Primordial Intermittent Non-Gaussianities
Speaker
Date
Time
Place
Room 7W3
Abstract
A major CITA concentration is "primordial intermittent nonGaussianities" (pinGs) which can arise generically during and after inflation from field-instabilities transverse to the inflaton. CMB and LSS lightcone Webskys we construct with spatially localized pinGs can evade the stringent 2D perturbative single-nonG-template constraints from the ~10 e-folds probed by Planck. pinGs could play a role in the low-k CMB anomalies and have correlated localized B-modes sourced by anisotropic stress. pinGs would be more easily detected in 3D LSS surveys and could be hugely-big in the largely obscured 50 e-foldings from CMB/LSS scales to the end of inflation. We explore the generic nature of pinGs using pseudo-spectral lattice simulations and dynamical systems theory applied to multi-field effective potentials cast in an in-out state formulation. Though similar in spirit to the $mass^2 >0$ cosmic collider program, the $mass^2 <0$ in (incomplete) phase transitions gives more dramatic observable phenomena, maybe even with entropic memories of domain wall and stringy structures in Webskys. I will also relate this pinGy work to our popular stochastic-inflation-pinGing framework.
Biography
Richard (Dick) Bond is a famous Canadian astrophysicist and cosmologist. He is a professor at the Canadian Institute for Theoretical Astrophysics (CITA) and at the University of Toronto. From 1996 to 2006, he was CITA's director, and since 2002 he has been the director of the Cosmology and Gravity Program for the Canadian Institute for Advanced Research (CIFAR). Among his many awards are the Dannie Heineman Prize for Astrophysics and the Gruber Prize in Cosmology. He is a Fellow of the Royal Society (of UK and Canada). Bond's most famous work concerns the theoretical modeling of anisotropies of the cosmic background radiation.