the s process NUCLEAR REACTIONS 208Pb, 209Bi(n, γ), E=spectrum; measured σ. Astrophysical implications discussed. Activation technique.
doi: 10.1103/PhysRevC.70.065803
2004TR05 Astrophys.J. 601, 864 (2004) C.Travaglio, R.Gallino, E.Arnone, J.Cowan, F.Jordan, C.Sneden Galactic evolution of Sr, Y, and Zr: A multiplicity of nucleosynthetic processes
doi: 10.1086/380507
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
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
2003KA50 Nucl.Phys. A718, 173c (2003) F.Kappeler, A.Mengoni, R.Gallino Neutron capture studies on difficult isotopes - experiments, theory, and astrophysics
doi: 10.1016/S0375-9474(03)00710-3
2003LU13 Nucl.Phys. A718, 419c (2003) M.Lugaro, R.Gallino, S.Amari, E.Zinner, L.R.Nittler The Effect of Heterogeneities in the Interstellar Medium on the CNO Isotopic Ratios of Presolar SiC and Corundum Grains
doi: 10.1016/S0375-9474(03)00819-4
2003OB03 Phys.Rev. C 68, 035801 (2003) S.O'Brien, S.Dababneh, M.Heil, F.Kappeler, R.Plag, R.Reifarth, R.Gallino, M.Pignatari Neutron capture cross section of 139La NUCLEAR REACTIONS 139La(n, γ), E=spectrum; measured capture σ; deduced Maxwellian-averaged capture σ. Activation technique. Astrophysical implications discussed.
doi: 10.1103/PhysRevC.68.035801
2003RE39 Astrophys.J. 582, 1251 (2003) R.Reifarth, C.Arlandini, M.Heil, F.Kappeler, P.V.Sedyshev, A.Mengoni, M.Herman, T.Rauscher, R.Gallino, C.Travaglio Stellar Neutron Capture on Promethium: Implications for the s-Process Neutron Density NUCLEAR REACTIONS 147Pm(n, γ), E=25 keV; measured reaction products, Eγ, Iγ; deduced Maxwellian-averaged σ and its uncertainties. NUCLEAR REACTIONS 147,148,149Pm(n, γ), E=5-100 keV; calculated Maxwellian-averaged σ. COMPILATION 146,147,148Nd, 147,148,149Pm, 147,148,149,150Sm(n, γ), E=10, 25, 30 keV; compiled Maxwellian-averaged σ and its uncertainties.
doi: 10.1086/344718
2003SO05 Astrophys.J. 583, 506 (2003) K.Sonnabend, P.Mohr, K.Vogt, A.Zilges, A.Mengoni, T.Rauscher, H.Beer, F.Kappeler, R.Gallino The s-Process Branching at 185W NUCLEAR REACTIONS 186W(γ, n), E=8775 keV bremsstrahlung; measured σ. 186W(γ, n), E=7-10 MeV; calculated σ. 185W(n, γ), E=stellar; calculated Maxwellian averaged σ, astrophysical s-process branching. Activation technique.
doi: 10.1086/345086
2002RE32 Phys.Rev. C 66, 064603 (2002) R.Reifarth, M.Heil, F.Kappeler, F.Voss, K.Wisshak, F.Becvar, M.Krticka, R.Gallino, Y.Nagai Stellar neutron capture cross sections of 128, 129, 130Xe NUCLEAR REACTIONS 128,129,130Xe(n, γ), E=3-225 keV; measured Eγ, Iγ, capture σ; deduced Maxwellian averaged σ. Astrophysical implications discussed.
doi: 10.1103/PhysRevC.66.064603
2001BU21 Nucl.Phys. A688, 505c (2001) M.Busso, R.Gallino, C.Travaglio, M.Lugaro s Processing in Post-AGB and CH Stars at Low Metallicity
doi: 10.1016/S0375-9474(01)00770-9
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
2001GA39 Nucl.Phys. A688, 433c (2001) R.Gallino, C.Travaglio, S.Amari, E.Zinner Mixing of SN Ejecta with O > C
doi: 10.1016/S0375-9474(01)00747-3
2001RY03 Nucl.Phys. A688, 209c (2001) S.G.Ryan, W.Aoki, J.E.Norris, T.C.Beers, R.Gallino, M.Busso, H.Ando Lead (Pb) in the C-Rich, s-Process Rich, Metal Poor Subgiant LP625-44
doi: 10.1016/S0375-9474(01)00699-6
2001TR14 Nucl.Phys. A688, 213c (2001) C.Travaglio, R.Gallino, M.Busso Galactic Chemical Evolution of Lead: the Role of Asymptotic giant branch stars
doi: 10.1016/S0375-9474(01)00700-X
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
2001ZI04 Nucl.Phys. A688, 102c (2001) E.Zinner, S.Amari, R.Gallino, M.Lugaro Evidence for a Range of Metallicities in the Parent Stars of Presolar SiC Grains
doi: 10.1016/S0375-9474(01)00677-7
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
1997BU13 Nucl.Phys. A621, 431c (1997) s-Process Abundances in AGB Stars at Various Metallicities and Their Theoretical Interpretation
doi: 10.1016/S0375-9474(97)00285-6
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
1993RA24 Astrophys.J. 419, 207 (1993) C.M.Raiteri, R.Gallino, M.Busso, D.Neuberger, F.Kappeler The Weak s-Component and Nucleosynthesis in Massive Stars NUCLEAR REACTIONS 87Rb(n, γ), E=25, 30 keV; measured reaction products, Eγ, Iγ; deduced Maxwellian-averaged σ and its uncertainties. COMPILATION 58,59,60Fe, 59,60Co, 58,59,60,61,62,63,64Ni, 63,64,65Cu, 64,65,66,67,68,70Zn, 69,71Ga, 70,71,72,73,74,76Ge, 75As, 76,77,78,79,80,82Se, 79,80,81Br, 80,81,82,83,84,85,86Kr, 85,86,87Rb, 86,87,88,89,90Sr, 89,90Y, 90,91,92,93,94,96Zr(n, γ), E=26, 91 keV; compiled experimental and theoretical (n, γ) Maxwellian-averaged σ and their uncertainties.
doi: 10.1086/173476
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