云南大学中国西南天文研究所

 首页 Home | 研究所简介 SWIFAR | 人员 People | 科学研究 Science | 科研设备 Facilities | 学术活动 Activities | 人才培养 Education | 国际合作 Collaborations | 科学普及 Outreach | 诚聘英才 Recruitment | 访问指南 For Visitors 
 
 首页 Home 
 研究所简介 SWIFAR 
 人员 People 
 科学研究 Science 
 学术活动 Activities 
 人才培养 Education 
 科学普及 Outreach 
 诚聘英才 Recruitment 
 访问指南 For Visitors 
 内部链接 Internal 
 
  过往活动 Past Events
当前位置: 首页 Home>>过往活动 Past Events>>正文
 

Colloquium on Oct. 20, 2022

Structure of halos and its importance in gamma-ray search of DM


Speaker: Nagisa Hiroshima (Toyama University)

Venue: Video Conference

Time: 16:00 PM, Thursday, Oct. 20, 2022

Abstract:

Dark matter (DM) is a mysterious component of our Universe that occupies ~25% of the total energy density. Its nature is investigated in kinds of strategies, such as collider, direct detection, and indirect detection experiments. Among these, indirect search is powerful in probing signals from heavy DM of m>O(1)TeV. A precise understanding of the halo structure, which is a natural outcome of particle DM properties, is especially important when we extract information about DM from astrophysical observables. In this talk, I will overview the general strategies of indirect search focusing on the importance of the halo structure, and introduce recent ideas to better model halos.


Report PPT:  SWIFAR_Nagisa Hiroshima.pdf

附件【SWIFAR_Nagisa Hiroshima.pdf已下载
关闭窗口

版权所有:云南大学中国西南天文研究所 

South-Western Institute For Astronomy Research, YNU