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Volumn 60, Issue 10, 1999, Pages

Robust evolution system for numerical relativity

Author keywords

[No Author keywords available]

Indexed keywords


EID: 18144384792     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.60.104014     Document Type: Article
Times cited : (38)

References (28)
  • 1
    • 85037214182 scopus 로고    scopus 로고
    • An up-to-date overview of the Binary Black Hole Grand Challenge Alliance can be found on the web page URL www.npac.syr.edu/projects/bh/
    • An up-to-date overview of the Binary Black Hole Grand Challenge Alliance can be found on the web page URL www.npac.syr.edu/projects/bh/
  • 2
    • 85037247397 scopus 로고    scopus 로고
    • An up-to-date overview of the NASA Neutron Star Grand Challenge can be found on the web page URL www.wugrav.wustl.edu/Relativ/nsgc.html
    • An up-to-date overview of the NASA Neutron Star Grand Challenge can be found on the web page URL www.wugrav.wustl.edu/Relativ/nsgc.html
  • 5
    • 85037251538 scopus 로고    scopus 로고
    • R. Arnowitt, S. Deser, and C. W. Misner, in Gravitation: An Introduction to Current Research
    • R. Arnowitt, S. Deser, and C. W. Misner, in Gravitation: An Introduction to Current Research 4.
  • 17
    • 0004251401 scopus 로고
    • Cambridge University Press, Cambridge, England, L. Smarr
    • J. W. York, Jr., in Sources of Gravitational Radiation, edited by L. Smarr (Cambridge University Press, Cambridge, England, 1979).
    • (1979) Sources of Gravitational Radiation
    • York, J.W.1
  • 24
    • 85037206269 scopus 로고    scopus 로고
    • Notice that Φ, (Formula presented) (Formula presented) are three-dimensional tensorial densities (not tensors) and the corresponding Lie derivatives must be computed accordingly
    • Notice that Φ, (Formula presented) (Formula presented) are three-dimensional tensorial densities (not tensors) and the corresponding Lie derivatives must be computed accordingly.


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