In type IIB Fibre Inflation models the inflaton is a Kaehler 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.Comment: 5 pages + references, 3 figure
In brane inflationary scenarios, the cosmological perturbations are supposed to originate from the v...
We review conceptual aspects of inflationary scenarios able to produce primordial black holes, by am...
In Higgs-otic inflation a complex neutral scalar combination of the h0 0 and H0 0 MSSM Higgs f...
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...
In this work, we propose a string-inspired two fields inflation model to address the fine-tuning pro...
We revisit the framework of axion-like inflation in view of the possibility that the coupling of the...
In Starobinsky inflation with a Weyl squared Lagrangian $-\alpha C^2$, where $\alpha$ is a coupling ...
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...
We study an inflation model driven by a triplet of antisymmetric tensor fields, with minimal and non...
If the inflaton decays into several components during reheating, and if the corresponding decay rate...
Inflationary cosmology proposes that the early Universe undergoes accelerated expansion, driven, in ...
If gauge fields are coupled to an axion field during inflation, they can lead to unique observationa...
In brane inflationary scenarios, the cosmological perturbations are supposed to originate from the v...
In brane inflationary scenarios, the cosmological perturbations are supposed to originate from the v...
We review conceptual aspects of inflationary scenarios able to produce primordial black holes, by am...
In Higgs-otic inflation a complex neutral scalar combination of the h0 0 and H0 0 MSSM Higgs f...
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...
In this work, we propose a string-inspired two fields inflation model to address the fine-tuning pro...
We revisit the framework of axion-like inflation in view of the possibility that the coupling of the...
In Starobinsky inflation with a Weyl squared Lagrangian $-\alpha C^2$, where $\alpha$ is a coupling ...
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...
We study an inflation model driven by a triplet of antisymmetric tensor fields, with minimal and non...
If the inflaton decays into several components during reheating, and if the corresponding decay rate...
Inflationary cosmology proposes that the early Universe undergoes accelerated expansion, driven, in ...
If gauge fields are coupled to an axion field during inflation, they can lead to unique observationa...
In brane inflationary scenarios, the cosmological perturbations are supposed to originate from the v...
In brane inflationary scenarios, the cosmological perturbations are supposed to originate from the v...
We review conceptual aspects of inflationary scenarios able to produce primordial black holes, by am...
In Higgs-otic inflation a complex neutral scalar combination of the h0 0 and H0 0 MSSM Higgs f...