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Volumn 52, Issue 10, 1995, Pages 5719-5723

Gravitational radiation from a particle in circular orbit around a black hole. VI. Accuracy of the post-Newtonian expansion

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EID: 0000259920     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.52.5719     Document Type: Article
Times cited : (122)

References (33)
  • 24
    • 0000640046 scopus 로고
    • Perturbations of a Rotating Black Hole. I. Fundamental Equations for Gravitational, Electromagnetic, and Neutrino-Field Perturbations
    • (1973) The Astrophysical Journal , vol.185 , pp. 635
    • Teukolsky, S.A.1
  • 26
    • 84927877761 scopus 로고    scopus 로고
    • The term of order v5, complete with its μ/M dependence, was recently calculated using post Newtonian theory by Luc Blanchet (personal communication).
  • 28
    • 84927877760 scopus 로고    scopus 로고
    • For such an analysis, see C. Cutler and É.E. Flanagan, (in preparation).
  • 29
    • 0001277843 scopus 로고
    • The stationary phase approximation introduces an error of order μ v5/M into the Fourier transform of the waveform. [See,] This error is always negligible in the limit μ/M to 0. However, corrections to the stationary phase approximation will play a role in the case of binary systems with large mass ratios.
    • (1994) Phys. Rev. D , vol.49 , pp. 6274
    • Apostolatos, T.A.1    Cutler, C.2    Sussman, G.J.3    Thorne, K.S.4
  • 30
    • 84927877759 scopus 로고    scopus 로고
    • We have used fortran subroutines from W.H. Press, S.A. Teukolsky, W.T. Vetterling, and B.P. Flannery, Numerical Recipes (Cambridge University Press, Cambridge, England, 1992).


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.