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Volumn 62, Issue 12, 2000, Pages 1-20

Gravitational waves from a compact star in a circular, inspiral orbit, in the equatorial plane of a massive, spinning black hole, as observed by LISA

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Indexed keywords


EID: 18144430272     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.62.124021     Document Type: Article
Times cited : (205)

References (58)
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    • hSAΔf with Δf=1/1 yr, it falls between the lowest Webbink-Han estimate ("no wind enhancement" curve) and the highest ("standard model") and agrees to within a factor 2 with both - except for one issue: Webbink and Han do not take account of the cutoff in the noise due to the line spikes of individual white-dwarf binaries ceasing to overlap each other, for 1 yr of integration, at frequencies above about 0.0017 Hz, so their noise curves fail to plunge above there.
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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.