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Astroparticle physics / Theoretical physics / Dark matter / Weakly interacting massive particles / Electron / XENON Dark Matter Search Experiment / Neutrino / Inelastic collision / Magnet / Physics / Particle physics / Exotic matter


Dark matter detection in two easy steps Maxim Pospelov,1, 2, ∗ Neal Weiner,3, † and Itay Yavin4, 2, ‡ 1 Department of Physics & Astronomy, University of Victoria, Victoria, BC, V8P 5C2, Canada Perimeter Institute f
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Document Date: 2013-12-05 20:17:26


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City

Waterloo / /

Company

iDM / /

Country

Canada / /

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Facility

University of Victoria / Canada Perimeter Institute / McMaster University / New York University / /

IndustryTerm

collision site / non-abelian force carrier / usual energy range / de-excitation energy / energy conservation / de-excitation energy falls / energy region / kinetic energy / transition energy / nuclear recoil energy / excitation energy / expected energy range / excited state energy / excited state kinetic energy / energy threshold / energy bin / energy resolution / given collision site / excited state recoil energy spectrum / search proposal / formidable tool / physical systems / energy / recoil energy / /

Organization

Department of Physics & Astronomy / New York University / New York / McMaster University / Canada Perimeter Institute for Theoretical Physics / Center for Cosmology and Particle Physics / University of Victoria / Victoria / Department of Physics / /

Person

Neal Weiner / Majorana / Ldark / /

Position

dark mediator / general model / local observer / /

Product

Monte-Carlo / /

ProvinceOrState

British Columbia / New York / Ontario / Victoria / /

Technology

x-ray / existing technology / simulation / recombination / /

SocialTag