S317p.75 — Chemical evolution of r-process elements in the hierarchical galaxy formation

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Aug 4th at 6:00 PM until 6:00 PM

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Author(s): Yutaka Komiya1

Institution(s): 1. Tokyo University

In the concordance cosmology, galaxies are formed hierarchically. Metal-poor stars in the stellar halo are thought to be relics of stars formed in dwarf galaxies in the early universe. In order to investigate metal enrichment history in the early universe, we have been built the chemical evolution model with merger trees.
In this presentation, we show our results of chemical evolution computations for r-process elements. For the r-process elements, two possible astronomical sources have been proposed: supernova and coalescence of neutron star binary. Recent nucleosynthetic studies favor the neutron star merger scenario but previous chemical evolution studies pointed out difficulties. We discuss the origin of r-process elements using our hierarchical chemical evolution model.