Dimensional reduction in the sky
Giovanni Amelino-Camelia, Michele Arzano, Giulia Gubitosi, Joao, Magueijo

TL;DR
This paper investigates how a quantum-gravity-inspired reduction of spacetime's spectral dimension to 2 in the ultraviolet leads to a naturally scale-invariant spectrum of cosmological fluctuations without inflation, impacting early universe models.
Contribution
It demonstrates that spectral dimension reduction to 2 in quantum gravity models produces scale-invariant fluctuations independently of the equation of state, challenging inflationary paradigms.
Findings
UV spectral dimension of 2 yields scale-invariant vacuum fluctuations
The fluctuation spectrum is scale-invariant before horizon crossing
Running spectral dimensions can improve cyclic/ekpyrotic models
Abstract
We explore the cosmological implications of a mechanism found in several approaches to quantum-gravity, whereby the spectral dimension of spacetime runs from the standard value of 4 in the infrared (IR) to a smaller value in the ultraviolet (UV). Specifically, we invoke the picture where the phenomenon is associated with modified dispersion relations. With minimal assumptions, we find that UV behaviour leading to 2 spectral dimensions results in an exactly scale-invariant spectrum of vacuum scalar and tensor fluctuations, regardless of the equation of state. The fluctuation production mechanism is analogous to the one known for varying speed of sound/light models and, unlike in inflation, the spectrum is already scale-invariant before leaving the horizon, remaining so after freeze-in. In the light of Planck's recent results we also discuss scenarios that break exact scale-invariance,…
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