Natural Dark Matter from Type I String Theory
arXiv:hep-ph/0608135 · doi:10.1088/1126-6708/2007/01/024
Abstract
We study neutralino dark matter within a semi-realistic type I string model, where supersymmetry breaking arises from F-terms of moduli fields parameterised in terms of Goldstino angles, which automatically gives rise to non-universal soft third sfamily and gaugino masses. We study the fine-tuning sensitivities for dark matter and electroweak symmetry breaking across the parameter space of the type I string model, and compare the results to a similar analysis in the non-universal MSSM. Within the type I string model we find that neutralino dark matter can be naturally implemented in the $\stau$ bulk region, the resonance region and the maximally tempered Bino/Wino/Higgsino region, in agreement with the results of the non-universal MSSM analysis. We also find that in the type I string model the ``well-tempered'' Bino/Wino region is less fine-tuned than in the MSSM, whereas the $\stau$ co-annihilation region exhibits a significantly higher degree of fine-tuning than in the MSSM.
22 pages, 5 figures
References in corpus (4)
Cited by in corpus (16)
- Compressed supersymmetry and natural neutralino dark matter from top squark-mediated annihilation to top quarks
- The MSSM with heavy scalars
- Natural Dark Matter in SUSY GUTs with Non-universal Gaugino Masses
- Diphoton decays of stoponium at the Large Hadron Collider
- Collider signals and neutralino dark matter detection in relic-density-consistent models without universality
- A New Measure of Fine Tuning
- Pseudo-Dirac Bino Dark Matter
- Exploring compressed supersymmetry with same-sign top quarks at the Large Hadron Collider
- Neutralino Dark Matter in the USSM
- The top squark-mediated annihilation scenario and direct detection of dark matter in compressed supersymmetry
- The Fine-Tuning Price of Neutralino Dark Matter in Models with Non-Universal Higgs Masses
- WIMP dark matter in bulk viscous non-standard cosmologies
- Spontaneous dark-matter mass generation along cosmological attractors in string theory
- FIMP Dark Matter in bulk viscous non-standard cosmologies
- Natural Dark Matter
- Natural SUSY Dark Matter: A Window on the GUT Scale