Abstract. We investigate the symmetry constraints on the bispectrum, i.e. the three-point correlation function of primordial density fluctuations, in slow-roll inflation. It follows from the defining property of slow-roll inflation that primordial correlation functions inherit most of their structure from weakly broken de Sitter symmetries. Using holographic techniques borrowed from the AdS/CFT correspondence, the symmetry constraints on the bispectrum can be mapped to a set of stress-tensor Ward identities in a weakly broken 2 + 1-dimensional Euclidean CFT. We construct the consistency condition from these Ward identities using conformal perturbation theory. This requires a second order Ward identity and the use of the evolution equation. ...
We argue that the non-detection of primordial tensor modes has taught us a great deal about the prim...
We present a new method to calculate the spectrum of (slow-roll) inflationary perturbations, inspire...
We study the multifield inflationary models where the cosmological perturbation is sourced by light ...
We investigate the symmetry constraints on the bispectrum, i.e. the three-point correlation function...
We calculate the four point correlation function for scalar perturbations in the canonical model of ...
We calculate the four point correlation function for scalar perturbations in the canonical model of ...
We provide a precise and quantitative holographic description of a class of inflationary slow-roll m...
Nongaussian statistics are a powerful discriminant between inflationary models, particularly those w...
We continue the study of inflationary fluctuations in Holographic Space Time models of inflation. We...
In this thesis, we study the origin of the primordial fluctuations in the Cosmic Microwave Backgroun...
If time-dependent disruptions from slow-roll occur during inflation, the correlation functions of th...
Using symmetry considerations, we derive Ward identities which relate the three point function of sc...
Using symmetry considerations, we derive Ward identities which relate the three point function of sc...
Scattering amplitudes at weak coupling are highly constrained by Lorentz invariance, locality and un...
We study the multifield inflationary models where the cosmological perturbation is sourced by light ...
We argue that the non-detection of primordial tensor modes has taught us a great deal about the prim...
We present a new method to calculate the spectrum of (slow-roll) inflationary perturbations, inspire...
We study the multifield inflationary models where the cosmological perturbation is sourced by light ...
We investigate the symmetry constraints on the bispectrum, i.e. the three-point correlation function...
We calculate the four point correlation function for scalar perturbations in the canonical model of ...
We calculate the four point correlation function for scalar perturbations in the canonical model of ...
We provide a precise and quantitative holographic description of a class of inflationary slow-roll m...
Nongaussian statistics are a powerful discriminant between inflationary models, particularly those w...
We continue the study of inflationary fluctuations in Holographic Space Time models of inflation. We...
In this thesis, we study the origin of the primordial fluctuations in the Cosmic Microwave Backgroun...
If time-dependent disruptions from slow-roll occur during inflation, the correlation functions of th...
Using symmetry considerations, we derive Ward identities which relate the three point function of sc...
Using symmetry considerations, we derive Ward identities which relate the three point function of sc...
Scattering amplitudes at weak coupling are highly constrained by Lorentz invariance, locality and un...
We study the multifield inflationary models where the cosmological perturbation is sourced by light ...
We argue that the non-detection of primordial tensor modes has taught us a great deal about the prim...
We present a new method to calculate the spectrum of (slow-roll) inflationary perturbations, inspire...
We study the multifield inflationary models where the cosmological perturbation is sourced by light ...