The twilight of the single field slow rolling inflaton
Jaume Amoros, Jaume de Haro

TL;DR
This paper evaluates 49 slow roll inflationary potentials against PLANCK data, finding most disfavored by the running of the spectral index, but recent data improves viability, though the running of the running remains problematic.
Contribution
It provides a comprehensive analysis of multiple inflationary potentials using recent observational data, highlighting the impact of updated measurements on model viability.
Findings
Most potentials disfavored by PLANCK2013 data based on the running of the spectral index.
Recent PLANCK2015 data reduces the discrepancy, making most potentials viable.
The running of the running remains incompatible with theoretical predictions, disfavouring many models.
Abstract
We present an study from PLANCK2013+WP+BAO:CDM++ data, where 49 slow roll inflationary potentials are tested, showing that the theoretical value of the running provided by 48 of these potentials has a deviation to the expected observational value larger than , and its modulus is smaller than the modulus of the expected observational one, what disfavours these models at 94.5 \% of Confidence Level (C.L.), concluding from these results that, inflationary cosmology may require multiple fields or a breakdown of slow roll condition. This conclusion has drastically changed with the last data provided by PLANCK2015 where the modulus of the expected observational value of the running has been reduced one order, getting shorter the distance to its theoretical value or more, what allows the viability of the majority of the potentials disfavored by the…
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Taxonomy
TopicsCosmology and Gravitation Theories · Galaxies: Formation, Evolution, Phenomena · Solar and Space Plasma Dynamics
