String and M-Theory Cosmological Solutions with Ramond Forms
(1996)
Kinetic Mixing and the Supersymmetric Gauge Hierarchy
(1996)
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.Supersymmetric inflation and large-scale structure
(1996)
Leptophobic U(1)'s and the Rb-Rc anomalies.
Phys Rev D Part Fields 54:7 (1996) 4635-4647