理論セミナー

日時: 2014-09-30 11:00 - 12:00
場所: 研究本館1階会議室1
会議名: Dark Matter Structure Formation Simulations on K Supercomputer
連絡先: 高見 一、takami-AT-post.kek.jp
講演者: 石山 智明 氏  (筑波大学計算科学研究センター )
講演言語: 英語
アブストラクト: Smaller dark matter subhalos are more abundant in the Milky Way. The survivability of such subhalos in the Milky Way depends on their structure. This suggests that the structure of subhalos can determine the fine structure of the Milky Way halo. I report the results of high resolution cosmological simulations of very small scale structure formation peformed on K computer. I focus on the formation and evolution of dark matter halos near the free streaming scale, and their impact on the indirect dark matter detection experiments.

[index]