Gravitational wave trains in the quasiequilibrium approximation: A model problem in scalar gravitation

Physical Review D

Volumn 63, Issue 6, 2001, Pages

  Yo, Hwei Jang ^a   Baumgarte, Thomas W ^a   Shapiro, Stuart L ^a  

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

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; COSMOS; DYNAMICS; GRAVITY; MATHEMATICAL MODEL; WAVEFORM;

EID: 0034898319     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.63.064035     Document Type: Article

References (19)

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18. It should be noted, however, that the monopole formula in scalar gravitation, like the quadrupole formula in GR, is only the lowest order term in a multipole expansion. Post-Newtonian expansions for the binary inspirai problem in GR have been developed well past the quadrupole approximation. In [3], for example, such binaries are constructed at the third post-Newtonian level. Also, a post-Newtonian "effective-one-body" method has recently been applied to the inspiral even inside the ISCO [A. Buonanno and T. Damour, Phys. Rev. D 62, 064015 (2000)].
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