Identification of new physics and general WIMP search at the ILC

M. Asano; K. Fujii; R. S. Hundi; H. Itoh; S. Matsumoto; N. Okada; T. Saito; T. Suehara; Y. Takubo; H. Yamamoto

Identification of new physics and general WIMP search at the ILC

M. Asano, K. Fujii, R. S. Hundi, H. Itoh, S. Matsumoto, N. Okada, T. Saito, T. Suehara, Y. Takubo, H. Yamamoto

研究成果: 会議への寄与タイプ › 学会誌 › 査読

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
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
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

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title = "Identification of new physics and general WIMP search at the ILC",

abstract = "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.",

author = "M. Asano and K. Fujii and Hundi, {R. S.} and H. Itoh and S. Matsumoto and N. Okada and T. Saito and T. Suehara and Y. Takubo and H. Yamamoto",

note = "Copyright: Copyright 2013 Elsevier B.V., All rights reserved.; 2010 Linear Collider Workshop, LCWS 2010 and International Linear Collider Meeting, ILC 2010 ; Conference date: 26-03-2010 Through 30-03-2010",

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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, T.

AU - Takubo, Y.

AU - Yamamoto, H.

PY - 2010

Y1 - 2010

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.

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M3 - Paper

AN - SCOPUS:84884635085

T2 - 2010 Linear Collider Workshop, LCWS 2010 and International Linear Collider Meeting, ILC 2010

Y2 - 26 March 2010 through 30 March 2010

ER -

Identification of new physics and general WIMP search at the ILC

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!!!All Science Journal Classification (ASJC) codes

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