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Lessons for adaptive mesh refinement in numerical relativity

Abstract:
We demonstrate the flexibility and utility of the Berger-Rigoutsos adaptive mesh refinement (AMR) algorithm used in the open-source numerical relativity (NR) code GRChombo for generating gravitational waveforms from binary black-hole (BH) inspirals, and for studying other problems involving non-trivial matter configurations. We show that GRChombo can produce high quality binary BH waveforms through a code comparison with the established NR code Lean. We also discuss some of the technical challenges involved in making use of full AMR (as opposed to, e.g. moving box mesh refinement), including the numerical effects caused by using various refinement criteria when regridding. We suggest several ‘rules of thumb’ for when to use different tagging criteria for simulating a variety of physical phenomena. We demonstrate the use of these different criteria through example evolutions of a scalar field theory. Finally, we also review the current status and general capabilities of GRChombo.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1088/1361-6382/ac6fa9

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Role:
Author
ORCID:
0000-0001-8861-2025
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Role:
Author
ORCID:
0000-0002-3134-7088
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Role:
Author
ORCID:
0000-0001-8252-602X
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Institution:
University of Oxford
Role:
Author
ORCID:
0000-0001-8841-1522
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Role:
Author
ORCID:
0000-0001-6438-315X


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Funder identifier:
10.13039/100010663
Grant:
639022
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Funder identifier:
10.13039/501100000271
Grant:
ST/P000673/1
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Funder identifier:
10.13039/100000104
Grant:
17-ATP17-0225
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Funder identifier:
10.13039/100000086
Grant:
AST-2006538
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Funder identifier:
10.13039/501100001943
Grant:
2020225359


Publisher:
IOP Publishing
Journal:
Classical and Quantum Gravity More from this journal
Volume:
39
Issue:
13
Pages:
135006-135006
Publication date:
2022-05-13
DOI:
EISSN:
1361-6382
ISSN:
0264-9381


Language:
English
Keywords:
Pubs id:
1265144
Local pid:
pubs:1265144
Source identifiers:
W4280549243
Deposit date:
2026-04-24
ARK identifier:
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