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Search: Author = R.Gallino

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2023GA10      Eur.Phys.J. A 59, 66 (2023)

R.Gallino

Franz and his friends: 35-years of s-process studies by the Karlsruhe-Torino collaboration

doi: 10.1140/epja/s10050-023-00934-8
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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 ^{80,82,83,84,86}Kr, Kr, ^85,87Rb, Rb, ^86,87,88Sr, Sr, ⁸⁹Y, Y, ^{90,91,92,94,96}Zr, Zr, ⁹³Nb, Nb, ^{94,95,96,97,98,100}Mo, Mo, ^{99,100,101,102,104}Ru, Ru, ¹⁰³Rh, Rh, ^{104,105,106,108,110}Pd, Pd, ^107,109Ag, Ag, ^{108,110,111,112,113,114,116}Cd, Cd, ^113,115In, In, ^{114,115,116,117,118,119,120,122,124}Sn, Sn, ^121,123Sb, Sb, ^{122,123,124,125,126,128}Te, Te, ¹²⁷I, I, ^{128,129,130,131,132,134}Xe, Xe, ¹³³Cs, Cs, ^{134,135,136,137,138}Ba, Ba, ¹³⁹La, La, ^140,142Ce, Ce, ¹⁴¹Pr, Pr, ^{142,143,144,145,146,148}Nd, Nd, ^{147,148,149,150,152,154}Sm, Sm, ^151,153Eu, Eu, ^{152,154,155,156,157,158,160}Gd, Gd, ¹⁵⁹Tb, Tb, ^{160,161,162,163,164}Dy, Dy, ¹⁶⁵Ho, Ho, ^{164,166,167,168,170}Er, Er, ¹⁶⁹Tm, Tm, ^{170,171,172,173,174,176}Yb, Yb, ^175,176Lu, Lu, ^{176,177,178,179,180}Hf, Hf, ^180,181Ta, Ta, ^{180,182,183,184,186}W, W, ^185,187Re, Re, ^{186,187,188,189,190,192}Os, Os, ^191,193Ir, Ir, ^{192,194,195,196,198}Pt, Pt, ¹⁹⁷Au, Au, ^{198,199,200,201,202,204}Hg, Hg, ^203,205Tl, Tl, ^{204,206,207,208}Pb, Pb, ²⁰⁹Bi, Bi(n, γ), E ∼ 30 keV; analyzed available data; deduced s-process abundances.

doi: 10.1088/0004-637x/787/1/10
Citations: PlumX Metrics

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, 22}Ne

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
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 dataset23265. Data from this article have been entered in the XUNDL database. For more information, click here.

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
Citations: PlumX Metrics

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 E_R, 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
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 dataset23330. 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

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 dataset14238.

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
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 dataset14237.

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22984.

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
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22996.

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, ^{80,82,83,84,86}Kr; ^85,87Rb, ^86,87,88Sr, ⁸⁹Y, ⁹⁰Zr; deduced total s-process abundances.

doi: 10.1103/PhysRevC.78.025802
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 dataset23035.

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
Citations: PlumX Metrics

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, ^{70,72,73,74,76}Ge, ⁷⁵As, ^{76,77,78,80,82}Se, ^79,81Br, ^{80,82,83,84,86}Kr, ^85,87Rb, ^86,87,88Sr, ⁸⁹Y, ^{90,91,92,94,96}Zr, ⁹³Nb, ^{95,96,97,98,100}Mo, ^{99,100,101,102,104}Ru, ¹⁰³Rh, ^{104,105,106,108,110}Pd, ^107,109Ag, ^{110,111,112,113,114,116}Cd, ¹¹⁵In, ^{116,117,118,119,120,122,124}Sn, ^121,123Sb, ^{122,123,124,125,126,128,130}Te, ¹²⁷I, ^{128,129,130,131,132,134}Xe, ¹³³Cs, ^{134,135,136,137,138}Ba, ¹³⁹La, ^140,142Ce, ¹⁴¹Pr, ^{142,143,144,145,146,148,150}Nd, ^{147,148,149,150,152,154}Sm, ^151,153Eu, ^{152,154,155,156,157,158,160}Gd, ¹⁵⁹Tb, ^{160,161,162,163,164}Dy, ¹⁶⁵Ho, ^{164,166,167,168,170}Er, ¹⁶⁹Tm, ^{170,171,172,173,174,176}Yb, ^175,176Lu, ^{176,177,178,179,180}Hf, ¹⁸¹Ta, ^{182,183,184,186}W, ^185,187Re, ^{186,187,188,189,190,192}Os, ^191,193Ir, ^{192,194,195,196,198}Pt, ¹⁹⁷Au, ^{198,199,200,201,202,204}Hg, ^203,205Tl, ^{204,206,207,208}Pb, 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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

2007MO01      Phys.Rev. C 75, 012802 (2007)

P.Mohr, F.Kappeler, R.Gallino

Survival of nature's rarest isotope ¹⁸⁰Ta under stellar conditions

NUCLEAR REACTIONS ^180mTa(γ, γ'), E=low; analyzed σ, T_1/2 in stellar environment.

doi: 10.1103/PhysRevC.75.012802
Citations: PlumX Metrics

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
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22963.

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22916.

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 ^{176,177,178,179,180}Hf(n, γ), E=3-225 keV; measured Eγ, Iγ, capture σ; deduced Maxwellian-averaged σ. Astrophysical implications discussed.

doi: 10.1103/PhysRevC.73.045807
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22926.

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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 ¹⁸⁰Ta^m. 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
Citations: PlumX Metrics

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. ^{133,134,135,136,137}Cs(n, γ), E=low; deduced Maxwellian averaged σ. Activation technique, comparison with previous results.

RADIOACTIVITY ¹³⁶Cs(β^-) [from ¹³⁵Cs(n, γ)]; measured T_1/2.

doi: 10.1103/PhysRevC.69.025803
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22846.

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
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22883.

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
Citations: PlumX Metrics

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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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
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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
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22879.

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, ^{147,148,149,150}Sm(n, γ), E=10, 25, 30 keV; compiled Maxwellian-averaged σ and its uncertainties.

doi: 10.1086/344718
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22829.

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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetG0030.

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, 130}Xe

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
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22816.

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
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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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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
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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
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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
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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 ¹⁸⁰Ta^m: 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.

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
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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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1997BU13      Nucl.Phys. A621, 431c (1997)

M.Busso, R.Gallino

s-Process Abundances in AGB Stars at Various Metallicities and Their Theoretical Interpretation

doi: 10.1016/S0375-9474(97)00285-6
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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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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, ^{58,59,60,61,62,63,64}Ni, ^63,64,65Cu, ^{64,65,66,67,68,70}Zn, ^69,71Ga, ^{70,71,72,73,74,76}Ge, ⁷⁵As, ^{76,77,78,79,80,82}Se, ^79,80,81Br, ^{80,81,82,83,84,85,86}Kr, ^85,86,87Rb, ^{86,87,88,89,90}Sr, ^89,90Y, ^{90,91,92,93,94,96}Zr(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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