Pseudospectral implementation of the Einstein-Maxwell system
Jorge Expósito Patiño, Hannes R. Rüter, David Hilditch
TL;DR
This work delivers a first construction of a pseudospectral, first-order symmetric-hyperbolic Maxwell evolution embedded in the Einstein equations within the BAMPS code. By introducing constraint-damping via auxiliary fields and boundary-preserving conditions, it achieves boundary stability for the electrovacuum system and enables robust, high-accuracy simulations. The authors validate the approach through convergence tests, Reissner–Nordström and Kerr quasinormal mode benchmarks, and a strong-field, near-threshold collapse–like scenario, demonstrating reliable EM–GR coupling in electrovacuum. The methodology and verification suite establish a solid foundation for exploring electrovacuum dynamics, critical phenomena, and EM–gravitational wave interactions in strong gravity environments.
Abstract
Electromagnetism plays an important role in a variety of applications in gravity that we wish to investigate. To that end, in this work, we present an implementation of the Maxwell equations within the adaptive-mesh pseudospectral numerical relativity code BAMPS. We perform a thorough analysis of the evolution equations as a first order symmetric hyperbolic system of PDEs. This includes both the construction of the characteristic variables for use in our penalty boundary communication scheme, as well as radiation controlling, constraint preserving outer boundary conditions which, for the first time in a numerical context, are shown to be boundary-stable. After choosing a formulation of the Maxwell constraints that we may solve for initial data, we move on to show a suite of numerical tests. Our simulations, both within the Cowling approximation, and in full non-linear evolution, demonstrate rapid convergence of error with resolution, as well as consistency with known quasinormal decay rates on the Kerr background. Finally we evolve the electrovacuum equations of motion with strong data, a good representation of typical critical collapse runs.
