We analyze the simplest possible realization of the curvaton scenario, where a nearly scale-invariant spectrum of adiabatic perturbations is generated by conversion of an isocurvature perturbation generated during inflation, rather than the usual inflationary mechanism. We explicitly evaluate all the constraints on the model, under both the assumptions of prompt and delayed reheating, and we outline the viable parameter space
The curvaton and the inhomogeneous reheating scenarios for the generation of the cosmological curvat...
We discuss the potentially important role played by preheating in certain variants of the curvaton m...
In non-oscillatory (NO) inflationary models, the reheating mechanism was usually based on gravitatio...
We analyze the simplest possible realization of the curvaton scenario, where a nearly scale-invarian...
We analyze the simplest possible realization of the curvaton scenario, where a nearly scale-invarian...
We carry out a comprehensive analysis of the simplest curvaton model, which is based on two non-inte...
We analyze the curvaton scenario in the context of supersymmety. Supersymmetric theories contain man...
AbstractThe cosmological curvature perturbation may be generated when some ‘curvaton’ field, differe...
We consider a supersymmetric grand unified model which naturally solves the strong CP and mu problem...
We consider a supersymmetric grand unified model which naturally solves the strong CP and mu problem...
We consider a supersymmetric grand unified model which naturally solves the strong CP and mu problem...
The curvaton scenario for the generation of the cosmological curvature perturbation on large scales ...
Since a positive future detection of non-linearity in the cosmic microwave background anisotropy pat...
AbstractIn this Letter, we study a curvaton model where the curvaton is acted by Galileon field. We ...
We study the curvaton dynamics in brane-world cosmologies. Assuming that the inflaton field survives...
The curvaton and the inhomogeneous reheating scenarios for the generation of the cosmological curvat...
We discuss the potentially important role played by preheating in certain variants of the curvaton m...
In non-oscillatory (NO) inflationary models, the reheating mechanism was usually based on gravitatio...
We analyze the simplest possible realization of the curvaton scenario, where a nearly scale-invarian...
We analyze the simplest possible realization of the curvaton scenario, where a nearly scale-invarian...
We carry out a comprehensive analysis of the simplest curvaton model, which is based on two non-inte...
We analyze the curvaton scenario in the context of supersymmety. Supersymmetric theories contain man...
AbstractThe cosmological curvature perturbation may be generated when some ‘curvaton’ field, differe...
We consider a supersymmetric grand unified model which naturally solves the strong CP and mu problem...
We consider a supersymmetric grand unified model which naturally solves the strong CP and mu problem...
We consider a supersymmetric grand unified model which naturally solves the strong CP and mu problem...
The curvaton scenario for the generation of the cosmological curvature perturbation on large scales ...
Since a positive future detection of non-linearity in the cosmic microwave background anisotropy pat...
AbstractIn this Letter, we study a curvaton model where the curvaton is acted by Galileon field. We ...
We study the curvaton dynamics in brane-world cosmologies. Assuming that the inflaton field survives...
The curvaton and the inhomogeneous reheating scenarios for the generation of the cosmological curvat...
We discuss the potentially important role played by preheating in certain variants of the curvaton m...
In non-oscillatory (NO) inflationary models, the reheating mechanism was usually based on gravitatio...