Enrico Pajer - Field Theory in Cosmology
These lectures introduce quantum field theory methods for early-universe cosmology, in particular the quantum generation of primordial perturbations during inflation. After a brief review of cosmology, we learn how to quantize scalars and gravitons in curved spacetime and compute cosmological correlators using the in-in (canonical) formalism. We briefly discuss the effective field theory approach to gravity and derive predictions for primordial non-Gaussianity, primarily bispectra. The notes conclude with a discussion of cosmological soft theorems and Maldacena's consistency relation.
Field Theory in Cosmology lecture notes (PDF)
Please do let me know if you find any typos or errors!
Contents
- A quick review of background cosmology
- Free fields on curved backgrounds
- Interacting fields and the in-in formalism
- Correlators from P(X,phi) theories
- Gravity
- Symmetries and soft theorems
- Phenomenology
Problem Sheets
These example sheets are from the Lent Term 2020 and 2021 versions of the course.
