A theory of evolution for the Universe requires both a mutation mechanism and a selection mechanism. We propose that both can be encountered in the stochastic approach to quantum cosmology. In Brans--Dicke chaotic inflation, the quantum fluctuations of Planck mass behave as mutations, such that new inflationary domains may contain values of Planck mass that differ slightly from their parent's. The selection mechanism establishes that the value of Planck mass should be such as to increase the proper volume of the inflationary domain, which will then generate more offsprings. For generic chaotic potentials we find runaway probability distributions that move towards large values of both inflaton and dilaton fields. Therefore, this mechani...
We propose a model of inflation driven by the relaxation of an initially Planckian cosmological cons...
We present a generic framework to compute the one-point statistics of cosmological perturbations, wh...
Quantum fluctuations of scalar fields during inflation could determine the very large-scale structur...
We propose a model of inflation driven by the relaxation of an initially Planckian cosmological cons...
Restricted Access.By the application of stochastic methods to a theory in which a potential V(ø) cau...
International audienceWe propose a model of inflation driven by the relaxation of an initially Planc...
This is the manuscript of my habilitation thesis, which was defended on the 30th of June 2020. It dr...
This is the manuscript of my habilitation thesis, which was defended on the 30th of June 2020. It dr...
This is the manuscript of my habilitation thesis, which was defended on the 30th of June 2020. It dr...
This is the manuscript of my habilitation thesis, which was defended on the 30th of June 2020. It dr...
This is the manuscript of my habilitation thesis, which was defended on the 30th of June 2020. It dr...
This is the manuscript of my habilitation thesis, which was defended on the 30th of June 2020. It dr...
This is the manuscript of my habilitation thesis, which was defended on the 30th of June 2020. It dr...
We propose a model of inflation driven by the relaxation of an initially Planckian cosmological cons...
We study two distinct aspects of the evolution of cosmological fluctuations. The first is the genera...
We propose a model of inflation driven by the relaxation of an initially Planckian cosmological cons...
We present a generic framework to compute the one-point statistics of cosmological perturbations, wh...
Quantum fluctuations of scalar fields during inflation could determine the very large-scale structur...
We propose a model of inflation driven by the relaxation of an initially Planckian cosmological cons...
Restricted Access.By the application of stochastic methods to a theory in which a potential V(ø) cau...
International audienceWe propose a model of inflation driven by the relaxation of an initially Planc...
This is the manuscript of my habilitation thesis, which was defended on the 30th of June 2020. It dr...
This is the manuscript of my habilitation thesis, which was defended on the 30th of June 2020. It dr...
This is the manuscript of my habilitation thesis, which was defended on the 30th of June 2020. It dr...
This is the manuscript of my habilitation thesis, which was defended on the 30th of June 2020. It dr...
This is the manuscript of my habilitation thesis, which was defended on the 30th of June 2020. It dr...
This is the manuscript of my habilitation thesis, which was defended on the 30th of June 2020. It dr...
This is the manuscript of my habilitation thesis, which was defended on the 30th of June 2020. It dr...
We propose a model of inflation driven by the relaxation of an initially Planckian cosmological cons...
We study two distinct aspects of the evolution of cosmological fluctuations. The first is the genera...
We propose a model of inflation driven by the relaxation of an initially Planckian cosmological cons...
We present a generic framework to compute the one-point statistics of cosmological perturbations, wh...
Quantum fluctuations of scalar fields during inflation could determine the very large-scale structur...