NSR Query Results
Output year order : Descending NSR database version of March 21, 2024. Search: Author = S.E.Woosley Found 27 matches. 2015BU08 Phys.Rev.Lett. 114, 251102 (2015) B.Bucher, X.D.Tang, X.Fang, A.Heger, S.Almaraz-Calderon, A.Alongi, A.D.Ayangeakaa, M.Beard, A.Best, J.Browne, C.Cahillane, M.Couder, R.J.deBoer, A.Kontos, L.Lamm, Y.J.Li, A.Long, W.Lu, S.Lyons, M.Notani, D.Patel, N.Paul, M.Pignatari, A.Roberts, D.Robertson, K.Smith, E.Stech, R.Talwar, W.P.Tan, M.Wiescher, S.E.Woosley First Direct Measurement of 12C(12C, n)23Mg at Stellar Energies NUCLEAR REACTIONS 12C(12C, n), E=7.5, 9.5 MeV; measured reaction products, Eγ, Iγ, En, In; deduced yields, S-factors, astrophysical reaction rate. Comparison with available data.
doi: 10.1103/PhysRevLett.114.251102
2007BY02 Phys.Rev.Lett. 98, 082501 (2007) A.Byelikov, T.Adachi, H.Fujita, K.Fujita, Y.Fujita, K.Hatanaka, A.Heger, Y.Kalmykov, K.Kawase, K.Langanke, G.Martinez-Pinedo, K.Nakanishi, P.von Neumann-Cosel, R.Neveling, A.Richter, N.Sakamoto, Y.Sakemi, A.Shevchenko, Y.Shimbara, Y.Shimizu, F.D.Smit, Y.Tameshige, A.Tamii, S.E.Woosley, M.Yosoi Gamow-Teller Strength in the Exotic Odd-Odd Nuclei 138La and 180Ta and Its Relevance for Neutrino, Nucleosynthesis NUCLEAR REACTIONS 138Ba, 180Hf(3He, t), E=140 MeV/nucleon; measured particle spectra. 138La, 180Ta deduced Gamow-Teller strength distributions. Implications for stellar nucleosynthesis discussed.
doi: 10.1103/PhysRevLett.98.082501
2007WO10 Nat.Phys. 3, 832 (2007) Nuclear astrophysics: The first 50 years
doi: 10.1038/nphys804
2006PR12 Astrophys.J. 644, 1028 (2006) J.Pruet, R.D.Hoffman, S.E.Woosley, H.-T.Janka, R.Buras Nucleosynthesis in early supernova winds. II. The role of neutrinos
doi: 10.1086/503891
2005HE02 Phys.Lett. B 606, 258 (2005) A.Heger, E.Kolbe, W.C.Haxton, K.Langanke, G.Martinez-Pinedo, S.E.Woosley Neutrino nucleosynthesis
doi: 10.1016/j.physletb.2004.12.017
2005PR19 Astrophys.J. 623, 325 (2005) J.Pruet, S.E.Woosley, R.Buras, H.-T.Janka, R.D.Hoffman Nucleosynthesis in the hot convective bubble in core-collapse supernovae
doi: 10.1086/428281
2003HE16 Nucl.Phys. A718, 159c (2003) A.Heger, S.E.Woosley, K.Langanke, E.Kolbe, T.Rauscher, R.D.Hoffman Nucleosynthesis of heavy elements in massive stars
doi: 10.1016/S0375-9474(03)00708-5
2003PR06 Astrophys.J. 586, 1254 (2003) J.Pruet, S.E.Woosley, R.D.Hoffman Nucleosynthesis in gamma-ray burst accretion disks
doi: 10.1086/367957
2003RA40 Nucl.Phys. A718, 463c (2003) T.Rauscher, A.Heger, R.D.Hoffman, S.E.Woosley Hydrostatic and Explosive Nucleosynthesis in Massive Stars Using Improved Nuclear and Stellar Physics
doi: 10.1016/S0375-9474(03)00852-2
2003WO09 Nucl.Phys. A718, 3c (2003) S.E.Woosley, A.Heger, T.Rauscher, R.D.Hoffman Nuclear Data Needs for the Study of Nucleosynthesis in Massive Stars
doi: 10.1016/S0375-9474(03)00673-0
2002RA44 Astrophys.J. 576, 323 (2002) T.Rauscher, A.Heger, R.D.Hoffman, S.E.Woosley Nucleosynthesis in Massive Stars with Improved Nuclear and Stellar Physics
doi: 10.1086/341728
2001HE20 Nucl.Phys. A688, 197c (2001) A.Heger, I.Baraffe, C.L.Fryer, S.E.Woosley Evolution and Nucleosynthesis of Very Massive Primordial Stars
doi: 10.1016/S0375-9474(01)00697-2
2001HO11 Astrophys.J. 549, 1085 (2001) R.D.Hoffman, S.E.Woosley, T.A.Weaver Nucleosynthesis Below A = 100 in Massive Stars
doi: 10.1086/319463
2001HO21 Nucl.Phys. A688, 481c (2001) R.D.Hoffman, S.E.Woosley, T.A.Weaver Nucleosynthesis Below A = 100 in Massive Stars
doi: 10.1016/S0375-9474(01)00762-X
2001RA23 Nucl.Phys. A688, 193c (2001) T.Rauscher, A.Heger, R.D.Hoffman, S.E.Woosley Nucleosynthesis in Massive Stars Revisited
doi: 10.1016/S0375-9474(01)00696-0
2001WO08 Nucl.Phys. A688, 9c (2001) Models for Type Ia Supernovae
doi: 10.1016/S0375-9474(01)00659-5
1999HO26 Astrophys.J. 521, 735 (1999) R.D.Hoffman, S.E.Woosley, T.A.Weaver, T.Rauscher, F.-K.Thielemann The Reaction Rate Sensitivity of Nucleosynthesis in Type II Supernovae NUCLEAR REACTIONS 32S, 39K, 45,46Ca, 50V, 69,70Zn(n, γ), 33S, 43Ca, 44Sc(p, γ), 33S, 40K, 45Ti(n, α), 40K, 45Ti(n, p), 44Ti(α, p), 24Mg, 28Si, 32S, 36Ar, 40Ca, 44Ti(α, γ), E not given; analyzed stellar reactions rates. Several libraries compared.
