Inflation from Flux Cascades
Guido D'Amico, Roberto Gobbetti, Matthew Kleban, Marjorie Schillo

TL;DR
This paper introduces a new inflationary mechanism driven by flux cascades in extra dimensions, leading to a prolonged inflation with observable signatures, naturally fitting into string theory without fine-tuning.
Contribution
It proposes a novel flux cascade process as a source of inflation, producing realistic cosmological perturbations and integrating naturally into the string landscape.
Findings
Achieves ~60 e-folds of inflation with decreasing Hubble constant.
Produces a nearly scale-invariant spectrum with observable non-Gaussianity and tensor modes.
Features a small oscillatory component in the power spectrum related to compact dimensions.
Abstract
When electric-type flux threads compact extra dimensions, a quantum nucleation event can break a flux line and initiate a cascade that unwinds many units of flux. Here, we present a novel mechanism for inflation based on this phenomenon. From the 4D point of view, the cascade begins with the formation of a bubble containing an open Friedmann-Robertson-Walker cosmology, but the vacuum energy inside the bubble is initially only slightly reduced, and subsequently decreases gradually throughout the cascade. If the initial flux number Q_0 ~ O(100), during the cascade the universe can undergo N ~ 60 efolds of inflationary expansion with gradually decreasing Hubble constant, producing a nearly scale-invariant spectrum of adiabatic density perturbations with amplitude and tilt consistent with observation, and a potentially observable level of non-Gaussianity and tensor modes. The power spectrum…
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