NSR Query Results

Output year order : Descending
Format : Normal

NSR database version of April 27, 2024.

Search: Author = D.D.Clayton

Found 8 matches.

Back to query form

2017CL05      Geochim.Cosmochim.Act. 221, 47 (2017)

D.D.Clayton, B.S.Meyer

Graphite grain-size spectrum and molecules from core-collapse supernovae

ATOMIC MASSES C, O; calculated abundances of carbon atomic complexes that emerge from the C + O cores of core-collapse supernovae.

doi: 10.1016/j.gca.2017.06.027
Citations: PlumX Metrics

1998TH07      Astrophys.J. 504, 500 (1998)

L.-S.The, D.D.Clayton, L.Jin, B.S.Meyer

Nuclear Reactions Governing the Nucleosynthesis of ⁴⁴Ti

NUCLEAR REACTIONS ⁴⁴Ti, ³⁶Ar, ⁴⁰Ca(α, p), ⁸Be, ⁴⁰Ca, ⁴⁴Ti, ¹²C, ³⁶Ar(α, γ), ⁴⁵V, ⁵⁷Ni, ⁵⁸Cu, ⁴⁴Ti, ⁵⁷Co(p, γ), ⁵⁷Co(p, n), ⁵⁷Ni(n, γ), ⁵⁴Fe(α, n), E not given; analyzed reaction rates influence on ⁴⁴Ti nucleosynthesis.

doi: 10.1086/306057
Citations: PlumX Metrics

1997CL04      Nucl.Phys. A621, 391c (1997)

D.D.Clayton, T.D.Krishnan, B.S.Meyer

Origin of ⁴⁸Ca

NUCLEAR STRUCTURE ⁴⁸Ca; analyzed reaction rates variation; deduced ⁴⁸Ca survival dependence on expansion type in nucleosynthesis.

doi: 10.1016/S0375-9474(97)00277-7
Citations: PlumX Metrics

1997JI04      Nucl.Phys. A621, 319c (1997)

L.Jin, B.S.Meyer, L.-S.The, D.D.Clayton

Nuclear Reaction Rates Governing the Nucleosynthesis of ⁴⁴Ti

NUCLEAR STRUCTURE ⁴⁴Ti; analyzed, surveyed nuclear reaction rates; deduced ⁴⁴Ti production dependence on certain reaction rates, astrophysical implication. Large reaction network.

doi: 10.1016/S0375-9474(97)00263-7
Citations: PlumX Metrics

1982KA39      Astrophys.J. 257, 821 (1982)

F.Kappeler, H.Beer, K.Wisshak, D.D.Clayton, R.L.Macklin, R.A.Ward

s-process studies in the light of new experimental cross sections - Distribution of neutron fluences and r-process residuals

COMPILATION ⁵⁸Fe, ⁷⁰Ge, ⁷⁶Se, ⁸²Kr, ⁹⁶Mo, ¹⁰⁰Ru, ¹⁰⁴Pd, ¹¹⁰Cd, ¹¹⁶Sn, ^122,123,124Te, ^128,130Xe, ^134,136Ba, ¹⁴²Nd, ^148,150Sm, ¹⁵⁴Gd, ¹⁶⁰Dy, ¹⁷⁰Yb, ¹⁷⁶Lu, ¹⁷⁶Hf, ¹⁸⁶Os, ¹⁹²Pt, ¹⁹⁸Hg, ²⁰⁴Pb, ^85,86Kr, ^85,86,87Rb, ^86,87,88Sr, ⁸⁹Y, ^90,91,92Zr, ¹³⁸Ba, ¹³⁹La, ¹⁴⁰Ce, ¹⁴¹Pr, ^206,207,208Pb, ²⁰⁹Bi(n, γ), E=30 keV; compiled experimental and theoretical (n, γ) Maxwellian-averaged σ and their uncertainties.

doi: 10.1086/160033
Citations: PlumX Metrics

1972WO05      Phys.Lett. 38B, 196 (1972)

S.W.Woosley, W.D.Arnett, D.D.Clayton

Astrophysical Importance of the Reaction ¹⁶O(p, α)¹³N

NUCLEAR REACTIONS ¹⁶O(p, α), E=5.2-6.7 MeV; calculated σ(E); analyzed astrophysical implications.

doi: 10.1016/0370-2693(72)90377-2
Citations: PlumX Metrics

1962CL04      Bull.Am.Phys.Soc. 7, No.7, 454, GA10 (1962)

D.D.Clayton

Energy Levels of N¹⁴ from N¹⁵(He³, α)N¹⁴

NUCLEAR STRUCTURE ¹⁵N; measured not abstracted; deduced nuclear properties.

1962CL12      Phys.Rev. 128, 2254 (1962)

D.D.Clayton

Energy Levels of N¹⁴ from N¹⁵(He³, α)N^14*

NUCLEAR STRUCTURE ¹⁵N; measured not abstracted; deduced nuclear properties.

doi: 10.1103/PhysRev.128.2254
Citations: PlumX Metrics