Evolving a puncture black hole with fixed mesh refinement
Breno Imbiriba, John Baker, Dae-Il Choi, Joan Centrella, David R. Fiske, J. David Brown, James R. van Meter, Kevin Olson
TL;DR
This work addresses how fixed mesh refinement interfaces affect numerical relativity simulations of dynamical black holes. It adopts the BSSN formulation with puncture data and implements a third-order guard cell filling scheme within Paramesh to maintain second-order convergence near refinement boundaries while expanding the computational domain beyond $100M$. Through geodesic slicing and a variant of 1+$\,$log slicing, it demonstrates robust convergence in strong-field regions and identifies gauge-dependent limits, including a high-frequency origin-related noise under certain conditions. The results support the viability of FMR for long, high-resolution simulations and efficient gravitational waveform extraction, with future work extending to non-zero shift gauges.
Abstract
We present an algorithm for treating mesh refinement interfaces in numerical relativity. We detail the behavior of the solution near such interfaces located in the strong field regions of dynamical black hole spacetimes, with particular attention to the convergence properties of the simulations. In our applications of this technique to the evolution of puncture initial data with vanishing shift, we demonstrate that it is possible to simultaneously maintain second order convergence near the puncture and extend the outer boundary beyond 100M, thereby approaching the asymptotically flat region in which boundary condition problems are less difficult and wave extraction is meaningful.
