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NSR database version of April 27, 2024.

Search: Author = S.Starrfield

Found 9 matches.

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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

2005ST25      Nucl.Phys. A758, 455c (2005)

S.Starrfield, W.R.Hix, F.X.Timmes, E.M.Sion, W.M.Sparks, S.J.Dwyer

Studies of Accretion onto Hot, Massive White Dwarfs: The Growth to the Chandrasekhar Limit?

doi: 10.1016/j.nuclphysa.2005.05.084
Citations: PlumX Metrics

2004SM08      Nucl.Phys. A746, 565c (2004)

M.S.Smith, W.R.Hix, S.Parete-Koon, L.Dessieux, Z.Ma, S.Starrfield, D.W.Bardayan, M.W.Guidry, D.L.Smith, J.C.Blackmon, A.Mezzacappa

Element synthesis calculations for stellar explosions: robust uncertainties, sensitivities, and radioactive ion beam measurements

doi: 10.1016/j.nuclphysa.2004.09.091
Citations: PlumX Metrics

2003HI14      Nucl.Phys. A718, 620c (2003)

W.R.Hix, M.S.Smith, S.Starrfield, A.Mezzacappa, D.L.Smith

Impact of Nuclear Reaction Rate Uncertainties on Nova Models

doi: 10.1016/S0375-9474(03)00904-7
Citations: PlumX Metrics

2003PA54      Astrophys.J. 598, 1239 (2003)

S.Parete-Koon, W.R.Hix, M.S.Smith, S.Starrfield, D.W.Bardayan, M.W.Guidry, A.Mezzacappa

A new ¹⁷F(p, γ)¹⁸Ne reaction rate and its implications for nova nucleosynthesis

NUCLEAR REACTIONS ¹⁷F(p, γ), E=low; analyzed data; deduced reaction rates, implications for nucleosynthesis in novae.

doi: 10.1086/378979
Citations: PlumX Metrics

2002IL05      Astrophys.J.Suppl.Ser. 142, 105 (2002)

Ch.Iliadis, A.Champagne, J.Jose, S.Starrfield, P.Tupper

The Effects of Thermonuclear Reaction-Rate Variations on Nova Nucleosynthesis: A Sensitivity Study

NUCLEAR REACTIONS ³He, ⁷Be, ¹⁵O(α, γ), ⁷Be, ⁸B, ^12,13C, ^13,14,15N, ^16,17,18O(p, γ), ¹⁵N, ¹⁷O, ^18,19F, ²³Na(p, α), ^17,18F, ^19,20,21,22Ne, ^21,22,23Na, ^23,24,25Mg(p, γ), E not given; calculated astrophysical abundances; deduced impact of σ and reaction rates uncertainties.

doi: 10.1086/341400
Citations: PlumX Metrics

2001IL02      Astrophys.J.Suppl.Ser. 134, 151 (2001)

C.Iliadis, J.M.D'Auria, S.Starrfield, W.J.Thompson, M.Wiescher

Proton-Induced Thermonuclear Reaction Rates for A = 20-40 Nuclei

NUCLEAR REACTIONS ^20,21,22Ne, ^20,21,22,23Na, ^{22,23,24,25,26}Mg, ^{23,24,25,26,27}Al, ^{26,27,28,29,30}Si, ^{27,28,29,30,31}P, ^{30,31,32,33,34}S, ^{31,32,33,34,35}Cl, ^34,35,36Ar, ^{35,36,37,38,39}K, ^39,40Ca(p, γ), E=low; ²³Na, ²⁷Al, ³¹P, ³⁵Cl, ³⁹K(p, α), E=low; compiled, analyzed astrophysical reaction rates.

doi: 10.1086/320364
Citations: PlumX Metrics

2001ST18      Nucl.Phys. A688, 110c (2001)

S.Starrfield, C.Iliadis, J.W.Truran, M.Wiescher, W.M.Sparks

Nuclear Reaction Rates and the Nova Outburst

NUCLEAR STRUCTURE ^12,13C, ^14,15N, ²²Na, ^26,27Al, ³²S; analyzed, surveyed astrophysical nuclear reaction rates; deduced nova luminosity, yields.

doi: 10.1016/S0375-9474(01)00679-0
Citations: PlumX Metrics

1997ST20      Nucl.Phys. A621, 495c (1997)

S.Starrfield, J.W.Truran, M.Wiescher, W.M.Sparks

Nova Nucleosynthesis

doi: 10.1016/S0375-9474(97)00296-0
Citations: PlumX Metrics