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Volumn 67, Issue 2, 2003, Pages

Detection template families for gravitational waves from the final stages of binary - Black-hole inspirais: Nonspinning case

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; COSMIC RADIATION; COSMOS; GRAVITY; MATHEMATICAL ANALYSIS; MOLECULAR DYNAMICS; PHYSICAL PARAMETERS; SIGNAL DETECTION; WAVEFORM;

EID: 33751358820     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.67.024016     Document Type: Article
Times cited : (36)

References (97)
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    • note
    • Parameters that are not extrinsic are known as intrinsic. This nomenclature was introduced by Owen [29], but the underlying concept had been present in the data-analysis literature for a long time (see, e. g., [33]). Sathyaprakash [39] draws the same distinction between kinematical and dynamical parameters.
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    • note
    • The amplitude of the measured gravity-wave signals depends not only on the actual distance to the source, but also on the reciprocal orientation between the detector and the direction of propagation of the waves. A combination of several detectors will be needed, in general, to evaluate the distance to a gravity-wave source starting from the signal-to-noise ratio alone.
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    • note
    • ψ=0.98, the overlaps between the neighboring detection templates are well described by the metric. However, due to the fact we do not know the true waveforms, and thus the true FF, it is not quite certain how exact this formula will eventually be. In some sense, this formula could be regarded an additional assumption.
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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.