报告题目：Galaxy formation in LCDM cosmologies

报 告 人：Guo Qi (NAOC)

报告时间：2014年3月20日（周四）13：30

报告地点：物理系三楼报告厅

报告摘要：The LCDM model has been successful in interpreting a wide range of observations. Structure formation in the gravitationally dominant dark matter distribution has been simulated reliably, thanks to the development of powerful parallel supercomputers, and is well understood within the standard cosmological paradigm. However, The formation of galaxy does not follow that of dark matter in a simple manner, and the observed galaxy data from large surveys cannot be compared to the CDM model properly without taken into account more complex baryonic processes. Here I will talk about some recent development in galaxy formation models in the context of LCDM cosmologies.