Non-Sphericity/foreground effect on the dark matter halo estimation of dwarf spheroidal galaxies / 市川 幸史 氏

 
分類宇宙物理セミナー
開始2016/10/20(木)15:30
終了2016/10/20(木)16:30
会場研究本館1階会議室3
講演タイトルNon-Sphericity/foreground effect on the dark matter halo estimation of dwarf spheroidal galaxies
講演者市川 幸史 氏(カブリ数物連携連携宇宙機構)
言語英語/English
連絡先jwhite-AT-post.kek.jp
ウェブサイト
食堂・売店利用予定なし/0

概要

One of the most promising ways to detect dark matter is to look for its annihilation or decay products among cosmic-rays. Especially, it is found that quite strong constraints can be imposed by the gamma-ray measurements of dwarf spheroidal galaxies. However, recent studies reveal that these constraints are largely affected by the uncertainty of the dark matter halo density. In this talk, we will discuss the robustness of the dark matter halo estimation especially focusing on the effect of the non-sphericity and contamination of foreground stars.

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