Multiple inflation
(1997)
Primordial Nucleosynthesis and Dark Matter
ArXiv astro-ph/9611232 (1996)
Abstract:
The cosmological abundance of nucleons determined from considerations of Big Bang nucleosynthesis allegedly provides compelling evidence for non-nucleonic dark matter. Recent developments in measurements of primordial light element abundances, in particular deuterium and helium, require reexamination of this important issue. The present situation is uncertain but exciting.Primordial Nucleosynthesis and Dark Matter
(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)