PIRSA:09120028

Approaches to Understanding Inflation: String Models and Axions

Hertzberg, M. (2009). Approaches to Understanding Inflation: String Models and Axions. Perimeter Institute. https://pirsa.org/09120028

Hertzberg, Mark. Approaches to Understanding Inflation: String Models and Axions. Perimeter Institute, Dec. 01, 2009, https://pirsa.org/09120028 

          @misc{ pirsa_PIRSA:09120028,
            doi = {10.48660/09120028},
            url = {https://pirsa.org/09120028},
            author = {Hertzberg, Mark},
            keywords = {Cosmology},
            language = {en},
            title = {Approaches to Understanding Inflation: String Models and Axions},
            publisher = {Perimeter Institute},
            year = {2009},
            month = {dec},
            note = {PIRSA:09120028 see, \url{https://pirsa.org}}
          }

Mark Hertzberg

Talk number
PIRSA:09120028
Collection
Talk Type
Subject
Abstract
Although the observational evidence for cosmological inflation is growing, the physical mechanism behind it is still unknown. In part this is because inflation probably occurred at energy scales many orders of magnitude higher than that at man-made or astrophysical particle accelerators. So how can we learn about inflation? How does it constrain microphysical theory? One approach to answering these questions is primarily theoretical: attempting to embed inflation in fundamental theories of quantum gravity, such as string theory. Another approach is primarily observational: looking for signatures left by light fields that existed during inflation, such as isocurvature fluctuations from the QCD-axion. In this talk I discuss work on these two approaches.