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NSR database version of May 21, 2024.

Search: Author = C.Travaglio

Found 17 matches.

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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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD4417.


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
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 80,82,83,84,86Kr, 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
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 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
Citations: PlumX Metrics


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


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22829.


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22801.


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