Gravitino production from reheating in split supersymmetry
arXiv:hep-ph/0410169 · doi:10.1103/PhysRevD.71.043505
Abstract
We discuss gravitino production from reheating in models where the splitting between particle and sparticle masses can be larger than TeV, as naturally arising in the context of split supersymmetry. We show that such a production typically dominates over thermal contributions arising from the interactions of gauginos, squarks and sleptons. We constrain the supersymmetry breaking scale of the relevant sector for a given reheat temperature. However the situation changes when the gravitinos dominate the Universe and decay before nucleosynthesis. We briefly describe prospects for a successful baryogenesis and a viable neutralino dark matter in this case.
5 pages, RevTeX4, typos corrected, references added
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- Hierarchically Split Supersymmetry with Fayet-Iliopoulos D-terms in String Theory
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- Virtual effects of light gauginos and higgsinos: a precision electroweak analysis of split supersymmetry
- Non-Canonical Gauge Coupling Unification in High-Scale Supersymmetry Breaking
- Neutrino Mass from R-parity Violation in Split Supersymmetry
- Signals for CP Violation in Split Supersymmetry
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- Structure of split supersymmetry and simple models
- Hunting long-lived gluinos at the Pierre Auger Observatory
- Distinguishing split supersymmetry in Higgs signals at the Large Hadron Collider
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- Gravitino Thermal Production, Dark Matter, and Reheating of the Universe
- Vacuum Stability in Split Susy and Little Higgs Models
- Dilepton decays and oscillation of in split supersymmetry with R-parity violation
- Split Supersymmetry in Unified Models
- Reheating, thermalization and non-thermal gravitino production in MSSM inflation
- Heavy Gravitino and Split SUSY in the Light of BICEP2