High order discontinuous Galerkin schemes with subcell finite volume limiter and AMR for a monolithic first--order BSSNOK formulation of the Einstein--Euler equations
<|reference_start|>High order discontinuous Galerkin schemes with subcell finite volume limiter and AMR for a monolithic first--order BSSNOK formulation of the Einstein--Euler equations: We propose a high order discontinuous Galerkin (DG) scheme with subcell finite volume (FV) limiter to solve a monolithic first--order hyperbolic BSSNOK formulation of the coupled Einstein--Euler equations. The numerical scheme runs with adaptive mesh refinement (AMR) in three space dimensions, is endowed with time-accurate local time stepping (LTS) and is able to deal with both conservative and non-conservative hyperbolic systems. The system of governing partial differential equations was shown to be strongly hyperbolic and is solved in a monolithic fashion with one numerical framework that can be simultaneously applied to both the conservative matter subsystem as well as the non-conservative subsystem for the spacetime. Since high order unlimited DG schemes are well-known to produce spurious oscillations in the presence of discontinuities and singularities, our subcell finite volume limiter is crucial for the robust discretization of shock waves arising in the matter as well as for the stable treatment of puncture black holes. We test the new method on a set of classical test problems of numerical general relativity, showing good agreement with available exact or numerical reference solutions. In particular, we perform the first long term evolution of the inspiralling merger of two puncture black holes with a high order ADER-DG scheme.<|reference_end|>
@article{dumbser2024high-order,
    title={High-order discontinuous Galerkin schemes with subcell finite volume
  limiter and adaptive mesh refinement for a monolithic first-order BSSNOK
  formulation of the Einstein-Euler equations},
    author={Michael Dumbser, Olindo Zanotti, Ilya Peshkov},
    journal={Physical Review D, Volume 110, 084015 (2024)},
    year={2024},
    doi={10.1103/PhysRevD.110.084015},
    archivePrefix={arXiv},
    eprint={2406.15798},
    primaryClass={gr-qc astro-ph.HE cs.NA math.NA}
}