Inflation in an effective gravitational model & asymptotic safety

TL;DR

This paper explores an inflationary model inspired by quantum gravitational effects near the Planck scale, refining the Starobinsky model with a logarithmic correction, and analyzes its compatibility with observational data.

Contribution

It introduces a re-summed effective Lagrangian incorporating quantum effects, extending the Starobinsky model with a logarithmic term, and assesses its inflationary predictions against Planck data.

Findings

Increasing parameter b raises n_s and r within observational limits.

The model predicts r up to 0.01, detectable by future CMB experiments.

The running of the spectral index remains around -5×10^{-4}, below current bounds.

Abstract

We consider an inflationary model motivated by quantum effects of gravitational and matter fields near the Planck scale. Our Lagrangian is a re-summed version of the effective Lagrangian recently obtained by Demmel, Saueressig and Zanusso~\cite{Demmel:2015oqa} in the context of gravity as an asymptotically safe theory. It represents a refined Starobinsky model, ${\cal L}_{\rm eff}=M_{\rm P}^2 R/2 + (a/2)R^2/[1+b\ln(R/\mu^2)]$, where $R$ is the Ricci scalar, $a$ and $b$ are constants and $\mu$ is an energy scale. By implementing the COBE normalisation and the Planck constraint on the scalar spectrum, we show that increasing $b$ leads to an increased value of both the scalar spectral index $n_s$ and the tensor-to-scalar ratio $r$. Requiring $n_s$ to be consistent with the Planck collaboration upper limit, we find that $r$ can be as large as $r\simeq 0.01$, the value possibly measurable by Stage IV CMB ground experiments and certainly from future dedicated space missions. The predicted running of the scalar spectral index $\alpha=d n_s/d\ln(k)$ is still of the order $-5\times 10^{-4}$ (as in the Starobinsky model), about one order of magnitude smaller than the current observational bound.