A positivity-preserving adaptive-order finite-difference scheme for GRMHD

Fuente: arXiv
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Main Authors: Deppe, Nils, Kidder, Lawrence E., Teukolsky, Saul A., Bonilla, Marceline S., Hébert, François, Kim, Yoonsoo, Scheel, Mark A., Throwe, William, Vu, Nils L.
Format: Preprint
Published: 2023
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author Deppe, Nils
Kidder, Lawrence E.
Teukolsky, Saul A.
Bonilla, Marceline S.
Hébert, François
Kim, Yoonsoo
Scheel, Mark A.
Throwe, William
Vu, Nils L.
author_facet Deppe, Nils
Kidder, Lawrence E.
Teukolsky, Saul A.
Bonilla, Marceline S.
Hébert, François
Kim, Yoonsoo
Scheel, Mark A.
Throwe, William
Vu, Nils L.
contents We present an adaptive-order positivity-preserving conservative finite-difference scheme that allows a high-order solution away from shocks and discontinuities while guaranteeing positivity and robustness at discontinuities. This is achieved by monitoring the relative power in the highest mode of the reconstructed polynomial and reducing the order when the polynomial series no longer converges. Our approach is similar to the multidimensional optimal order detection (MOOD) strategy, but differs in several ways. The approach is a priori and so does not require retaking a time step. It can also readily be combined with positivity-preserving flux limiters that have gained significant traction in computational astrophysics and numerical relativity. This combination ultimately guarantees a physical solution both during reconstruction and time stepping. We demonstrate the capabilities of the method using a standard suite of very challenging 1d, 2d, and 3d general relativistic magnetohydrodynamics test problems.
format Preprint
id arxiv_https___arxiv_org_abs_2306_04755
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle A positivity-preserving adaptive-order finite-difference scheme for GRMHD
Deppe, Nils
Kidder, Lawrence E.
Teukolsky, Saul A.
Bonilla, Marceline S.
Hébert, François
Kim, Yoonsoo
Scheel, Mark A.
Throwe, William
Vu, Nils L.
High Energy Astrophysical Phenomena
General Relativity and Quantum Cosmology
We present an adaptive-order positivity-preserving conservative finite-difference scheme that allows a high-order solution away from shocks and discontinuities while guaranteeing positivity and robustness at discontinuities. This is achieved by monitoring the relative power in the highest mode of the reconstructed polynomial and reducing the order when the polynomial series no longer converges. Our approach is similar to the multidimensional optimal order detection (MOOD) strategy, but differs in several ways. The approach is a priori and so does not require retaking a time step. It can also readily be combined with positivity-preserving flux limiters that have gained significant traction in computational astrophysics and numerical relativity. This combination ultimately guarantees a physical solution both during reconstruction and time stepping. We demonstrate the capabilities of the method using a standard suite of very challenging 1d, 2d, and 3d general relativistic magnetohydrodynamics test problems.
title A positivity-preserving adaptive-order finite-difference scheme for GRMHD
topic High Energy Astrophysical Phenomena
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2306.04755