Minimal Dark Matter

By Marco Cirelli, N. Fornengo, Alessandro Strumia. 2005

279 citations recorded by the source corpus.

Abstract A few multiplets that can be added to the SM contain a lightest neutral component which is automatically stable and provides allowed DM candidates with a non-standard phenomenology. Thanks to coannihilations, a successful thermal abundance is obtained for well defined DM masses. The best candidate seems to be a SU ( 2 ) L fermion quintuplet with mass 4.4 TeV, accompanied by a charged partner 166 MeV heavier with life-time 1.8 cm , that manifests at colliders as charged tracks disappearing in π ± with 97.7% branching ratio. The cross section for usual NC direct DM detection is σ SI = f 2 1.0 × 10 −43 cm 2 where f ∼ 1 is a nucleon matrix element. We study prospects for CC direct detection and for indirect detection.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/20dd1dcc000f6827f972780374d59616df8c403d

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In Astronomy and Astrophysics

  1. M. Redi
  2. Andrea Tesi
  3. A. Wulzer
  4. G. Panico
  5. R. Rattazzi
  6. Roberto Contino
  7. Jonathan L. Feng
  8. Alessandro Strumia

In Nuclear and High Energy Physics

  1. Cms Collaboration
  2. Atlas Collaboration
  3. Gudrun Heinrich
  4. A. Wulzer
  5. G. Panico
  6. M. Redi
  7. Andrea Tesi
  8. R. Rattazzi

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