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 primordial curvature perturbation zeta may be generated by some curvaton field sigma, which is n...
We discuss the potentially important role played by preheating in certain variants of the curvaton m...
AbstractIn this Letter, we study a curvaton model where the curvaton is acted by Galileon field. We ...
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...
AbstractThe cosmological curvature perturbation may be generated when some ‘curvaton’ field, differe...
The curvaton scenario for the generation of the cosmological curvature perturbation on large scales ...
We analyze the curvaton scenario in the context of supersymmety. Supersymmetric theories contain man...
Since a positive future detection of non-linearity in the cosmic microwave background anisotropy pat...
AbstractWe present a mechanism for the origin of the large-scale curvature perturbation in our Unive...
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...
In non-oscillatory (NO) inflationary models, the reheating mechanism was usually based on gravitatio...
The primordial curvature perturbation zeta may be generated by some curvaton field sigma, which is n...
We discuss the potentially important role played by preheating in certain variants of the curvaton m...
AbstractIn this Letter, we study a curvaton model where the curvaton is acted by Galileon field. We ...
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...
AbstractThe cosmological curvature perturbation may be generated when some ‘curvaton’ field, differe...
The curvaton scenario for the generation of the cosmological curvature perturbation on large scales ...
We analyze the curvaton scenario in the context of supersymmety. Supersymmetric theories contain man...
Since a positive future detection of non-linearity in the cosmic microwave background anisotropy pat...
AbstractWe present a mechanism for the origin of the large-scale curvature perturbation in our Unive...
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...
In non-oscillatory (NO) inflationary models, the reheating mechanism was usually based on gravitatio...
The primordial curvature perturbation zeta may be generated by some curvaton field sigma, which is n...
We discuss the potentially important role played by preheating in certain variants of the curvaton m...
AbstractIn this Letter, we study a curvaton model where the curvaton is acted by Galileon field. We ...