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Cited by 1,248

The DOI matches its Crossref record; 13 of the 13 references it cites were found in a registry or an index.

Numerical integration of Einstein’s field equations

Open access
Baumgarte, Thomas W., Shapiro, Stuart L.·1998·Physical Review D

Abstract

Many numerical codes now under development to solve Einstein's equations of general relativity in $(3+1)$-dimensional spacetimes employ the standard ADM form of the field equations. This form involves evolution equations for the raw spatial metric and extrinsic curvature tensors. Following Shibata and Nakamura, we modify these equations by factoring out the conformal factor and introducing three ``connection functions.'' The evolution equations can then be reduced to wave equations for the conformal metric components, which are coupled to evolution equations for the connection functions. We evolve small amplitude gravitational waves and make a direct comparison of the numerical performance of the modified equations with the standard ADM equations. We find that the modified form exhibits much improved stability.

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Metadata

Authors
Baumgarte, T. W., & Shapiro, S. L.
Venue
Physical Review D
Published
1998-12-07
Volume
59
Issue
2
ISSN
  • 0556-2821 (ISSN-L)
  • 1089-4918
OpenAlex
W2104853465
Cited by
1,248
References
13
FWCI
11.54
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Numerical integration of Einstein’s field equations. https://app.cochat.ai/papers/10.1103/physrevd.59.024007
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Baumgarte, T. W., & Shapiro, S. L. (1998). Numerical integration of Einstein’s field equations. Physical Review D. https://doi.org/10.1103/physrevd.59.024007

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