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NSR database version of April 26, 2024.

Search: Author = S.Bisterzo

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2017MA15      Phys.Lett. B 768, 1 (2017)

C.Massimi, S.Altstadt, J.Andrzejewski, L.Audouin, M.Barbagallo, V.Becares, F.Becvar, F.Belloni, E.Berthoumieux, J.Billowes, S.Bisterzo, D.Bosnar, M.Brugger, M.Calviani, F.Calvino, D.Cano-Ott, C.Carrapico, D.M.Castelluccio, F.Cerutti, E.Chiaveri, L.Cosentino, M.Chin, G.Clai, N.Colonna, G.Cortes, M.A.Cortes-Giraldo, S.Cristallo, M.Diakaki, C.Domingo-Pardo, I.Duran, R.Dressler, C.Eleftheriadis, A.Ferrari, P.Finocchiaro, K.Fraval, S.Ganesan, A.R.Garcia, G.Giubrone, I.F.Goncalves, E.Gonzalez-Romero, E.Griesmayer, C.Guerrero, F.Gunsing, A.Hernandez-Prieto, D.G.Jenkins, E.Jericha, Y.Kadi, F.Kappeler, D.Karadimos, N.Kivel, P.Koehler, M.Kokkoris, S.Kopecky, M.Krticka, J.Kroll, C.Lampoudis, C.Langer, E.Leal-Cidoncha, C.Lederer, H.Leeb, L.S.Leong, S.Lo Meo, R.Losito, A.Mallick, A.Manousos, J.Marganiec, T.Martinez, P.F.Mastinu, M.Mastromarco, E.Mendoza, A.Mengoni, P.M.Milazzo, F.Mingrone, M.Mirea, W.Mondelaers, A.Musumarra, C.Paradela, A.Pavlik, J.Perkowski, M.Pignatari, L.Piersanti, A.Plompen, J.Praena, J.M.Quesada, T.Rauscher, R.Reifarth, A.Riego, M.S.Robles, C.Rubbia, M.Sabate-Gilarte, R.Sarmento, A.Saxena, P.Schillebeeckx, S.Schmidt, D.Schumann, G.Tagliente, J.L.Tain, D.Tarrio, L.Tassan-Got, A.Tsinganis, S.Valenta, G.Vannini, I.Van Rijs, V.Variale, P.Vaz, A.Ventura, M.J.Vermeulen, V.Vlachoudis, R.Vlastou, A.Wallner, T.Ware, M.Weigand, C.Weiss, R.Wynants, T.Wright, P.Zugec

Neutron spectroscopy of ²⁶Mg states: Constraining the stellar neutron source ²²Ne(α, n)²⁵Mg

NUCLEAR REACTIONS ²⁵Mg(n, γ), (n, X), E<300 KeV; measured reaction products, En, In, Eγ, Iγ; deduced yields, σ, resonance parameters and corresponding excitation energies of the ²⁶Mg compound nucleus, Maxwellian-averaged cross sections, reaction rates for inverse reactions. R-matrix analysis of the experimental data.

doi: 10.1016/j.physletb.2017.02.025
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 dataset23327. Data from this article have been entered in the XUNDL database. For more information, click here.

2017UB01      Phys.Rev. C 95, 025803 (2017)

E.Uberseder, M.Heil, F.Kappeler, C.Lederer, A.Mengoni, S.Bisterzo, M.Pignatari, M.Wiescher

Stellar (n, γ) cross sections of ²³Na

NUCLEAR REACTIONS ²³Na(n, γ)²⁴Na, E=quasistellar thermal neutrons with kT=5.1-25 keV; measured neutron spectra, Eγ, Iγ, Maxwellian averaged σ(E) (MACS) by activation method using NaCl target at Karlsruhe Van de Graaff accelerator; σ(E) analyzed by R-matrix method using SAMMY code. Comparison with ENDF/B-VII.1 evaluation. Calculated relative s-abundance distribution at the end of C-shell burning with the MACS of ²³Na from the KADONIS database compilation, ratio of s-process yields.

doi: 10.1103/PhysRevC.95.025803
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 dataset23337.

2016HE06      Phys.Rev. C 93, 055807 (2016)

M.Heil, R.Plag, E.Uberseder, S.Bisterzo, F.Kappeler, A.Mengoni, M.Pignatari

Stellar neutron capture cross sections of ⁴¹K and ⁴⁵Sc

NUCLEAR REACTIONS ⁴⁵Sc, ⁴¹K(n, γ), kT=25 keV; measured Eγ, Iγ, capture cross section by activation method at Karlsruhe 3.7-MV Van de Graaff accelerator facility; deduced Maxwellian averaged cross sections (MACS) for the s-process nucleosynthesis yields in AGB stars and in massive stars. Comparison with previous experimental values and evaluated libraries JEFF-3.2, JENDL-4.0 and ENDF/B-VII.1. Discussed effect of neutron poisons in s-process scenario.

doi: 10.1103/PhysRevC.93.055807
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 dataset23306.

2016TA09      Phys.Rev. C 93, 055803 (2016)

R.Talwar, T.Adachi, G.P.A.Berg, L.Bin, S.Bisterzo, M.Couder, R.J.deBoer, X.Fang, H.Fujita, Y.Fujita, J.Gorres, K.Hatanaka, T.Itoh, T.Kadoya, A.Long, K.Miki, D.Patel, M.Pignatari, Y.Shimbara, A.Tamii, M.Wiescher, T.Yamamoto, M.Yosoi

Probing astrophysically important states in the ²⁶Mg nucleus to study neutron sources for the s process

NUCLEAR REACTIONS ²⁶Mg(α, α'), E=206 MeV; ²²Ne(⁶Li, d)²⁶Mg, E=82.3 MeV; measured Eα, Iα, E(d), I(d), σ(θ) using Grand Raiden (GR) spectrometer at RCNP-Osaka. ²⁶Mg; deduced α-unbound resonance energies, levels, J, π, α-spectroscopic factors, resonance strengths. Angular distributions for inelastic scattering analyzed by coupled channel code PTOLEMY and for transfer reactions by FRESCO code. ²²Ne(α, γ)²⁶Mg, ²²Ne(α, n)²⁵Mg, T₉=0.01-10; deduced astrophysical reaction rates from resonance parameters. Comparison with previous results. Relevance to slow neutron capture process (s process) in massive stars.

doi: 10.1103/PhysRevC.93.055803
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 datasetE2514. Data from this article have been entered in the XUNDL database. For more information, click here.

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.

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

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.

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

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.

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