doi: 10.1086/307568
1997HA36 Nucl.Phys. A621, 83c (1997) D.H.Hartmann, P.Predehl, J.Greiner, R.Egger, J.Trumper, B.Ashenbach, A.F.Iyudin, R.D.Diehl, U.Oberlack, V.Schonfelder, M.D.Leising, L.-S.The, F.X.Timmes, S.E.Woosley, R.Hoffman, N.Langer, G.Garcia-Segura On Flamsteed's Supernova Cas A
doi: 10.1016/S0375-9474(97)00217-0
1997HO10 Nucl.Phys. A621, 397c (1997) R.D.Hoffman, S.E.Woosley, Y.-Z.Qian Model Independent r-Process Nucleosynthesis - Constraints on the Key Parameters
doi: 10.1016/S0375-9474(97)00278-9
1997LA24 Nucl.Phys. A621, 457C (1997) N.Langer, J.Fliegner, A.Heger, S.E.Woosley Nucleosynthesis in Rotating Massive Stars
doi: 10.1016/S0375-9474(97)00290-X
1997WO07 Nucl.Phys. A621, 445c (1997) S.E.Woosley, R.D.Hoffman, F.X.Timmes, T.A.Weaver, F.-K.Thielemann Nucleosynthesis in Massive Stars and Supernovae
doi: 10.1016/S0375-9474(97)00288-1
1996WO09 Nucl.Phys. A606, 137 (1996) Making Black Holes in Supernovae
doi: 10.1016/0375-9474(96)00235-7
1994WO06 Astrophys.J. 433, 229 (1994) S.E.Woosley, J.R.Wilson, G.J.Mathews, R.D.Hoffman, B.S.Meyer The r-Process and Neutrino-Heated Supernova Ejecta
doi: 10.1086/174638
1992WO15 Astrophys.J. 395, 202 (1992) The α-Process and the r-Process NUCLEAR STRUCTURE A=80-100; analyzed reaction data; deduced α-, r-processes role.
doi: 10.1086/171644
1979WO07 At.Data Nucl.Data Tables 22, 371 (1979) S.E.Woosley, W.A.Fowler, J.A.Holmes, B.A.Zimmerman Semiempirical Thermonuclear Reaction-Rate Data for Intermediate-Mass Nuclei COMPILATION A=16-74; compiled, evaluated available semiempirical thermonuclear reaction data. Parametrized analytic formulas.
doi: 10.1016/0092-640X(78)90018-9
1977DA07 Nucl.Phys. A279, 70 (1977) R.Dayras, Z.E.Switkowski, S.E.Woosley Neutron Branching in the Reaction 12C + 12C NUCLEAR REACTIONS 12C(12C, n), E=3.54-4.94 MeV; measured σ(E); deduced neutron branching ratio. Activation technique. Discussed in context of hydrostatic carbon burning.
doi: 10.1016/0375-9474(77)90421-3
1976MA02 Nucl.Phys. A256, 163 (1976) F.M.Mann, D.W.Kneff, Z.E.Switkowski, S.E.Woosley A Study of the 23Na+p Reactions to Determine 23Mg Consumption in Stars NUCLEAR REACTIONS 23Na(p, p'), (p, α0), E=5.05-6.2 MeV; measured σ(θ). 23Na(p, n), E=5.05-11.5 MeV; measured σ; deduced reaction rates for 23Mg+n.
doi: 10.1016/0375-9474(76)90101-9
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