activity
20172020
most citedGeometrical destabilization, premature end of inflation and Bayesian model selection

35 citations · 58 across the 2 of their papers we have counts for

collaborators

8 papers

astro-ph.CO2020

Metric preheating and radiative decay in single-field inflation

Jérôme Martin, Theodoros Papanikolaou, Lucas Pinol +1

At the end of inflation, the inflaton oscillates at the bottom of its potential and these oscillations trigger a parametric instability for scalar fluctuations with wavelength

astro-ph.CO2019

The exponential tail of inflationary fluctuations: consequences for primordial black holes

Jose María Ezquiaga, Juan García-Bellido, Vincent Vennin

The curvature perturbations produced during an early era of inflation are known to have quasi-Gaussian distribution functions close to their maximum, where they are well constraine…

astro-ph.CO2019

Primordial black holes from the preheating instability

Jerome Martin, Theodoros Papanikolaou, Vincent Vennin

After the end of inflation, the inflaton field oscillates around a local minimum of its potential and decays into ordinary matter. These oscillations trigger a resonant instability…

astro-ph.CO2019

Stochastic inflation beyond slow roll

Chris Pattison, Vincent Vennin, Hooshyar Assadullahi +1

We study the stochastic formalism of inflation beyond the usual slow-roll approximation. We verify that the assumptions on which the stochastic formalism relies still hold even far…

astro-ph.CO2019

Inflation after Planck: Judgment Day

Debika Chowdhury, Jerome Martin, Christophe Ringeval +1

Inflation is considered as the best theory of the early universe by a very large fraction of cosmologists. However, the validity of a scientific model is not decided by counting th…

astro-ph.CO201923 cited

On backreaction effects in geometrical destabilisation of inflation

Oskar Grocholski, Marcin Kalinowski, Maciej Kolanowski +3

We study the geometrical instability arising in multi-field models of inflation with negatively-curved field space. We analyse how the homogeneous background evolves in presence of…