Textures and Semi-Local Strings in SUSY Hybrid Inflation
arXiv:0807.1729 · doi:10.1088/1475-7516/2008/09/020
Abstract
Global topological defects may account for the large cold spot observed in the Cosmic Microwave Background. We explore possibilities of constructing models of supersymmetric F-term hybrid inflation, where the waterfall fields are globally SU(2)-symmetric. In contrast to the case where SU(2) is gauged, there arise Goldstone bosons and additional moduli, which are lifted only by masses of soft-supersymmetry breaking scale. The model predicts the existence of global textures, which can become semi-local strings if the waterfall fields are gauged under U(1)_X. Gravitino overproduction can be avoided if reheating proceeds via the light SU(2)-modes or right-handed sneutrinos. For values of the inflaton- waterfall coupling >=10^-4, the symmetry breaking scale imposed by normalisation of the power spectrum generated from inflation coincides with the energy scale required to explain the most prominent of the cold spots. In this case, the spectrum of density fluctuations is close to scale-invariant which can be reconciled with measurements of the power spectrum by the inclusion of the sub-dominant component due to the topological defects.
29 pages
References in corpus (45)
- Particle Physics Models of Inflation and the Cosmological Density Perturbation
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data
- Hybrid Inflation
- False Vacuum Inflation with Einstein Gravity
- Brane Inflation
- Resonant Leptogenesis
- Big-Bang Nucleosynthesis and Hadronic Decay of Long-Lived Massive Particles
- CP Violation and Baryogenesis due to Heavy Majorana Neutrinos
- Large Scale Structure and Supersymmetric Inflation without Fine Tuning
- Hadronic Decay of Late-Decaying Particles and Big-Bang Nucleosynthesis
- Electroweak-Scale Resonant Leptogenesis
- D-Term Inflation
- R Symmetry Breaking Versus Supersymmetry Breaking
- Hybrid Inflation from Supergravity D Terms
- The South Pole Telescope
- Inflation after WMAP3: Confronting the Slow-Roll and Exact Power Spectra with CMB Data
- The non-Gaussian Cold Spot in the 3-year WMAP data
- Fitting CMB data with cosmic strings and inflation
- Improved Results in Supersymmetric Electroweak Baryogenesis
- Inflation model constraints from the Wilkinson Microwave Anisotropy Probe three-year data
- Bounds on Cosmic Strings from WMAP and SDSS
- Effective number of neutrinos and baryon asymmetry from BBN and WMAP
- A Cosmic Microwave Background feature consistent with a cosmic texture
- Resonant τ-Leptogenesis with Observable Lepton Number Violation
- MSSM Electroweak Baryogenesis and Flavour Mixing in Transport Equations
- Mu Problem and Hybrid Inflation in Supersymmetric SU(2)_L x SU(2)_R x U(1)_B-L
- Constraints on Supersymmetric Models of Hybrid Inflation
- Semilocal Topological Defects
- The CMB cold spot: texture, cluster or void?
- Slow Roll Reconstruction: Constraints on Inflation from the 3 Year WMAP Dataset
- The Atacama Cosmology Telescope Project: A Progress Report
- Minimal Supersymmetric
- Anatomy of F_D-Term Hybrid Inflation
- WMAP constraints on inflationary models with global defects
- Blue Perturbation Spectra from Hybrid Inflation with Canonical Supergravity
- Cosmic microwave anisotropies from BPS semilocal strings
- Update of D3/D7-Brane Inflation on K3 x T^2/Z_2
- Cosmic Strings as the Source of Small-Scale Microwave Background Anisotropy
- Constraints on Brane Inflation and Cosmic Strings
- Semilocal Cosmic String Networks
- Prospects for ACT: simulations, power spectrum, and non-Gaussian analysis
- Observations of the Corona Borealis supercluster with the superextended Very Small Array: further constraints on the nature of the non-Gaussian CMB cold spot
- Constraining Modular Inflation in the MSSM from Giant Q-Ball Formation
- High Density Preheating Effects on Q-ball Decays and MSSM Inflation
- F_D-Term Hybrid Inflation with Electroweak-Scale Lepton Number Violation
Cited by in corpus (9)
- Vacuum Topology of the Two Higgs Doublet Model
- Tight constraints on F- and D-term hybrid inflation scenarios
- Cosmic String Power Spectrum, Bispectrum and Trispectrum
- SO and USp Kahler and Hyper-Kahler Quotients and Lumps
- Searching for Signatures of Cosmic String Wakes in 21cm Redshift Surveys using Minkowski Functionals
- Cosmic Strings and the Origin of Globular Clusters
- Effects of Cosmic String Velocities and the Origin of Globular Clusters
- Search for non-Gaussianities in the WMAP data with the Scaling Index Method
- Measuring CMB non-Gaussianity as a probe of Inflation and Cosmic Strings