The critical geometry of a thermal big bang
Niayesh Afshordi, Joao Magueijo

TL;DR
This paper introduces a novel scalar-tensor cosmological model with a critical geometry that predicts a specific spectral index for scalar fluctuations, suggesting a thermal origin of fluctuations without requiring inflation.
Contribution
It identifies a critical solution in scalar-tensor theories with two non-conformal metrics, leading to a highly predictive cosmological model with unique fluctuation properties.
Findings
Predicts scalar spectral index n_S=0.96478(64)
No gravitational waves produced in the model
Fluctuations originate thermally inside the horizon without inflation
Abstract
We explore the space of scalar-tensor theories containing two non-conformalmetrics, and find a discontinuity pointing to a "critical" cosmological solution. Due to the different maximal speeds of propagation for matter and gravity,the cosmological fluctuations start off inside the horizon even without inflation, and will more naturally have a thermal origin (since there is never vacuum domination). The critical model makes an unambiguous, non-tuned prediction for the spectral index of the scalar fluctuations: . Considering also that no gravitational waves are produced, we have unveiled the most predictive model on offer. The model has a simple geometrical interpretation as a probe 3-brane embedded in an geometry.
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