Interaction of the Barbero--Immirzi Field with Matter and Pseudo-Scalar Perturbations

TL;DR

This paper explores a generalized Holst action in Loop Quantum Gravity, introducing a more natural coupling of the Barbero--Immirzi field with matter and analyzing its cosmological implications as a pseudo-scalar field.

Contribution

It proposes a new generalization of the Holst action that improves the coupling of the Barbero--Immirzi field with matter and investigates its cosmological effects.

Findings

A generalized Holst action with improved matter coupling

Potential cosmological roles of the Barbero--Immirzi pseudo-scalar field

Implications for quantum gravity and matter interactions

Abstract

In Loop Quantum Gravity the classical point of departure is the Einstein-Hilbert action modified by the addition of the so-called Holst term. Classically, this term does not affect the equations of motion, but it induces a well-known quantization ambiguity in the quantum theory, parametrized by the Barbero--Immirzi parameter. Recently, it has been suggested to promote the Barbero--Immirzi parameter to a field. The resulting theory, obtainable starting from the usual Holst action, is General Relativity coupled to a pseudo-scalar field. However, this theory turns out to have an unconventional kinetic term for the BI field and a rather unnatural coupling with fermions. The main goal of this work is twofold: Firstly, to propose a further generalization of the Holst action, which yields a theory of gravity and matter with a more natural coupling to the Barbero--Immirzi field; secondly, to study the possible implications for cosmology correlated to the existence of this new pseudo-scalar field.