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.
| 元の言語 | 英語 |
|---|---|
| 出版物ステータス | 出版済み - 12 1 2010 |
| 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 26 2010 → 3 30 2010 |
その他
| その他 | 2010 Linear Collider Workshop, LCWS 2010 and International Linear Collider Meeting, ILC 2010 |
|---|---|
| 国 | 中国 |
| 市 | Beijing |
| 期間 | 3/26/10 → 3/30/10 |
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All Science Journal Classification (ASJC) codes
- Nuclear and High Energy Physics
これを引用
Identification of new physics and general WIMP search at the ILC. / Asano, M.; Fujii, K.; Hundi, R. S.; Itoh, H.; Matsumoto, S.; Okada, N.; Saito, T.; Suehara, Taikan; Takubo, Y.; Yamamoto, H.
2010. 論文発表場所 2010 Linear Collider Workshop, LCWS 2010 and International Linear Collider Meeting, ILC 2010, Beijing, 中国.研究成果: 会議への寄与タイプ › 論文
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TY - CONF
T1 - Identification of new physics and general WIMP search at the ILC
AU - Asano, M.
AU - Fujii, K.
AU - Hundi, R. S.
AU - Itoh, H.
AU - Matsumoto, S.
AU - Okada, N.
AU - Saito, T.
AU - Suehara, Taikan
AU - Takubo, Y.
AU - Yamamoto, H.
PY - 2010/12/1
Y1 - 2010/12/1
N2 - 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.
AB - 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.
UR - http://www.scopus.com/inward/record.url?scp=84884635085&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=84884635085&partnerID=8YFLogxK
M3 - Paper
AN - SCOPUS:84884635085
ER -