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NSR database version of April 27, 2024.

Search: Author = T.A.Weaver

Found 6 matches.

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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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

1972BA14      Nucl.Phys. A181, 453 (1972)

A.D.Bacher, E.A.McClatchie, M.S.Zisman, T.A.Weaver, T.A.Tombrello

Observation of the 14 MeV Resonance in ¹²C(p, p)¹²C with Molecular Ion Beams

NUCLEAR REACTIONS ¹²C(p, p), E=14.2 MeV; measured σ(E), θ(lab)=165°. ¹³N deduced change in resonance shape of lowest T=3/2 level due to molecular ion beams.

doi: 10.1016/0375-9474(72)90495-2
Citations: PlumX Metrics

1971CO27      Nucl.Phys. A175, 300 (1971)

R.G.Couch, H.Spinka, T.A.Tombrello, T.A.Weaver

Total Cross-Section Measurements for ¹⁴N(α, γ)¹⁸F

NUCLEAR REACTIONS ¹⁴N(α, γ), E=0.5-1.2 MeV; measured σ(E). ¹⁸F deduced resonances, resonance parameters. Natural target.

doi: 10.1016/0375-9474(71)90284-3
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2779.