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.
|Publication status||Published - 2010|
|Event||2010 Linear Collider Workshop, LCWS 2010 and International Linear Collider Meeting, ILC 2010 - Beijing, China|
Duration: Mar 26 2010 → Mar 30 2010
|Other||2010 Linear Collider Workshop, LCWS 2010 and International Linear Collider Meeting, ILC 2010|
|Period||3/26/10 → 3/30/10|
All Science Journal Classification (ASJC) codes
- Nuclear and High Energy Physics