Recent years have seen the introduction of various multi-field inflationary scenarios in which the curvature and geodesics of the scalar manifold play a crucial role. We outline a simple description that unifies these different proposals and discuss their stability criteria. We demonstrate how the underlying dynamics is governed by an effective potential, whose critical points and bifurcations determine the late-time behaviour of the system, thus unifying hyperinflation, angular, orbital and side-tracked inflation. Interestingly, we show that hyperinflation is a special case of side-tracked inflation, relying on the enhanced isometries of the hyperbolic manifold. We provide the explicit coordinate transformation that maps the two models int...
We compute the covariant three-point function near horizon-crossing for a system of slowly-rolling s...
We re-examine the importance of slow-roll corrections during the evolution of cosmological perturbat...
We present a new class of two-field inflationary attractor models, known as shift-symmetric orbital ...
Recent years have seen the introduction of various multi-field inflationary scenarios in which the c...
Multi-field inflation with a curved scalar geometry has been found to support background trajectorie...
We explore the dynamics of multi-field models of inflation in which the field-space metric is a hype...
Recent years have seen the introduction of various multi-field inflationary scenarios, in which the ...
In this thesis, we focus on the dynamics and predictions of multi-field models of inflation. In the ...
In this thesis we study models of inflation with a curved field-space metric. We concern ourselves w...
International audienceHeavy scalar fields can undergo an instability during inflation as a result of...
We explore in detail the dynamics of multi-field inflationary models. We first revisit the two-field...
Inflation is currently the most promising paradigm of the Early Universe. The simple paradigm involv...
We study cosmological perturbations in two-field inflation, allowing for non-standard kinetic terms....
Multi-field inflation models include a variety of scenarios for how inflation proceeds and ends. Mod...
We compute the covariant three-point function near horizon-crossing for a system of slowly-rolling s...
We re-examine the importance of slow-roll corrections during the evolution of cosmological perturbat...
We present a new class of two-field inflationary attractor models, known as shift-symmetric orbital ...
Recent years have seen the introduction of various multi-field inflationary scenarios in which the c...
Multi-field inflation with a curved scalar geometry has been found to support background trajectorie...
We explore the dynamics of multi-field models of inflation in which the field-space metric is a hype...
Recent years have seen the introduction of various multi-field inflationary scenarios, in which the ...
In this thesis, we focus on the dynamics and predictions of multi-field models of inflation. In the ...
In this thesis we study models of inflation with a curved field-space metric. We concern ourselves w...
International audienceHeavy scalar fields can undergo an instability during inflation as a result of...
We explore in detail the dynamics of multi-field inflationary models. We first revisit the two-field...
Inflation is currently the most promising paradigm of the Early Universe. The simple paradigm involv...
We study cosmological perturbations in two-field inflation, allowing for non-standard kinetic terms....
Multi-field inflation models include a variety of scenarios for how inflation proceeds and ends. Mod...
We compute the covariant three-point function near horizon-crossing for a system of slowly-rolling s...
We re-examine the importance of slow-roll corrections during the evolution of cosmological perturbat...
We present a new class of two-field inflationary attractor models, known as shift-symmetric orbital ...