NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = C.Travaglio Found 17 matches. 2023KE10 Astrophys.J.Suppl.Ser. 268, 8 (2023) J.D.Keegans, M.Pignatari, R.J.Stancliffe, C.Travaglio, S.Jones, B.K.Gibson, D.M.Townsley, B.J.Miles, Ken J.Shen, G.Few Type Ia Supernova Nucleosynthesis: Metallicity-dependent Yields
doi: 10.3847/1538-4365/ace102
2022SC17 J.Phys.(London) G49, 110502 (2022) H.Schatz, A.D.Becerril Reyes, A.Best, E.F.Brown, K.Chatziioannou, K.A.Chipps, C.M.Deibel, R.Ezzeddine, D.K.Galloway, C.J.Hansen, F.Herwig, A.P.Ji, M.Lugaro, Z.Meisel, D.Norman, J.S.Read, L.F.Roberts, A.Spyrou, I.Tews, F.X.Timmes, C.Travaglio, N.Vassh, C.Abia, P.Adsley, S.Agarwal, M.Aliotta, W.Aoki, A.Arcones, A.Aryan, A.Bandyopadhyay, A.Banu, D.W.Bardayan, J.Barnes, A.Bauswein, T.C.Beers, J.Bishop, T.Boztepe, B.Cote, M.E.Caplan, A.E.Champagne, J.A.Clark, M.Couder, A.Couture, S.E.de Mink, S.Debnath, R.J.deBoer, J.den Hartogh, P.Denissenkov, V.Dexheimer, I.Dillmann, J.E.Escher, M.A.Famiano, R.Farmer, R.Fisher, C.Frohlich, A.Frebel, C.Fryer, G.Fuller, A.K.Ganguly, S.Ghosh, B.K.Gibson, T.Gorda, K.N.Gourgouliatos, V.Graber, M.Gupta, W.C.Haxton, A.Heger, W.R.Hix, W.C.G.Ho, E.M.Holmbeck, A.A.Hood, S.Huth, G.Imbriani, R.G.Izzard, R.Jain, H.Jayatissa, Z.Johnston, T.Kajino, A.Kankainen, G.G.Kiss, A.Kwiatkowski, M.La Cognata, A.M.Laird, L.Lamia, P.Landry, E.Laplace, K.D.Launey, D.Leahy, G.Leckenby, A.Lennarz, B.Longfellow, A.E.Lovell, W.G.Lynch, S.M.Lyons, K.Maeda, E.Masha, C.Matei, J.Merc, B.Messer, F.Montes, A.Mukherjee, M.R.Mumpower, D.Neto, B.Nevins, W.G.Newton, L.Q.Nguyen, K.Nishikawa, N.Nishimura, F.M.Nunes, E.O'Connor, B.W.O'Shea, W.-J.Ong, S.D.Pain, M.A.Pajkos, M.Pignatari, R.G.Pizzone, V.M.Placco, T.Plewa, B.Pritychenko, A.Psaltis, D.Puentes, Y.-Z.Qian, D.Radice, D.Rapagnani, B.M.Rebeiro, R.Reifarth, A.L.Richard, N.Rijal, I.U.Roederer, J.S.Rojo, J.S K, Y.Saito, A.Schwenk, M.L.Sergi, R.S.Sidhu, A.Simon, T.Sivarani, A.Skuladottir, M.S.Smith, A.Spiridon, T.M.Sprouse, S.Starrfield, A.W.Steiner, F.Strieder, I.Sultana, R.Surman, T.Szucs, A.Tawfik, F.Thielemann, L.Trache, R.Trappitsch, M.B.Tsang, A.Tumino, S.Upadhyayula, J.O.Valle Martinez, M.Van der Swaelmen, C.Viscasillas Vazquez, A.Watts, B.Wehmeyer, M.Wiescher, C.Wrede, J.Yoon, R.G.T.Zegers, M.A.Zermane, M.Zingale, the Horizon 2020 Collaborations Horizons: nuclear astrophysics in the 2020s and beyond
doi: https://dx.doi.org/10.1088/1361-6471/ac8890
2021GY02 J.Phys.(London) G48, 105202 (2021) G.Gyurky, Z.Halasz, G.G.Kiss, T.Szucs, R.Huszank, Z.Torok, Z.Fulop, T.Rauscher, C.Travaglio Measurement of the 91Zr(p, γ)92mNb cross section motivated by type Ia supernova nucleosynthesis NUCLEAR REACTIONS 91,96Zr(p, γ), E=1450-2800 keV; measured reaction products, Eγ, Iγ; deduced σ and uncertainties. Comparison with theoretical calculations.
doi: 10.1088/1361-6471/ac2132
2016PI06 Int.J.Mod.Phys. E25, 1630003 (2016) M.Pignatari, K.Gobel, R.Reifarth, C.Travaglio The production of proton-rich isotopes beyond iron: The γ-process in stars
doi: 10.1142/S0218301316300034
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
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
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
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
2003HI13 Nucl.Phys. A718, 229c (2003) W.Hillebrandt, J.C.Niemeyer, M.Reinecke, F.Ropke, C.Travaglio Multidimensional Simulations of Type Ia Supernova Explosions and Nucleosynthesis
doi: 10.1016/S0375-9474(03)00719-X
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
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
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
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
2001TR16 Nucl.Phys. A688, 396c (2001) C.Travaglio, A.Burkert, D.Galli Inhomogeneous Chemical Evolution of the Galactic Halo
doi: 10.1016/S0375-9474(01)00735-7
2001TR17 Nucl.Phys. A688, 442c (2001) C.Travaglio, D.Galli, S.Randich Galactic Evolution of 7Li: The interplay between Novae and AGB stars
doi: 10.1016/S0375-9474(01)00750-3
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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