Inflation without an inflaton
We propose a novel scenario in which scalar perturbations, which 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, where tensor metric fluctuations (i.e., gravitational wav...
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Main Authors: | Daniele Bertacca, Raul Jimenez, Sabino Matarrese, Angelo Ricciardone |
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Format: | Article |
Language: | English |
Published: |
American Physical Society
2025-07-01
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Series: | Physical Review Research |
Online Access: | http://doi.org/10.1103/vfny-pgc2 |
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