Dark Matter Direct Detection in Electron Accelerators

Details Dark Matter Direct Detection in Electron Accelerators Dark Matter Direct Detection in Electron Accelerators

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..805..423s&link_type=abstract

PARTICLES, STRINGS, AND COSMOLOGY: 11th International Symposium on Particles, Strings, and Cosmology; PASCOS 2005. AIP Conferen

Other

Dark Matter

Scientific paper

We propose an alternative neutralino dark matter (DM) direct detection in electron accelerators. In this experiment, we count the number of electron recoil events by neutralinos in halo. If mass difference between selectron and neutralino is precisely measured in future collider experiments and it is small, the beam energy can be tuned to that. Then, scatterings are dominated by the resonant on-pole selectron exchange. If an electron accelerator can supply high current beams of O(100)A, the local DM density, the velocity dispersion and the DM wind due to a circular motion of the solar system can be measured when selectron and neutralino mass difference is O(10)%. This method is applicable to other DM candidates such as the lightest Kaluza-Klein particle in universal extra dimension models.

Affiliated with

Also associated with

No associations

Rating

Dark Matter Direct Detection in Electron Accelerators does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Dark Matter Direct Detection in Electron Accelerators, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dark Matter Direct Detection in Electron Accelerators will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1030328