Inflation without an Inflaton
Abstract
We propose a novel scenario in which scalar perturbations, that seed the large scale structure of the Universe, are generated without relying on a scalar field (the inflaton). In this framework, inflation is driven by a de Sitter space-time (dS), where tensor metric fluctuations (i.e., gravitational waves) naturally arise from quantum vacuum oscillations, and scalar fluctuations are generated via second-order tensor effects. We compute the power spectrum of such scalar fluctuations and show it to be consistent with near scale-invariance. We derive the necessary conditions under which scalar perturbations become significant and much larger than the tensor modes, and we identify a natural mechanism to end inflation via a transition to a radiation-dominated phase. Our proposed mechanism could remove the need for a model-dependent scenario: the choice of a scalar field, as the inflaton, to drive inflation.
Cite
@article{arxiv.2412.14265,
title = {Inflation without an Inflaton},
author = {Daniele Bertacca and Raul Jimenez and Sabino Matarrese and Angelo Ricciardone},
journal= {arXiv preprint arXiv:2412.14265},
year = {2024}
}