# The Spectrum of Quantum Gravity

**Authors:** Xavier Calmet, Boris Latosh

arXiv: 1907.10024 · 2019-07-24

## TL;DR

This paper investigates additional degrees of freedom in quantum gravity beyond the graviton, analyzing how higher curvature operators affect the pole structure and scalar modes, and clarifies the relation between different frames in effective theories.

## Contribution

It provides a detailed analysis of how higher order curvature operators influence the spectrum of quantum gravity and clarifies the mapping between Jordan and Einstein frames for these theories.

## Key findings

- Operators of type R^2 and Ricci tensor squared do not alter existing poles.
- Operators like R□R introduce new poles and shift existing ones.
- The paper resolves ambiguities in relating scalar degrees of freedom between frames.

## Abstract

In this paper we consider the degrees of freedom beyond the graviton present in the effective field theory for quantum gravity. We point out that the position of the poles due to $R^2$ and $R_{\mu\nu}R^{\mu\nu}$ cannot be affected by operators that are higher order in curvature. On the other hand, operators of the type $R\Box R$ will lead to new poles while shifting the positions of the poles found at second order in curvature. New degrees of freedom can be identified either, as just described, by looking at the poles of the graviton propagator corrected by quantum gravity or by mapping the Jordan frame theory to the Einstein frame theory. While this procedure is very well defined for second order curvature terms in the effective action, we point out that higher order terms in curvature lead to a nonlinear and non-local relation between the propagating scalar degree of freedom and the Ricci scalar. We show how to resolve these ambiguities and how to obtain the correct action in the Einstein frame. We illustrate our results by looking at $f(R)$ gravity.

## Full text

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## References

26 references — full list in the complete paper: https://tomesphere.com/paper/1907.10024/full.md

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Source: https://tomesphere.com/paper/1907.10024