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arxiv: 1503.08749 · v2 · pith:J56KYTTNnew · submitted 2015-03-30 · ✦ hep-ph · astro-ph.CO· hep-th

Accidental Composite Dark Matter

classification ✦ hep-ph astro-ph.COhep-th
keywords modelstheoriescompositegaugegiveaccidentalcrossdark
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We build models where Dark Matter candidates arise as composite states of a new confining gauge force, stable thanks to accidental symmetries. Restricting to renormalizable theories compatible with SU(5) unification, we find 13 models based on SU(N) gauge theories and 9 based on SO(N). We also describe other models that require non-renormalizable interactions. The two gauge groups lead to distinctive phenomenologies: SU(N) theories give complex DM, with potentially observable electric and magnetic dipole moments that lead to peculiar spin-independent cross sections; SO(N) theories give real DM, with challenging spin-dependent cross sections or inelastic scatterings. Models with Yukawa couplings also give rise to spin-independent direct detection mediated by the Higgs boson and to electric dipole moments for the electron. In some models DM has higher spin. Each model predicts a specific set of lighter composite scalars, possibly observable at colliders.

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