Self-Interacting Dark Matter in the SU(3)C⊗ SU(3)L ⊗ U(1)N models

Details Self-Interacting Dark Matter in the SU(3)C⊗ SU(3)L ⊗ U(1)N models Self-Interacting Dark Matter in the SU(3)C⊗ SU(3)L ⊗ U(1)N models

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ap%26ss.305..225l&link_type=abstract

Astrophysics and Space Science, Volume 305, Issue 3, pp.225-233

Astronomy and Astrophysics

Astrophysics

Dark Matter, Extended Standard Model

Scientific paper

We present the gauge models based on SU(3)C⊗ SU(3)L ⊗ U(1)N (3-3-1) group which contain particles satisfying conditions for dark matter. There are two such models: one with exotic positive charged lepton and a variant with right-handed neutrinos. The scalar self-interacting dark matters are stable without imposing of new symmetry and should be weak-interacting.

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