How heavy can the Fermions in Split Susy be? A study on Gravitino and Extradimensional LSP
arXiv:hep-ph/0412103 · doi:10.1103/PhysRevD.71.103510
Abstract
In recently introduced Split Susy theories, in which the scale of Susy breaking is very high, the requirement that the relic abundance of the Lightest SuperPartner (LSP) provides the Dark Matter of the Universe leads to the prediction of fermionic superpartners around the weak scale. This is no longer obviously the case if the LSP is a hidden sector field, such as a Gravitino or an other hidden sector fermion, so, it is interesting to study this scenario. We consider the case in which the Next-Lightest SuperPartner (NLSP) freezes out with its thermal relic abundance, and then it decays to the LSP. We use the constraints from BBN and CMB, together with the requirement of attaining Gauge Coupling Unification and that the LSP abundance provides the Dark Matter of the Universe, to infer the allowed superpartner spectrum. As very good news for a possible detaction of Split Susy at LHC, we find that if the Gravitino is the LSP, than the only allowed NLSP has to be very purely photino like. In this case, a photino from 700 GeV to 5 TeV is allowed, which is difficult to test at LHC. We also study the case where the LSP is given by a light fermion in the hidden sector which is naturally present in Susy breaking in Extra Dimensions. We find that, in this case, a generic NLSP is allowed to be in the range 1-20 TeV, while a Bino NLSP can be as light as tens of GeV.
arXiv comment29 pages, 12 figures. v2: modified conclusions for bino NLSP. v3: corrected small mistake in Gauge Coupling Unification, conclusions unchanged
References in corpus (21)
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
- Big Bang Nucleosynthesis (in "The Review of Particle Properties" 2004)
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
- Heterotic and Type I String Dynamics from Eleven Dimensions
- The Cosmic Microwave Background Spectrum from the Full COBE/FIRAS Data Set
- Big-Bang Nucleosynthesis and Hadronic Decay of Long-Lived Massive Particles
- Aspects of Split Supersymmetry
- Hadronic Decay of Late-Decaying Particles and Big-Bang Nucleosynthesis
- Superweakly Interacting Massive Particles
- Updated Nucleosynthesis Constraints on Unstable Relic Particles
- SuperWIMP Dark Matter Signals from the Early Universe
- Did Something Decay, Evaporate, or Annihilate during Big Bang Nucleosynthesis?
- Supergravity with a Gravitino LSP
- Neutralinos, Big Bang Nucleosynthesis and 6Li in Low-Metallicity Stars
- Nucleon Decay Matrix Elements from Lattice QCD
- Dark Matter in the Finely Tuned Minimal Supersymmetric Standard Model
- Neutralino Dark Matter Detection in Split Supersymmetry Scenarios
- Almost No-Scale Supergravity
- DarkSUSY - A numerical package for supersymmetric dark matter calculations
- Precision Electroweak Tests of the Standard Model
- Multi-Megaton Water Cherenkov Detector for a Proton Decay Search -- TITAND
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- Dark Matter Constraints on Gaugino/Higgsino Masses in Split Supersymmetry and Their Implications at Colliders
- Supersymmetry for Fermion Masses
- Structure of split supersymmetry and simple models
- Dark Matter in split extended supersymmetry
- Gravitino dark matter from gluino late decay in split supersymmetry
- Infrared fixed point of the top Yukawa coupling in split supersymmetry
- Split Supersymmetry in Unified Models
- Vacuum Stability in Split Susy and Little Higgs Models
- Dilepton decays and oscillation of in split supersymmetry with R-parity violation
- Virtual Effects of Split SUSY in Higgs Productions at Linear Colliders
- Hierarchy from Baryogenesis