In type IIB fibre inflation models the inflation is a Kahler modulus which is kinetically coupled to the corresponding axion. In this setup the curvature of the field space induces tachyonic isocurvature perturbations normal to the background inflationary trajectory. However we argue that the associated instability is unphysical since it is due to the use of ill-defined entropy variables. In fact, upon using the correct relative entropy perturbation, we show that in fibre inflation axionic isocurvature perturbations decay during inflation and the dynamics is essentially single-field
We propose a natural inflation model driven by an imaginary or axionic component of a Kähler modulus...
The primordial curvature perturbation zeta may be generated by some curvaton field sigma, which is n...
We study the structure of multi-field inflation models where the primordial curvature perturbation i...
In type IIB fibre inflation models the inflation is a Kahler modulus which is kinetically coupled to...
In type IIB Fibre Inflation models the inflaton is a Kaehler modulus which is kinetically coupled to...
none3noWe perform a detailed analytical and numerical analysis of the multi-field evolution of Fibre...
The present work suggests that the isocurvature tension between axion and high energy inflationary s...
In brane inflationary scenarios, the cosmological perturbations are supposed to originate from the v...
We study the behaviour of isocurvature perturbations in non-linear sigma models which naturally emer...
In brane inflationary scenarios, the cosmological perturbations are supposed to originate from the v...
If the inflaton decays into several components during reheating, and if the corresponding decay rate...
We investigate the interplay between moduli dynamics and inflation, focusing on the Kachru-Kallosh-L...
We present a gauge-invariant formalism to study the evolution of the curvature and entropy perturbat...
International audienceWe study the development of entropy fluctuations in brane inflation in a warpe...
We study adiabatic (curvature) and entropy (isocurvature) perturbations produced during a period of ...
We propose a natural inflation model driven by an imaginary or axionic component of a Kähler modulus...
The primordial curvature perturbation zeta may be generated by some curvaton field sigma, which is n...
We study the structure of multi-field inflation models where the primordial curvature perturbation i...
In type IIB fibre inflation models the inflation is a Kahler modulus which is kinetically coupled to...
In type IIB Fibre Inflation models the inflaton is a Kaehler modulus which is kinetically coupled to...
none3noWe perform a detailed analytical and numerical analysis of the multi-field evolution of Fibre...
The present work suggests that the isocurvature tension between axion and high energy inflationary s...
In brane inflationary scenarios, the cosmological perturbations are supposed to originate from the v...
We study the behaviour of isocurvature perturbations in non-linear sigma models which naturally emer...
In brane inflationary scenarios, the cosmological perturbations are supposed to originate from the v...
If the inflaton decays into several components during reheating, and if the corresponding decay rate...
We investigate the interplay between moduli dynamics and inflation, focusing on the Kachru-Kallosh-L...
We present a gauge-invariant formalism to study the evolution of the curvature and entropy perturbat...
International audienceWe study the development of entropy fluctuations in brane inflation in a warpe...
We study adiabatic (curvature) and entropy (isocurvature) perturbations produced during a period of ...
We propose a natural inflation model driven by an imaginary or axionic component of a Kähler modulus...
The primordial curvature perturbation zeta may be generated by some curvaton field sigma, which is n...
We study the structure of multi-field inflation models where the primordial curvature perturbation i...