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Volumn 57, Issue 2, 1998, Pages 885-907

Improved filters for gravitational waves from inspiraling compact binaries

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EID: 0000614545     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.57.885     Document Type: Article
Times cited : (348)

References (34)
  • 15
    • 85037210411 scopus 로고    scopus 로고
    • The most accuracy-demanding case is the wave form emitted by a binary system made of a (Formula presented) neutron star and a (Formula presented) black hole
    • The most accuracy-demanding case is the wave form emitted by a binary system made of a (Formula presented) neutron star and a (Formula presented) black hole 1114.
  • 18
    • 0001630137 scopus 로고
    • in Gravitational Radiation, edited by N. Deruelle and T. Piran (North-Holland, Amsterdam, 1983), pp. 59–144
    • C. R. Seances Acad. Sci., Ser. 2T. Damour, 294, 1355 (1982);in Gravitational Radiation, edited by N. Deruelle and T. Piran (North-Holland, Amsterdam, 1983), pp. 59–144.
    • (1982) C. R. Seances Acad. Sci., Ser. 2 , vol.294 , pp. 1355
    • Damour, T.1
  • 26
    • 85037224555 scopus 로고    scopus 로고
    • Note that we consistently label the successive approximants by the order in velocity. E.g. a 2PN-accurate object has the label 4
    • Note that we consistently label the successive approximants by the order in velocity. E.g. a 2PN-accurate object has the label 4.
  • 28
    • 85037227880 scopus 로고    scopus 로고
    • E.g., if one factorized out the log factors in the flux function of Eq. (4.1) as in Eq. (4.5), (Formula presented)(Formula presented)then the corresponding coefficients (Formula presented) are given by (Formula presented). The (Formula presented) are as given by Eq. (4.9)
    • E.g., if one factorized out the log factors in the flux function of Eq. (4.1) as in Eq. (4.5), (Formula presented)(Formula presented)then the corresponding coefficients (Formula presented) are given by (Formula presented). The (Formula presented) are as given by Eq. (4.9).
  • 34
    • 85037243782 scopus 로고    scopus 로고
    • The problem of phase maximization was first considered by Schutz for the case of two wave forms which both have the same shape: B. F. Schutz, in The Detection of Gravitational Radiation, edited by D. Blair (Cambridge, University Press, Cambridge, England, 1989), pp. 406–427 (also see Ref
    • The problem of phase maximization was first considered by Schutz for the case of two wave forms which both have the same shape: B. F. Schutz, in The Detection of Gravitational Radiation, edited by D. Blair (Cambridge, University Press, Cambridge, England, 1989), pp. 406–427 (also see Ref. 38). Here we are addressing the problem of maximization over phase when the signal and the template wave forms belong to different post-Newtonian families.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.