We develop a method for treating a series of secularly growing terms obtained from quantum perturbative calculations: autonomous first-order differential equations are constructed such that they reproduce this series to the given order. The exact solutions of these equations are free of secular terms and approach a finite limit at late times. This technique is illustrated for the well-known problem of secular growth of correlation functions of a massless scalar field with a quartic self-interaction in de Sitter space. For the expectation value of the product of two fields at coinciding space-time points, we obtain a finite late-time result that is very close to the one following from Starobinsky’s stochastic approach
Massless minimally coupled quantum scalar field with an asymmetric self interaction, $V(\phi)=\lambd...
We compute the renormalization group flow of <math altimg="si1.gif" xmlns="http://www.w3.org/1998/Ma...
We analyze the long distance behavior of the two-point functions for an interacting scalar O(N) mode...
We develop a method for treating a series of secularly growing terms obtained from quantum perturbat...
Abstract: Perturbative corrections to correlation functions for interacting theo-ries in de Sitter s...
Perturbative corrections to correlation functions for interacting theories in de Sitter spacetime of...
The study of cosmology draws us to the topic of quantum fields in curved space-time. In particular, ...
The study of quantum field theory in de Sitter spacetime is notably motivated by the success of infl...
We consider a theory of N self-interacting quantum scalar fields with quartic O(N)-symmetric potenti...
La cosmologie moderne amène à étudier la théorie quantique des champs en espace-temps courbe. Les ch...
AbstractWe compute the renormalization group flow of O(N) scalar field theories in de Sitter space u...
We revisit the issues of non-linear AdS stability, its relation to growing (secular) terms in näıve...
We examine long-wavelength correlation functions of massive scalar fields in de Sitter spacetime. F...
de Sitter spacetime plays a central role in modern (quantum) cosmology. Yet, there are various aspec...
We consider an $O(N)$ scalar field model with quartic interaction in $d$-dimensional Euclidean de Si...
Massless minimally coupled quantum scalar field with an asymmetric self interaction, $V(\phi)=\lambd...
We compute the renormalization group flow of <math altimg="si1.gif" xmlns="http://www.w3.org/1998/Ma...
We analyze the long distance behavior of the two-point functions for an interacting scalar O(N) mode...
We develop a method for treating a series of secularly growing terms obtained from quantum perturbat...
Abstract: Perturbative corrections to correlation functions for interacting theo-ries in de Sitter s...
Perturbative corrections to correlation functions for interacting theories in de Sitter spacetime of...
The study of cosmology draws us to the topic of quantum fields in curved space-time. In particular, ...
The study of quantum field theory in de Sitter spacetime is notably motivated by the success of infl...
We consider a theory of N self-interacting quantum scalar fields with quartic O(N)-symmetric potenti...
La cosmologie moderne amène à étudier la théorie quantique des champs en espace-temps courbe. Les ch...
AbstractWe compute the renormalization group flow of O(N) scalar field theories in de Sitter space u...
We revisit the issues of non-linear AdS stability, its relation to growing (secular) terms in näıve...
We examine long-wavelength correlation functions of massive scalar fields in de Sitter spacetime. F...
de Sitter spacetime plays a central role in modern (quantum) cosmology. Yet, there are various aspec...
We consider an $O(N)$ scalar field model with quartic interaction in $d$-dimensional Euclidean de Si...
Massless minimally coupled quantum scalar field with an asymmetric self interaction, $V(\phi)=\lambd...
We compute the renormalization group flow of <math altimg="si1.gif" xmlns="http://www.w3.org/1998/Ma...
We analyze the long distance behavior of the two-point functions for an interacting scalar O(N) mode...