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Journal Article

Simulating magnetized neutron stars with discontinuous Galerkin methods

MPS-Authors
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Pfeiffer,  Harald P.
Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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Wittek,  Nikolas
Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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2109.12033.pdf
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Citation

Deppe, N., Hébert, F., Kidder, L. E., Throwe, W., Anantpurkar, I., Armaza, C., et al. (2022). Simulating magnetized neutron stars with discontinuous Galerkin methods. Physical Review D, 105(12): 123031. doi:10.1103/PhysRevD.105.123031.


Cite as: https://hdl.handle.net/21.11116/0000-000A-B3D6-A
Abstract
Discontinuous Galerkin methods are popular because they can achieve high
order where the solution is smooth, because they can capture shocks while
needing only nearest-neighbor communication, and because they are relatively
easy to formulate on complex meshes. We perform a detailed comparison of
various limiting strategies presented in the literature applied to the
equations of general relativistic magnetohydrodynamics. We compare the standard
minmod/$\Lambda\Pi^N$ limiter, the hierarchical limiter of Krivodonova, the
simple WENO limiter, the HWENO limiter, and a discontinuous
Galerkin-finite-difference hybrid method. The ultimate goal is to understand
what limiting strategies are able to robustly simulate magnetized TOV stars
without any fine-tuning of parameters. Among the limiters explored here, the
only limiting strategy we can endorse is a discontinuous
Galerkin-finite-difference hybrid method.