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14–16 May 2024
CERN
Europe/Zurich timezone

Scale-invariant inflation

15 May 2024, 12:01
5m
500/1-001 - Main Auditorium (CERN)

500/1-001 - Main Auditorium

CERN

400
Show room on map
early universe cosmology Early Universe

Speaker

Chiara Cecchini (University of Trento, TIFPA-INFN)

Description

Fundamental scale invariance has been proposed as a new theoretical principle beyond renormalizability. Besides its highly predictive power, a scale-invariant formulation of gravity could provide a natural explanation for the long-standing hierarchy problem and interesting applications in cosmology.
We present a globally scale-invariant model of quadratic gravity and study its solutions in a spatially flat Robertson-Walker metric. The system admits a dynamical flow from an unstable to a stable fixed point, where scale symmetry gets spontaneously broken, and a mass scale — the Planck mass — is classically generated. This trajectory is compatible with an arbitrarily long stage of inflation which is investigated both at the classical level and at first order in perturbation theory. We outline some of the most recent result obtained within the framework of scale-invariant inflation.

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Primary authors

Chiara Cecchini (University of Trento, TIFPA-INFN) Mrs Mariaveronica De Angelis (University of Sheffield) Massimiliano Rinaldi (University of Trento) Sunny Vagnozzi William Giare (University of Sheffield)

Presentation materials