Gravitational radiation from inspiralling compact binaries completed at the third post-Newtonian order

Physical Review Letters

Volumn 93, Issue 9, 2004, Pages

  Blanchet, Luc ^a   Damour, Thibault ^b   Esposito Farèse, Gilles ^a   Iyer, Bala R ^c  

^a CNRS   (France)

^b INSTITUT DES HAUTES ÉTUDES SCIENTIFIQUES   (France)

^c RAMAN RESEARCH INSTITUTE   (India)

Author keywords

[No Author keywords available]

Indexed keywords

APPROXIMATION THEORY; COALESCENCE; COMPUTATIONAL METHODS; EQUATIONS OF MOTION; GRAVITATIONAL EFFECTS; INTEGRATION; NEUTRONS; RADIATION EFFECTS; SET THEORY; ULTRAVIOLET RADIATION;

GRAVITATIONAL RADIATIONS; INSPIRALLING COMPACT BINARIES (ICB); NEWTONIAN APPROXIMATION; STRESS-ENERGY TENSOR; WAVE DETECTORS;

NEWTONIAN FLOW;

EID: 19544379158     PISSN: 00319007     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevLett.93.091101     Document Type: Article

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