Coordinate conditions in three-dimensional numerical relativity

Classical and Quantum Gravity

Volumn 13, Issue 12, 1996, Pages

  Balakrishna, Jayashree ^a   Daues, Gregory ^a   Seidel, Edward ^b   Suen, Wai Mo ^a,b,c   Tobias, Malcolm ^a   Wang, Edward ^a  

^a WASHINGTON UNIVERSITY   (United States)

^b UNIVERSITY OF ILLINOIS AT URBANA CHAMPAIGN   (United States)

^c CHINESE UNIVERSITY OF HONG KONG   (Hong Kong)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 21444432992     PISSN: 02649381     EISSN: None     Source Type: Journal    
DOI: 10.1088/0264-9381/13/12/001     Document Type: Article

References (11)

1. Shapiro S L and Teukolsky S A 1986 Dynamical Spacetimes and Numerical Relativity ed J Centrella (Cambridge: Cambridge University Press)
2. Seidel E and Suen W-M 1992 Phys. Rev. Lett. 69 1845
3. Anninos P et al 1995 Phys. Rev. D 51 5562
4. Scheel M et al 1995 Phys. Rev. D 51 4208
5. Smarr L and York J 1978 Phys. Rev. D 17 2529
6. Anninos P et al 1995 Phys. Rev. D 52 2059
7. Seidel E and Suen W-M 1990 Phys. Rev. D 42 384
8. After finishing this study we noticed that Eppley K 1979 Sources of Gravitational Radiation ed L Smarr (Cambridge: Cambridge University Press) mentioned the addition of a term linear in K to equation (2), though without further analysis
9. Balakrishna J et al in preparation
10. Schutz B et al 1995 reported on using the constant γ condition to determine the shift vector in GR14, Florence, 1995
11. See e.g. Saylor P E and Smolarski C C 1991 Lin. Alg. App. 154 615 and references therein