NSR Query Results
Output year order : Descending NSR database version of April 25, 2024. Search: Author = R.D.Hoffman Found 18 matches. 2010CY01 Astrophys.J.Suppl.Ser. 189, 240 (2010) R.H.Cyburt, A.M.Amthor, R.Ferguson, Z.Meisel, K.Smith, S.Warren, A.Heger, R.D.Hoffman, T.Rauscher, A.Sakharuk, H.Schatz, F.K.Thielemann, M.Wiescher The JINA REACLIB Database: Its Recent Updates and Impact on Type-I X-ray Bursts
doi: 10.1088/0067-0049/189/1/240
2007FO04 Phys.Rev. C 75, 055807 (2007) C.Forssen, F.S.Dietrich, J.Escher, R.D.Hoffman, K.Kelley Determining neutron capture cross sections via the surrogate reaction technique NUCLEAR REACTIONS Zr(n, γ), E< 5 MeV; calculated cross sections and neutron tranmission coefficients using the surrogate method. Discussed astrophysical implications.
doi: 10.1103/PhysRevC.75.055807
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
2005FO11 Nucl.Phys. A758, 130c (2005) C.Forssen, L.Ahle, L.A.Bernstein, J.A.Church, F.S.Dietrich, J.Escher, R.D.Hoffman Theoretical challenges of determining low-energy neutron-capture cross sections via the Surrogate Technique
doi: 10.1016/j.nuclphysa.2005.05.026
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
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
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
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
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
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
Back to query form |