ATTENTION! We have to do a short maintenance with downtime on Wed 8 Oct 2025, 09:00 - 10:00 CEST . Please finish your work in time to prevent data loss.
For further information, please have look at the IT-News article

25–28 Sept 2012
DESY Hamburg
Europe/Berlin timezone

Observational degeneracy between non-canonical and canonical single field inflation

27 Sept 2012, 16:50
20m
Seminar room 2 (DESY)

Seminar room 2

DESY

Cosmology & Astroparticle Physics Parallel Session 2: Cosmology & Astroparticle Physics

Speaker

Mr Markus Rummel (University of Hamburg)

Description

We discuss observational degeneracy between non-canonical and canonical single field inflation. We map the dynamics of the non-canonical inflationary trajectory to a Lagrangian with canonically normalized kinetic term and a scalar potential. At the level of the two-point function, the two theories are observationally degenerate at all times. To obtain observationally degeneracy at the level of the three-point function, we add sinusodial contributions to the scalar potential. These give rise to resonant non-Gaussianities, whose superpositions are shown to approximately match equilateral non-Gaussianity which is characteristic for non-canonical inflation. We discuss explicit examples such as DBI-inflation.

Primary authors

Dr Alexander Westphal (DESY) Mr Markus Rummel (University of Hamburg) Dr Rhiannon Gwyn (University of Hamburg)

Presentation materials