Affine Connections in Quantum Gravity and New Scalar Fields

TL;DR

This paper explores the use of more general affine connections in quantum gravity, introducing new scalar fields that could explain phenomena like inflation and dark energy, and discusses formalism extensions beyond traditional metric-compatible approaches.

Contribution

It proposes a novel formalism using general affine connections in quantum gravity, leading to new scalar fields and extending traditional Palatini and metric-affine formalisms.

Findings

General affine connections introduce two massless scalar fields.

One scalar field contributes a negative stress-tensor in Einstein's equations.

The formalism could explain inflation and dark energy phenomena.

Abstract

In this manuscript, we will discuss the construction of covariant derivative operator in quantum gravity. We will find it is more perceptive alternative to use affine connections more general than metric compatible connections in quantum gravity. We will demonstrate this using the canonical quantization procedure. This is valid irrespective of the presence and nature of sources. The conventional Palatini and metric-affine formalisms, where the actions are linear in the scalar curvature with metric and affine connections being the the independent variables, are not much suitable to construct a source-free theory of gravity with general affine connections. This is also valid for many minimally coupled interacting theories where sources only couple with metric by using the Levi-Civita connections exclusively. We will discuss potential formalism of affine connections to introduce affine connections more general than metric compatible connections in gravity. We will also discuss possible extensions of the actions for this purpose. General affine connections introduce new fields in gravity besides metric. In this article, we will consider a simple potential formalism with symmetric affine connections and symmetric Ricci tensor. Corresponding affine connections introduce two massless scalar fields. One of these fields contributes a stress-tensor with opposite sign to the sources of Einstein's equation when we state the equation using the Levi-Civita connections. This means we have a massless scalar field with negative stress-tensor in Einstein's equation. This field brings us beyond strict local Minkowski geometries. These scalar fields can be useful to explain inflation and dark energy.