PIRSA:24090152

Video URL

https://pirsa.org/24090152

Graviton non-Gaussianity with non-Bunch-Davies initial conditions

Mylova, M. (2024). Graviton non-Gaussianity with non-Bunch-Davies initial conditions. Perimeter Institute for Theoretical Physics. https://pirsa.org/24090152

Mylova, Maria. Graviton non-Gaussianity with non-Bunch-Davies initial conditions. Perimeter Institute for Theoretical Physics, Sep. 17, 2024, https://pirsa.org/24090152 

          @misc{ scivideos_PIRSA:24090152,
            doi = {10.48660/24090152},
            url = {https://pirsa.org/24090152},
            author = {Mylova, Maria},
            keywords = {Cosmology},
            language = {en},
            title = {Graviton non-Gaussianity with non-Bunch-Davies initial conditions},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2024},
            month = {sep},
            note = {PIRSA:24090152 see, \url{https://scivideos.org/index.php/pirsa/24090152}}
          }

Maria Mylova University of Tokyo

Talk numberPIRSA:24090152
DOI10.48660/24090152
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

I will discuss recent progress on the initial conditions for inflation and how this can potentially enhance gravitational wave non-Gaussianity (NG). In particular, there is a significant additional NG contribution in the flattened configuration, offering a straightforward way to boost parity-violating NG from Chern-Simons gravity, which typically suffers from graviton ghost-production. Furthermore, I will explore how this shape – at the level of the trispectrum – can enable direct measurement of NG in the stochastic gravitational wave background (SGWB) using pulsar timing arrays (PTA). This is particularly intriguing as it allows us to investigate NG at scales complementary to those observed in the CMB, which could help us distinguish between various early universe models and physical mechanisms.