Supersymmetric inflation and large-scale structure
ArXiv hep-ph/9610248 (1996)
Abstract:
In effective supergravity theories following from the superstring, a modulus field can quite naturally set the neccessary initial conditions for successful cosmological inflation to be driven by a hidden sector scalar field. The leading term in the scalar potential is {\em cubic} hence the spectrum of scalar density perturbations neccessarily deviates from scale-invariance, while the generation of gravitational waves is negligible. The growth of large-scale structure is then consistent with observational data assuming a critical density cold dark matter universe, with no need for a component of hot dark matter. The model can be tested thorough measurements of cosmic microwave background anisotropy on small angular scales.Leptophobic U(1)'s and the Rb-Rc anomalies.
Phys Rev D Part Fields 54:7 (1996) 4635-4647
O(d, d) symmetry in quantum cosmology
Nuclear Physics B Elsevier 477:2 (1996) 549-563
Quark and lepton mass matrices from horizontal U(1) symmetry
Physics Letters B Elsevier 387:1 (1996) 99-106