An axisymmetric evolution code for the Einstein equations on hyperboloidal slices
Oliver Rinne

TL;DR
This paper introduces a stable numerical evolution scheme for Einstein's equations on hyperboloidal slices, enabling accurate simulations extending to null infinity, with successful long-term evolution of Schwarzschild spacetime and gravitational perturbations.
Contribution
It presents the first stable dynamical evolution of Einstein's equations on hyperboloidal slices using a conformally rescaled metric, incorporating regularization techniques at null infinity.
Findings
Achieved long-term stable evolutions of Schwarzschild spacetime.
Successfully computed the Bondi news function at null infinity.
Demonstrated regularization of singular equations at null infinity.
Abstract
We present the first stable dynamical numerical evolutions of the Einstein equations in terms of a conformally rescaled metric on hyperboloidal hypersurfaces extending to future null infinity. Axisymmetry is imposed in order to reduce the computational cost. The formulation is based on an earlier axisymmetric evolution scheme, adapted to time slices of constant mean curvature. Ideas from a previous study by Moncrief and the author are applied in order to regularize the formally singular evolution equations at future null infinity. Long-term stable and convergent evolutions of Schwarzschild spacetime are obtained, including a gravitational perturbation. The Bondi news function is evaluated at future null infinity.
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.
