Decaying Dark Matter in the Supersymmetric Standard Model with Freeze-in and Seesaw mechanims
arXiv:1008.1621 · doi:10.1007/JHEP02(2011)035
Abstract
Inspired by the decaying dark matter (DM) which can explain cosmic ray anomalies naturally, we consider the supersymmetric Standard Model with three right-handed neutrinos (RHNs) and R-parity, and introduce a TeV-scale DM sector with two fields ϕ_{1,2} and a discrete symmetry. The DM sector only interacts with the RHNs via a very heavy field exchange and then we can explain the cosmic ray anomalies. With the second right-handed neutrino N_2 dominant seesaw mechanism at the low scale around 10^4 GeV, we show that ϕ_{1,2} can obtain the vacuum expectation values around the TeV scale, and then the lightest state from ϕ_{1,2} is the decay DM with lifetime around \sim 10^{26}s. In particular, the DM very long lifetime is related to the tiny neutrino masses, and the dominant DM decay channels to μand τare related to the approximate μ-τsymmetry. Furthermore, the correct DM relic density can be obtained via the freeze-in mechanism, the small-scale problem for power spectrum can be solved due to the decays of the R-parity odd meta-stable states in the DM sector, and the baryon asymmetry can be generated via the soft leptogensis.
24 pages,3 figures
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- The Dawn of FIMP Dark Matter: A Review of Models and Constraints
- Light Dark Matter from the U(1)_X Sector in the NMSSM with Gauge Mediation
- Neutrino Portal to FIMP Dark Matter with an Early Matter Era
- T(13) Flavor Symmetry and Decaying Dark Matter
- A Snowmass Whitepaper: Dark Matter Production at Intensity-Frontier Experiments