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arXiv · 2412.14265

Inflation without an Inflaton

Daniele Bertacca·Raul Jimenez·Sabino Matarrese·Angelo Ricciardone
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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.

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Daniele Bertacca, Raul Jimenez, Sabino Matarrese, Angelo Ricciardone. 2024-12-18. Inflation without an Inflaton. https://arxiv.org/abs/2412.14265

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