We calculate the trispectrum of curvature perturbations for a model of inflation endowed with Galilean symmetry at the level of the fluctuations around an FRWbackground. Such a model has been shown to posses desirable properties such as non-renormalization of the leading operators. The cubic curvature fluctuations of this model produce quite distinct signatures at the level of the bispectrum. Our analysis shows how this holds true at higher order in perturbations. We provide a detailed study of the trispectrum shape-functions in different configurations and a comparison with existent literature. Most notably, predictions markedly differ from their P(X, \u3c6) counterpart in the so called equilateral trispectrum configuration
We compute the large scalar four-point correlation functions in general single field inflation model...
Abstract. Very few explicit inflationary scenarios are known to generate a large bis-pectrum of orth...
We compute the primordial trispectrum for curvature perturbations produced during cosmic inflation i...
Abstract. We calculate the trispectrum of curvature perturbations for a model of inflation endowed w...
We present a detailed study of the trispectrum of the curvature perturbation generated within a stab...
We perform the analysis of the trispectrum of curvature perturbations generated by the interactions ...
We study the consequences of imposing an approximate Galilean symmetry on the Effective Theory of In...
AbstractWe use the δN formalism to study the trispectrum Tζ of the primordial curvature perturbation...
We study the consequences of imposing an approximate Galilean symmetry on the Effective Theory of In...
We use the delta N-formalism to describe the leading order contributions to the primordial power spe...
Byrnes C, Sasaki M, Wands D. Primordial trispectrum from inflation. Phys.Rev.D. 2006;74(12): 123519....
We calculate the trispectrum of the primordial curvature perturbation generated by an epoch of slow-...
We compute the leading order contribution to the four-point function of the primordial curvature per...
Motivated by the interest in models of the early universe where statistical isotropy is broken and c...
The new Planck constraints on the local bispectrum parameter $f_{\rm NL}$ are about 105 times tight...
We compute the large scalar four-point correlation functions in general single field inflation model...
Abstract. Very few explicit inflationary scenarios are known to generate a large bis-pectrum of orth...
We compute the primordial trispectrum for curvature perturbations produced during cosmic inflation i...
Abstract. We calculate the trispectrum of curvature perturbations for a model of inflation endowed w...
We present a detailed study of the trispectrum of the curvature perturbation generated within a stab...
We perform the analysis of the trispectrum of curvature perturbations generated by the interactions ...
We study the consequences of imposing an approximate Galilean symmetry on the Effective Theory of In...
AbstractWe use the δN formalism to study the trispectrum Tζ of the primordial curvature perturbation...
We study the consequences of imposing an approximate Galilean symmetry on the Effective Theory of In...
We use the delta N-formalism to describe the leading order contributions to the primordial power spe...
Byrnes C, Sasaki M, Wands D. Primordial trispectrum from inflation. Phys.Rev.D. 2006;74(12): 123519....
We calculate the trispectrum of the primordial curvature perturbation generated by an epoch of slow-...
We compute the leading order contribution to the four-point function of the primordial curvature per...
Motivated by the interest in models of the early universe where statistical isotropy is broken and c...
The new Planck constraints on the local bispectrum parameter $f_{\rm NL}$ are about 105 times tight...
We compute the large scalar four-point correlation functions in general single field inflation model...
Abstract. Very few explicit inflationary scenarios are known to generate a large bis-pectrum of orth...
We compute the primordial trispectrum for curvature perturbations produced during cosmic inflation i...