Gauge-invariant coefficients in perturbative quantum gravity
Fiorenzo Bastianelli, Roberto Bonezzi, Marco Melis

TL;DR
This paper recalculates heat kernel coefficients in perturbative quantum gravity, confirms their gauge invariance on-shell, and identifies necessary corrections in the worldline approach for arbitrary dimensions.
Contribution
It provides a benchmark for gauge-invariant coefficients and proposes amendments to the worldline quantization method in arbitrary dimensions.
Findings
Recomputed heat kernel coefficients match literature in D=4.
Discovered mismatch in coefficients at D≠4 in the worldline approach.
Proposed fixing the worldline path integral to ensure consistency across dimensions.
Abstract
Heat kernel methods are useful for studying properties of quantum gravity. We recompute here the first three heat kernel coefficients in perturbative quantum gravity with cosmological constant to ascertain which ones are correctly reported in the literature. They correspond to the counterterms needed to renormalize the one-loop effective action in four dimensions. They may be evaluated at arbitrary dimensions , in which case they identify only a subset of the divergences appearing in the effective action for . Generically, these coefficients depend on the gauge-fixing choice adopted in quantizing the Einstein-Hilbert action. However, they become gauge-invariant once evaluated on-shell, i.e. using Einstein's field equations with cosmological constant. We identify them and use them as a benchmark for checking alternative approaches to perturbative quantum gravity. One such…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsNoncommutative and Quantum Gravity Theories · Black Holes and Theoretical Physics · Cosmology and Gravitation Theories
