NSR Query Results


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NSR database version of May 21, 2024.

Search: Author = G.Magkotsios

Found 2 matches.

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2010BE40      J.Phys.:Conf.Ser. 202, 012023 (2010)

M.E.Bennett, R.Hirschi, M.Pignatari, S.Diehl, C.Fryer, F.Herwig, A.Hungerford, G.Magkotsios, G.Rockefeller, F.Timmes, M.Wiescher, P.Young

The effect of 12C + 12C rate uncertainties on s-process yields

NUCLEAR REACTIONS 12C(12C, p), (12C, α), E≈50-100 keV;23Na(p, α), E≈50-100 keV; calculated 12C burning rates. A≈12-96 calculated isotope yields based on these burning rates in massive stars for s-process.

doi: 10.1088/1742-6596/202/1/012023
Citations: PlumX Metrics


2010MA48      Astrophys.J.Suppl.Ser. 191, 66 (2010)

G.Magkotsios, F.X.Timmes, A.L.Hungerford, C.L.Fryer, P.A.Young, M.Wiescher

Trends in 44Ti and 56Ni from Core-collapse Supernovae

NUCLEAR REACTIONS 44Ti(α, p), (p, γ), 40Ca(α, γ), (α, p), 45V(p, γ), 17F(α, p), 21Na(α, p), 41,43Sc(p, γ), 57Ni(p, γ), E=344.6 - 861.7 keV; calculated yields; 44Ti, 56Ni; deduced mass fraction profile for core-collapse supernovae models.

doi: 10.1088/0067-0049/191/1/66
Citations: PlumX Metrics


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