Right-handed sneutrinos as self-interacting dark matter in supersymmetric economical 3-3-1 model

Abstract

In this work we show that the supersymmetric economical SU(3)_C X SU(3)_L X U(1)_X (3-3-1) gauge model has a realistic candidate for self-interacting dark matter. In the model under consideration, the right-handed sneutrino is in bottom of the triplet, which is a singlet of the Standard Model SU(2)_L group. In addition, the right-handed sneutrino is the lightest slepton. By these properties, the right-handed sneutrino is weakly interacting with the Standard Model and stable without introduction of extra symmetry. From the Spergel-Steinhardt condition, the typical mass limit $\le 10$ MeV is derived. With self-interacting coupling constant fixed by supersymmetry, this limit is deduced without any approximation. The condition for thermal generated self-interacting dark matter in the Universe is also obtained.

16 pages

References in corpus (5)

• A Supersymmetry Primer
• Higgs Physics as a Window Beyond the MSSM (BMSSM)
• Higgs phenomenology of supersymmetric economical 3-3-1 model
• Sfermion masses in the supersymmetric economical 3-3-1 model
• Scalar sector of Supersymmetric $SU(3{)}_C\otimes SU(3{)}_L\otimes U(1{)}_N$ Model with right-handed neutrinos

Cited by in corpus (5)

• Constraining the Z' Mass in 331 Models using Direct Dark Matter Detection
• The right-handed sneutrino as thermal dark matter in U(1) extensions of the MSSM
• Scalar neutrino dark matter in $U(1{)}_X$SSM
• Higgs mass and right-handed sneutrino WIMP in a supersymmetric 3-3-1 model
• Sfermion masses in the supersymmetric economical 3-3-1 model