메뉴 건너뛰기




Volumn 53, Issue 12, 1996, Pages 6749-6761

Search templates for gravitational waves from inspiraling binaries: Choice of template spacing

Author keywords

[No Author keywords available]

Indexed keywords


EID: 0000903765     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.53.6749     Document Type: Article
Times cited : (503)

References (28)
  • 1
    • 0001912696 scopus 로고
    • edited by S. W. Hawking and W. Israel, Cambridge University Press, Cambridge, England
    • K. S. Thorne, in 300 Years of Gravitation, edited by S. W. Hawking and W. Israel (Cambridge University Press, Cambridge, England, 1987), p. 330.
    • (1987) 300 Years of Gravitation , pp. 330
    • Thorne, K.S.1
  • 16
    • 85035224930 scopus 로고    scopus 로고
    • Omitted end note
    • Omitted end note.
  • 17
    • 0012256290 scopus 로고
    • edited by D. Blair, Cambridge University Press, Cambridge, England
    • B. F. Schutz, in The Detection of Gravitational Radiation, edited by D. Blair (Cambridge University Press, Cambridge, England, 1989).
    • (1989) The Detection of Gravitational Radiation
    • Schutz, B.F.1
  • 19
    • 85035237152 scopus 로고    scopus 로고
    • Note that the, which is used by Cutler and Flanagan in Ref. 15
    • Note that the, which is used by Cutler and Flanagan in Ref. 15.
  • 20
    • 85035200807 scopus 로고    scopus 로고
    • preparation, also L. S. Finn (in preparation)
    • S. V. Dhurandhar and S. D. Mohanty (in preparation); also L. S. Finn (in preparation).
    • Dhurandhar, S.V.1    Mohanty, S.D.2
  • 21
    • 85035234231 scopus 로고    scopus 로고
    • Omitted end note
    • Omitted end note.
  • 23
    • 85035208627 scopus 로고    scopus 로고
    • The given here are different from those given in Eq. (13a-e) of Ref. 14 because Sathyaprakash does not use as kinematical parameters, but rather the time and phase at which the quadrupole part of the wave form reaches a frequency of
    • The given here are different from those given in Eq. (13a-e) of Ref. 14 because Sathyaprakash does not use as kinematical parameters, but rather the time and phase at which the quadrupole part of the wave form reaches a frequency of.
  • 26
    • 85035195605 scopus 로고    scopus 로고
    • Omitted end note
    • Omitted end note.
  • 27
    • 85035223573 scopus 로고    scopus 로고
    • Omitted end note
    • Omitted end note.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.