41 pages, 7 figures, 2 appendices. Added some clarifications and comments, additional references, to appear in JCAPInternational audienceModifications of the initial-state of the inflaton field can induce a departure from Gaussianity and leave a testable imprint on the higher order correlations of the CMB and large scale structures in the Universe. We focus on the bispectrum statistics of the primordial curvature perturbation and its projection on the CMB. For a canonical single-field action the three-point correlator enhancement is localized, maximizing in the collinear limit, corresponding to enfolded or squashed triangles in comoving momentum space. We show that the available local and equilateral template are very insensitive to this lo...
Over thirty years since an early epoch of inflation was proposed as an elegant way solution to the B...
We argue that a plausible operational definition for an initial state of the universe is the initial...
We consider a primordial SU(2) vector multiplet during inflation in models where quantum fluctuation...
41 pages, 7 figures, 2 appendices. Added some clarifications and comments, additional references, to...
If time-dependent disruptions from slow-roll occur during inflation, the correlation functions of th...
We calculate the bispectrum of the Cosmic Microwave Background (CMB) temperature anisotropies induce...
Deviations from the Bunch-Davies vacuum during an inflationary period can leave a testable imprint o...
Until recently our knowledge of the primordial curvature perturbation was relatively modest. Ever si...
We revisit the predictions for the expected cosmic microwave background bispectrum signal from the c...
In this short note we translate the best available observational bounds on the CMB bispectrum amplit...
We present measurements of the dark matter bispectrum in N-body simulations with non-Gaussian initia...
In order to gain new insights into the gauge field couplings in the early universe, we consider the ...
The bispectrum, the three-point function of density fluctuations in Fourier space, is the lowest ord...
We consider a non-inflationary early Universe scenario in which relevant scalar perturbations get fr...
We investigate the degree to which the Cosmic Microwave Background (CMB) can be used to constrain pr...
Over thirty years since an early epoch of inflation was proposed as an elegant way solution to the B...
We argue that a plausible operational definition for an initial state of the universe is the initial...
We consider a primordial SU(2) vector multiplet during inflation in models where quantum fluctuation...
41 pages, 7 figures, 2 appendices. Added some clarifications and comments, additional references, to...
If time-dependent disruptions from slow-roll occur during inflation, the correlation functions of th...
We calculate the bispectrum of the Cosmic Microwave Background (CMB) temperature anisotropies induce...
Deviations from the Bunch-Davies vacuum during an inflationary period can leave a testable imprint o...
Until recently our knowledge of the primordial curvature perturbation was relatively modest. Ever si...
We revisit the predictions for the expected cosmic microwave background bispectrum signal from the c...
In this short note we translate the best available observational bounds on the CMB bispectrum amplit...
We present measurements of the dark matter bispectrum in N-body simulations with non-Gaussian initia...
In order to gain new insights into the gauge field couplings in the early universe, we consider the ...
The bispectrum, the three-point function of density fluctuations in Fourier space, is the lowest ord...
We consider a non-inflationary early Universe scenario in which relevant scalar perturbations get fr...
We investigate the degree to which the Cosmic Microwave Background (CMB) can be used to constrain pr...
Over thirty years since an early epoch of inflation was proposed as an elegant way solution to the B...
We argue that a plausible operational definition for an initial state of the universe is the initial...
We consider a primordial SU(2) vector multiplet during inflation in models where quantum fluctuation...