Dark matter and cosmic-ray anomalies

• 高橋 史宜

  東大IPMU

抄録

After giving a review of recent cosmic-ray observations such as PAMELA, ATIC/PPB-BETS, Fermi and H.E.S.S, I explain what kind of conditions must be met if the PAMELA/Fermi excesses are due to dark matter. Finally I will give one dark matter model based on a Wino LSP with a tiny R-parity violation.

収録刊行物

• 素粒子論研究

  素粒子論研究 117 (6), F7-F13, 2010

  素粒子論グループ 素粒子論研究 編集部

詳細情報

• CRID: 1390001204069169664
• NII論文ID: 110007574522
• NII書誌ID: AN00135266
• DOI: 10.24532/soken.117.6_f7
• ISSN: 24332895
• ISSN: 03711838
• NDL書誌ID: 10568124
• Web Site: https://ndlsearch.ndl.go.jp/books/R000000004-I10568124
• 本文言語コード: en
• データソース種別:
  • JaLC
  • NDL
  • CiNii Articles
• 抄録ライセンスフラグ: 使用不可