Cosmological Inflation: where we are, and where we (might be) headed
by
Will Kinney(University at Buffalo, SUNY, and Visiting faculty at OKC)
→
Europe/Stockholm
FA31
FA31
Description
Cosmological inflation proposes the existence of a period of
near-exponential expansion in the very early universe, providing a dynamical explanation for the initial condition for a flat, homogeneous universe. Quantum fluctuations during inflation, stretched to long wavelengths by the rapid expansion, form a background of nearly scale-invariant perturbations, providing a powerful observational test of the model. In this colloquium, I will review the evidence for inflation in light of the most recent observations, and discuss current ideas and issues in inflationary model building, including recently proposed ``swampland'' conjectures for consistency with string-based UV completions.