PIRSA:17080057

Video URL

https://pirsa.org/17080057

Baryon Asymmetry and Gravitational Waves from Pseudoscalar Inflation

Schmitzk, K. (2017). Baryon Asymmetry and Gravitational Waves from Pseudoscalar Inflation. Perimeter Institute for Theoretical Physics. https://pirsa.org/17080057

Schmitzk, Kai. Baryon Asymmetry and Gravitational Waves from Pseudoscalar Inflation. Perimeter Institute for Theoretical Physics, Aug. 10, 2017, https://pirsa.org/17080057 

          @misc{ scivideos_PIRSA:17080057,
            doi = {10.48660/17080057},
            url = {https://pirsa.org/17080057},
            author = {Schmitzk, Kai},
            keywords = {Cosmology},
            language = {en},
            title = {Baryon Asymmetry and Gravitational Waves from Pseudoscalar Inflation},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2017},
            month = {aug},
            note = {PIRSA:17080057 see, \url{https://scivideos.org/index.php/pirsa/17080057}}
          }

Kai Schmitzk Max Planck Institute

Talk numberPIRSA:17080057
DOI10.48660/17080057
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

In models of inflation driven by an axion-like pseudoscalar field, the inflaton, a, may couple to the standard model hypercharge gauge field via a Chern-Simons-type interaction, L ⊃ a F F̃. This coupling results in the explosive production of hypermagnetic fields during inflation, which has two interesting consequences: (1) The primordial hypermagnetic field is maximally helical. It is therefore capable of sourcing the generation of nonzero baryon number around the electroweak phase transition (via the chiral anomaly in the standard model). (2) The gauge field production during inflation feeds back into the stochastic background of gravitational waves (GWs). In this talk, I am going to discuss the correlation between these two phenomena. To this end, I will (a) present an updated study of baryogenesis via hypermagnetic fields after pseudoscalar inflation and (b) describe the corresponding implications for GWs. As it turns out, successful baryogenesis is feasible---provided the axion coupling to the gauge fields is suppressed by a decay constant \Lambda ~ 3 x 10^17 GeV. Moreover, in the case of successful baryogenesis, one expects a characteristic peak in the GW spectrum at frequencies in the MHz range