We review the Källén-Lehmann spectral representation in �at spacetime before moving on to de Sitter space. We compute one-loop corrections of de Sitter invariant two-point functions in the Lorentzian signature which are de�ned by the interacting Euclidean vacuum for scalar �elds with cubic interactions. These apply to all massive scalars in the complementary and principal series. Our investigations are motivated by the behaviour of the spectral density at the one-loop level whereby we can �nd a general expression relating the two-point function and the free propagators. Using well established techniques for treating quantum �elds in de Sitter, we compute the spectral density for speci�c cases, in both complementary and principal ser...
We propose an ansatz which solves the Dyson-Schwinger equation for the real scalar fields in Poincar...
The general boundary formulation of quantum theory is applied to quantize a real massive scalar fiel...
Quantization of a massive neutral scalar field without self-interaction defined on a space-time mani...
We examine long-wavelength correlation functions of massive scalar fields in de Sitter spacetime. F...
The study of quantum field theory in de Sitter spacetime is notably motivated by the success of infl...
We examine long-wavelength correlation functions of massive scalar fields in de Sitter spacetime. Fo...
We present a survey of rigourous quantization results obtained in recent works on quantum free field...
We investigate the propagation of arbitrarily coupled scalar fields on the $N$-dimensional hyperboli...
AbstractWe compute the four-point correlation function of a light O(N) scalar field in de Sitter spa...
We present a survey of rigourous quantization results obtained in recent works on quantum free field...
We obtain analytic results for the four-point amplitude, at one loop, of an interacting scalar field...
We compute the four-point correlation function of a light <math altimg="si1.gif" xmlns="http://www.w...
We consider light scalar fields during inflation and show how the stochastic spectral expansion meth...
We analyze the long distance behavior of the two-point functions for an interacting scalar O(N) mode...
We propose an ansatz which solves the Dyson-Schwinger equation for the real scalar fields in Poincar...
The general boundary formulation of quantum theory is applied to quantize a real massive scalar fiel...
Quantization of a massive neutral scalar field without self-interaction defined on a space-time mani...
We examine long-wavelength correlation functions of massive scalar fields in de Sitter spacetime. F...
The study of quantum field theory in de Sitter spacetime is notably motivated by the success of infl...
We examine long-wavelength correlation functions of massive scalar fields in de Sitter spacetime. Fo...
We present a survey of rigourous quantization results obtained in recent works on quantum free field...
We investigate the propagation of arbitrarily coupled scalar fields on the $N$-dimensional hyperboli...
AbstractWe compute the four-point correlation function of a light O(N) scalar field in de Sitter spa...
We present a survey of rigourous quantization results obtained in recent works on quantum free field...
We obtain analytic results for the four-point amplitude, at one loop, of an interacting scalar field...
We compute the four-point correlation function of a light <math altimg="si1.gif" xmlns="http://www.w...
We consider light scalar fields during inflation and show how the stochastic spectral expansion meth...
We analyze the long distance behavior of the two-point functions for an interacting scalar O(N) mode...
We propose an ansatz which solves the Dyson-Schwinger equation for the real scalar fields in Poincar...
The general boundary formulation of quantum theory is applied to quantize a real massive scalar fiel...
Quantization of a massive neutral scalar field without self-interaction defined on a space-time mani...