Gaugid inflation

Federico Piazza (1) , David Pirtskhalava , Riccardo Rattazzi , Olivier Simon

1 CPT - Centre de Physique Théorique - UMR 7332

The spectrum of primordial gravitational waves is one of the most robust inflationary observables, often thought of as a direct probe of the energy scale of inflation. We present a simple model, where the dynamics controlling this observable is very different than in the standard paradigm of inflation. The model is based on a peculiar finite density phase—the magnetic gaugid—which stems from a highly non-linear effective theory of a triplet of abelian gauge fields. The gaugid extends the notion of homogeneous isotropic solid, in that its spectrum of fluctuations includes helicity-2 phonons. We show how, upon implementing the gaugid to drive inflation, the helicity-2 phonon mixes with the graviton, significantly affecting the size of the primordial tensor spectrum. The rest of the features of the theory, in particular the vector and scalar perturbations, closely resemble those of solid inflation.

Mots clés: scale: inflation; fluctuation: spectrum; spectrum: tensor; gravitational radiation: primordial; gauge field theory: abelian; perturbation: scalar; density: finite; phonon; solids; gravitation; nonlinear; graviton; triplet

Domaines: Physique des Hautes Energies - Théorie [hep-th]; Astrophysique [astro-ph]; Physique des Hautes Energies - Phénoménologie [hep-ph]

Federico Piazza, David Pirtskhalava, Riccardo Rattazzi, Olivier Simon. Gaugid inflation. JCAP, 2017, 11, pp.041. ⟨10.1088/1475-7516/2017/11/041⟩. ⟨hal-01669547⟩