抄録
We investigate the possibility of the identification of TeV physics models including WIMP dark matter at the International Linear Collider. Many TeV physics models contain a WIMP dark matter (χ°) and charged new particle (χ±) which interacts with the WIMP dark matter via the vertex χ± χ°W+. Through Monte Carlo simulations, we study the process, e+e- → x+X- → χ°χ°W+W-, because the signal contains the fruitful information of the model. We show that, in particular, the distribution of the X± production angle is the powerful probe in the TeV physics model search.
本文言語 | 英語 |
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出版ステータス | 出版済み - 2010 |
外部発表 | はい |
イベント | 2010 Linear Collider Workshop, LCWS 2010 and International Linear Collider Meeting, ILC 2010 - Beijing, 中国 継続期間: 3月 26 2010 → 3月 30 2010 |
その他
その他 | 2010 Linear Collider Workshop, LCWS 2010 and International Linear Collider Meeting, ILC 2010 |
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国/地域 | 中国 |
City | Beijing |
Period | 3/26/10 → 3/30/10 |
!!!All Science Journal Classification (ASJC) codes
- 核物理学および高エネルギー物理学