The DOI matches its Crossref record; 2 of the 2 references it cites were found in a registry or an index.
Extrinsic curvature and the Einstein constraints
Open accessAbstract
The Einstein initial-value equations in the extrinsic curvature (Hamiltonian) representation and conformal thin sandwich (Lagrangian) representation are brought into complete conformity by the use of a decomposition of symmetric tensors which involves a weight function. In stationary spacetimes, there is a natural choice of the weight function such that the transverse traceless part of the extrinsic curvature (or canonical momentum) vanishes.
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Citations
Cites
Role of Conformal Three-Geometry in the Dynamics of Gravitation
York, J. W. (1972) · Physical Review Letters · doi:10.1103/physrevlett.28.1082 · Cited by 1,392
Self-citationNew Hamiltonian formulation of general relativity
Ashtekar, A. (1987) · Physical Review D · doi:10.1103/physrevd.36.1587 · Cited by 1,119
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The SXS collaboration catalog of binary black hole simulations
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Self-citationCalibration of moving puncture simulations
Brügmann, B., González, J. A., Hannam, M., Husa, S., Sperhake, U., & Tichy, W. (2008) · Physical Review D · doi:10.1103/physrevd.77.024027 · Cited by 388
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Metadata
- Authors
- Pfeiffer, H. P., & York, J. W.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 2003-02-28
- Volume
- 67
- Issue
- 4
- ISSN
- 0556-2821 (ISSN-L)
- 1089-4918
- OpenAlex
- W1999032058
- Cited by
- 238
- References
- 2
- FWCI
- 5.80
- Type
- journal article
- Language
- en
- Open access
- green
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- Pfeiffer, H. P., & York, J. W. (2003). Extrinsic curvature and the Einstein constraints. Physical Review D. https://doi.org/10.1103/physrevd.67.044022
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