Can the post-Newtonian gravitational waveform of an inspiraling binary be improved by solving the energy balance equation numerically?

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 61, Issue 10, 2000, Pages

  Poisson, Eric ^b   Flanagan, Éanna É ^a  

^a Cornell University ^*  (United States)

^b UNIVERSITY OF GUELPH   (Canada)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 17144372256     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.61.104015     Document Type: Article

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