Goldilocks Supersymmetry: Simultaneous Solution to the Dark Matter and Flavor Problems of Supersymmetry
arXiv:0709.0297 · doi:10.1103/PhysRevLett.100.021302
Abstract
Neutralino dark matter is well motivated, but also suffers from two shortcomings: it requires gravity-mediated supersymmetry breaking, which generically violates flavor constraints, and its thermal relic density Ωis typically too large. We propose a simple solution to both problems: neutralinos freezeout with Ω~10-100, but then decay to ~1 GeV gravitinos, which are simultaneously light enough to satisfy flavor constraints and heavy enough to be all of dark matter. This scenario is naturally realized in high-scale gauge-mediation models, ameliorates small scale structure problems, and implies that ``cosmologically excluded'' models may, in fact, be cosmologically preferred.
4 pages; v2: references added; v3: published version
References in corpus (6)
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- Big Bang Nucleosynthesis Constraints on Hadronically and Electromagnetically Decaying Relic Neutral Particles
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Cited by in corpus (8)
- The WIMPless Miracle: Dark Matter Particles without Weak-scale Masses or Weak Interactions
- Gravitino Dark Matter and general neutralino NLSP
- The number density of a charged relic
- The Standard Model and Supersymmetric Flavor Puzzles at the Large Hadron Collider
- SUSY in the sky or a keV signature of sub-GeV gravitino dark matter
- Affleck-Dine Baryogenesis, Condensate Fragmentation and Gravitino Dark Matter in Gauge-Mediation with a Large Messenger Mass
- Building a Better mSUGRA: WIMP Dark Matter Without Flavor Violation
- R-invariant New Inflation Model vs Supersymmetric Standard Model