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Volumn 74, Issue 18, 1995, Pages 3515-3518

Gravitational-radiation damping of compact binary systems to second post-Newtonian order

Author keywords

[No Author keywords available]

Indexed keywords


EID: 0000317659     PISSN: 00319007     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevLett.74.3515     Document Type: Article
Times cited : (511)

References (45)
  • 12
    • 84927481941 scopus 로고
    • in 300 Years of Gravitation, S. W. Hawking, Canbridge University Press, Cambridge, p. 406, B. F. Schutz, in The Detection of Gravitational Waves, edited by, D. G. Blair, Cambridge University Press, Cambridge
    • (1987) , pp. 330
    • Thorne, K.S.1    Israel, W.2
  • 13
    • 84927460325 scopus 로고
    • in Relativistic Cosmology, M. Sasaki, Universal Academy Press, Tokyo
    • (1994) , pp. 83
    • Will, C.M.1
  • 15
    • 84927477233 scopus 로고
    • (1977) , vol.215 , pp. 984
  • 22
    • 84927477870 scopus 로고    scopus 로고
    • In the presence of spin-dependent interactions, a circular orbit only exists as an approximation; the formulas presented here are averaged over one orbit. The only other effects that might contribute are finite-size, quadrupole effects; these would be significant only for fast-rotating compact bodies, for which they scale as (R0/r)2∼(m/r)2, i.e., 2PN relative to Newtonian order, where R0∼m is the size of the compact body. However, they enter via the equations of motion, not via the radiation field at 2PN order.
  • 27


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.