We perform the analysis of the trispectrum of curvature perturbations generated by the interactions characterizing a general theory of single-field inflation obtained by effective field theory methods. We find that curvature-generated interaction terms, which can in general give an important contribution to the amplitude of the four-point function, show some new distinctive features in the form of their trispectrum shape-function. These interesting interactions are invariant under some recently proposed symmetries of the general theory and, as shown explicitly, do allow for a large value of the trispectrum
We compute the leading order contribution to the four-point function of the primordial curvature per...
We calculate the three-point correlation function evaluated at horizon crossing for a set of interac...
We compute the connected four point correlation function (the trispectrum in Fourier space) of cosmo...
We perform the analysis of the trispectrum of curvature perturbations generated by the interactions ...
The methods of effective field theory are used to study generic theories of inflation with a single ...
This is a version of the author's Ph.D. thesis. The methods of effective field theory are used to st...
We calculate the trispectrum of curvature perturbations for a model of inflation endowed with Galile...
Abstract. We calculate the trispectrum of curvature perturbations for a model of inflation endowed w...
We compute the large scalar four-point correlation functions in general single field inflation model...
We investigate non-Gaussianity in general multiple-field inflation using the formalism we developed ...
Motivated by the interest in models of the early universe where statistical isotropy is broken and c...
We derive semianalytic formulas for the local bispectrum and trispectrum from general two-field infl...
AbstractWe use the δN formalism to study the trispectrum Tζ of the primordial curvature perturbation...
Non-Gaussianities of the primordial density perturbations have emerged as a very powerful possible s...
We compute the connected four-point correlation function of the primordial curvature perturbation ge...
We compute the leading order contribution to the four-point function of the primordial curvature per...
We calculate the three-point correlation function evaluated at horizon crossing for a set of interac...
We compute the connected four point correlation function (the trispectrum in Fourier space) of cosmo...
We perform the analysis of the trispectrum of curvature perturbations generated by the interactions ...
The methods of effective field theory are used to study generic theories of inflation with a single ...
This is a version of the author's Ph.D. thesis. The methods of effective field theory are used to st...
We calculate the trispectrum of curvature perturbations for a model of inflation endowed with Galile...
Abstract. We calculate the trispectrum of curvature perturbations for a model of inflation endowed w...
We compute the large scalar four-point correlation functions in general single field inflation model...
We investigate non-Gaussianity in general multiple-field inflation using the formalism we developed ...
Motivated by the interest in models of the early universe where statistical isotropy is broken and c...
We derive semianalytic formulas for the local bispectrum and trispectrum from general two-field infl...
AbstractWe use the δN formalism to study the trispectrum Tζ of the primordial curvature perturbation...
Non-Gaussianities of the primordial density perturbations have emerged as a very powerful possible s...
We compute the connected four-point correlation function of the primordial curvature perturbation ge...
We compute the leading order contribution to the four-point function of the primordial curvature per...
We calculate the three-point correlation function evaluated at horizon crossing for a set of interac...
We compute the connected four point correlation function (the trispectrum in Fourier space) of cosmo...