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Volumn 56, Issue 8, 1997, Pages 4449-4454

Gravitational waves from inspiraling compact binaries: Second post-Newtonian waveforms as search templates

Author keywords

[No Author keywords available]

Indexed keywords


EID: 0001396195     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.56.4449     Document Type: Article
Times cited : (23)

References (36)
  • 3
    • 0004259614 scopus 로고    scopus 로고
    • edited by D. G. Blair (Cambridge University Press, Cambridge, England, 1991), p. 406
    • For an overview, see B. F. Schutz, in The Detection of Gravitational Waves, edited by D. G. Blair (Cambridge University Press, Cambridge, England, 1991), p. 406.
    • The Detection of Gravitational Waves
    • Schutz, B.F.1
  • 12
    • 85038274016 scopus 로고    scopus 로고
    • 55, 7980 (1997).
    • (1997) , vol.55 , pp. 7980
  • 14
    • 85038344029 scopus 로고    scopus 로고
    • Here and below, the signal-to-noise ratio is defined to be the expectation value of the maximum correlation between the noisy detector output and the templates
    • Here and below, the signal-to-noise ratio is defined to be the expectation value of the maximum correlation between the noisy detector output and the templates.
  • 30
    • 0003811646 scopus 로고    scopus 로고
    • edited by S.W. Hawking and W. Israel (Cambridge University Press, Cambridge, England, 1987), p. 330
    • K.S. Thorne, in 300 Years of Gravitation, edited by S.W. Hawking and W. Israel (Cambridge University Press, Cambridge, England, 1987), p. 330.
    • 300 Years of Gravitation
    • Thorne, K.S.1
  • 33
    • 85038280204 scopus 로고    scopus 로고
    • The software is VIS5D, and is available free of charge from URL http://www.scsc.edu/(Formula presented)michaels/vizwiz.html
    • The software is VIS5D, and is available free of charge from URL http://www.scsc.edu/(Formula presented)michaels/vizwiz.html
  • 36
    • 85038334347 scopus 로고    scopus 로고
    • Cutler and Flanagan derived these results using a 1.5 PN wave form. We have recalculated the statistical uncertainties using a 2 PN waveform, and have found the same answer
    • Cutler and Flanagan derived these results using a 1.5 PN wave form. We have recalculated the statistical uncertainties using a 2 PN waveform, and have found the same answer.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.