Constraining the Barbero-Immirzi parameter from the duration of inflation in loop quantum cosmology

TL;DR

This paper investigates how the duration of inflation in loop quantum cosmology constrains the Barbero-Immirzi parameter, analyzing various inflationary potentials and their observable implications on the cosmic microwave background.

Contribution

It provides a novel analysis linking the Barbero-Immirzi parameter to inflation duration, considering different potentials and allowing for its variation within loop quantum gravity.

Findings

Lower limit for the Barbero-Immirzi parameter consistent with CMB data

Inflation duration depends on initial conditions set at the bounce

Different inflationary potentials can produce observable signatures

Abstract

We revisit the predictions for the duration of the inflationary phase after the bounce in loop quantum cosmology. We present our analysis for different classes of inflationary potentials that include the monomial power-law chaotic type of potentials, the Starobinsky and the Higgs-like symmetry breaking potential with different values for the vacuum expectation value. Our setup can easily be extended to other forms of primordial potentials than the ones we have considered. Independently on the details of the contracting phase, if the dynamics starts sufficiently in the far past, the kinetic energy will come to dominate at the bounce, uniquely determining the amplitude of the inflaton at this moment. This will be the initial condition for the further evolution that will provide us with results for the number of e-folds from the bounce to the beginning of the accelerated inflationary regime and the subsequent duration of inflation. We also discuss under which conditions each model considered could lead to observable signatures on the spectrum of the cosmic microwave background or else be excluded for not predicting a sufficient amount of accelerated expansion. A first analysis is performed considering the standard value for the Barbero-Immirzi parameter obtained from black hole entropy calculations. In a second analysis, we consider the possibility of varying the value of this parameter, which is motivated by the fact that the Barbero-Immirzi parameter can be considered a free parameter of the underlying quantum theory in the context of loop quantum gravity. From this analysis, we obtain a lower limit for this parameter by requiring the minimum amount of inflationary expansion that makes the model consistent with the CMB observations. [abridged]