Quantization of Gravity in Spherical Harmonic Basis
Renata Kallosh

TL;DR
This paper presents a canonical quantization of gravity around a Schwarzschild black hole, demonstrating a unitary, ghost-free Hamiltonian with specific degrees of freedom, applicable also in Minkowski space.
Contribution
It introduces a new quantization scheme for gravity in spherical coordinates using the Regge-Wheeler gauge, ensuring unitarity and ghost-freedom at quadratic order.
Findings
Hamiltonian is unitary and ghost-free
Two degrees of freedom linked to metric perturbations
Quantization valid in both black hole and Minkowski backgrounds
Abstract
We perform canonical quantization of gravity in the background of a Schwarzschild black hole in the generalized Regge-Wheeler gauge proposed in \cite{Kallosh:2021ors}. We find that the Hamiltonian at the quadratic level is unitary and ghost-free. Two canonical degrees of freedom are associated with Zerilli-Moncrief and Cunningham-Price-Moncrief functions of the metric perturbations. The part of the Hamiltonian vanishes. This quantization with the unitary Hamiltonian for gravity is valid also in Minkowski space in spherical coordinates.
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.
