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19982007
most citeds-Process Nucleosynthesis in Advanced Burning Phases of Massive Stars

143 citations · 250 across the 4 of their papers we have counts for

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astro-ph200763 cited

r-Process Nucleosynthesis in Shocked Surface Layers of O-Ne-Mg Cores

H. Ning, Y. -Z. Qian, B. S. Meyer

We demonstrate that rapid expansion of the shocked surface layers of an O-Ne-Mg core following its collapse can result in r-process nucleosynthesis. As the supernova shock accelera…

astro-ph2006143 cited

s-Process Nucleosynthesis in Advanced Burning Phases of Massive Stars

Lih-Sin The, Mounib F. El Eid, Bradley S. Meyer

We present a detailed study of s-process nucleosynthesis in massive stars of solar-like initial composition and masses 15, 20,25, and 30 Msun. We update our previous results of s-p…

astro-ph2006

Are Ti44-Producing Supernovae Exceptional?

L. -S. The, D. D. Clayton, R. Diehl +6

According to standard models supernovae produce radioactive Ti, which should be visible in gamma-rays following decay to Ca for a few centuries. $^{44}Ti production i…

astro-ph2004

Evolution of Massive Stars Up to the End of Central Oxygen Burning

Mounib F. El Eid, Bradley S. Meyer, Lih-Sin The

We present a detailed study of the evolution of massive stars of masses 15, 20, 25 and 30 $\msun$ assuming solar-like initial chemical composition. The stellar sequences were evolv…

astro-ph2004

Nucleosynthesis in Fast Expansions of High-Entropy, Proton Rich Matter

G. C. Jordan, B. S. Meyer

We demonstrate that nucleosynthesis in rapid, high-entropy expansions of proton-rich matter from high temperature and density can result in a wider variety of abundance patterns th…

astro-ph2002

The r-Process without Excess Neutrons

Bradley S. Meyer

The r-process of nucleosynthesis requires a large neutron-to-seed nucleus ratio. This does not, however, that there be an excess of neutrons over protons. If the expansion of the m…