Using symmetry considerations, we derive Ward identities which relate the three point function of scalar perturbations produced during inflation to the scalar four point function, in a particular limit. The derivation assumes approximate conformal invariance, and the conditions for the slow roll approximation, but is otherwise model independent. The Ward identities allow us to deduce that the three point function must be suppressed in general, being of the same order of magnitude as in the slow roll model. They also fix the three point function in terms of the four point function, upto one constant which we argue is generically suppressed. Our approach is based on analyzing the wave function of the universe, and the Ward identities arise by...
In this paper, we explore a novel observational signature of gravitational corrections during slow-r...
In this thesis, we study the origin of the primordial fluctuations in the Cosmic Microwave Backgroun...
Non-Gaussianities of the primordial density perturbations have emerged as a very powerful possible s...
Using symmetry considerations, we derive Ward identities which relate the three point function of sc...
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 calculate the four point correlation function for scalar perturbations in the canonical model of ...
We investigate the symmetry constraints on the bispectrum, i.e. the three-point correlation function...
We study the multifield inflationary models where the cosmological perturbation is sourced by light ...
Abstract. We investigate the symmetry constraints on the bispectrum, i.e. the three-point correlatio...
We study the multifield inflationary models where the cosmological perturbation is sourced by light ...
We consider the most general three point function for gravitational waves produced during a period o...
The consistency relation for the three-point function of the cosmic microwave background is a very p...
Scattering amplitudes at weak coupling are highly constrained by Lorentz invariance, locality and un...
Scattering amplitudes at weak coupling are highly constrained by Lorentz invariance, locality and un...
In this paper, we explore a novel observational signature of gravitational corrections during slow-r...
In this thesis, we study the origin of the primordial fluctuations in the Cosmic Microwave Backgroun...
Non-Gaussianities of the primordial density perturbations have emerged as a very powerful possible s...
Using symmetry considerations, we derive Ward identities which relate the three point function of sc...
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 calculate the four point correlation function for scalar perturbations in the canonical model of ...
We investigate the symmetry constraints on the bispectrum, i.e. the three-point correlation function...
We study the multifield inflationary models where the cosmological perturbation is sourced by light ...
Abstract. We investigate the symmetry constraints on the bispectrum, i.e. the three-point correlatio...
We study the multifield inflationary models where the cosmological perturbation is sourced by light ...
We consider the most general three point function for gravitational waves produced during a period o...
The consistency relation for the three-point function of the cosmic microwave background is a very p...
Scattering amplitudes at weak coupling are highly constrained by Lorentz invariance, locality and un...
Scattering amplitudes at weak coupling are highly constrained by Lorentz invariance, locality and un...
In this paper, we explore a novel observational signature of gravitational corrections during slow-r...
In this thesis, we study the origin of the primordial fluctuations in the Cosmic Microwave Backgroun...
Non-Gaussianities of the primordial density perturbations have emerged as a very powerful possible s...