Heavy Right-Handed Neutrinos and Dark Matter in the CMSSM
arXiv:0909.3075 · doi:10.1103/PhysRevD.80.095015
Abstract
We perform a systematic study of the effects of the type-I seesaw mechanism on the dark matter abundance in the constrained supersymmetric standard model (CMSSM) which includes three right-handed neutrinos (the CMSSM). For large values of , we exploit the effects of large neutrino Yukawa couplings on the renormalization group (RG) evolution of the up-type Higgs. In particular, we show that the focus point scale can greatly exceed the electroweak scale resulting in the absence of a focus point region for which the relic density of neutralinos is within the range determined by WMAP. We also discuss the effects of the right-handed neutrinos on the so-called funnel region, where the relic density is controlled by s-channel annihilations through a heavy Higgs. For small values of , we discuss the possibility of sneutrino coannihilation regions with an emphasis on the suppression of the left-handed slepton doublet masses due to the neutrino Yukawa coupling. We consider two types of toy models consistent with either the normal or inverted hierarchy of neutrino masses.
18 pages, 7 figures, references and a footnote added, typos corrected
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- Constrained Supersymmetric Flipped SU(5) GUT Phenomenology
- Effects of Large Threshold Corrections in Supersymmetric Type-I Seesaw Model
- Examining leptogenesis with lepton flavor violation and the dark matter abundance
- Supersymmetric mass spectra and the seesaw scale
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- Focus Point Assisted by Right-Handed Neutrinos
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- Precise focus point scenario for a natural Higgs boson in the MSSM
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- Enhanced Tau Lepton Signatures at LHC in Constrained Supersymmetric Seesaw
- Constraining Affleck-Dine Leptogenesis after Thermal Inflation
- Shifted focus point of the Higgs mass parameter from the minimal mixed mediation of SUSY breaking
- Naturalness-guided Gluino Mass Bound from the Minimal Mixed Mediation of SUSY Breaking