Galactic and Cosmic Chemical Evolution with Hypernovae

Astronomy and Astrophysics – Astrophysics

Scientific paper

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6 pages, 3 figure. To appear in the Proceedings of the IAU Symposium 228 "From Li to U: Elemental Tracers of Early Cosmic Evol

Scientific paper

10.1017/S1743921305005880

We provide new nucleosynthesis yields depending on metallicity and energy (i.e., (normal supernovae and hypernovae), and show the evolution of heavy element abundances from C to Zn in the solar neighborhood. We then show the chemodynamical simulation of the Milky Way Galaxy and discuss the G-dwarf problem. We finally show the cosmological simulation and discuss the galaxy formation and chemical enrichment.

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