PIRSA:18060001

Video URL

https://pirsa.org/18060001

Connecting inflation to diverse observables: leptons, baryons and cosmological magnetic fields

Sfakianakis, E. (2018). Connecting inflation to diverse observables: leptons, baryons and cosmological magnetic fields. Perimeter Institute for Theoretical Physics. https://pirsa.org/18060001

Sfakianakis, Evangelos. Connecting inflation to diverse observables: leptons, baryons and cosmological magnetic fields. Perimeter Institute for Theoretical Physics, Jun. 12, 2018, https://pirsa.org/18060001 

          @misc{ scivideos_PIRSA:18060001,
            doi = {10.48660/18060001},
            url = {https://pirsa.org/18060001},
            author = {Sfakianakis, Evangelos},
            keywords = {Cosmology},
            language = {en},
            title = {Connecting inflation to diverse observables: leptons, baryons and cosmological magnetic fields},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2018},
            month = {jun},
            note = {PIRSA:18060001 see, \url{https://scivideos.org/pirsa/18060001}}
          }

Evangelos Sfakianakis Leiden University

Talk numberPIRSA:18060001
DOI10.48660/18060001
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

Axions are attractive candidates for theories of large-field inflation that are capable of generating observable primordial gravitational wave backgrounds. These fields enjoy shift-symmetries that protect their role as inflatons from being spoiled by coupling to unknown UV physics. This symmetry also restricts the couplings of these axion fields to other matter fields. At lowest order, the only allowed interactions are derivative couplings to gauge fields and fermions. These derivative couplings lead to the biased production of fermion and gauge-boson helicity states during and after inflation. I will discuss preheating in axion-inflation models that are derivatively coupled to Abelian gauge-fields and fermion axial-currents.

For an axion coupled to U(1) gauge fields preheating is efficient for a wide range of parameters. In certain cases the inflaton is seen to transfer all its energy to the gauge fields within a few oscillations. Identifying the gauge field as the hypercharge sector of the Standard Model can lead to the generation of cosmologically relevant magnetic fields.

Coupling the inflaton-axion to Majorana fermions leads to the biased production of fermion helicity-states which can have interesting phenomenological implications for leptogenesis.