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Volumn 77, Issue 22, 1996, Pages 4483-4486

Colliding Black Holes: How far can the close approximation go?

Author keywords

[No Author keywords available]

Indexed keywords


EID: 6244277143     PISSN: 00319007     EISSN: 10797114     Source Type: Journal    
DOI: 10.1103/PhysRevLett.77.4483     Document Type: Article
Times cited : (125)

References (12)
  • 1
    • 0000212414 scopus 로고
    • PRVDAQ
    • L. S. Finn, Phys. Rev. D 46, 5236 (1992). PRVDAQ
    • (1992) Phys. Rev. D , vol.46 , pp. 5236
    • Finn, L.S.1
  • 2
    • 0004251401 scopus 로고
    • L. Smarr (Cambridge University Press, Cambridge, England
    • L. Smarr, in Sources of Gravitational Radiation, L. Smarr (Cambridge University Press, Cambridge, England, 1979), p. 245.
    • (1979) Sources of Gravitational Radiation , pp. 245
    • Smarr, L.1
  • 7
    • 36149018604 scopus 로고
    • PHRVAO
    • C. Misner, Phys. Rev. 118, 1110 (1960). PHRVAO
    • (1960) Phys. Rev , vol.118 , pp. 1110
    • Misner, C.1
  • 10
    • 0002331213 scopus 로고
    • e.g., K. Tomita
    • This feature of second-order perturbation theory is pointed out in, e.g., K. Tomita, Prog. Theor. Phys. 52, 1188 (1974).
    • (1974) Prog. Theor. Phys. , vol.52 , pp. 1188


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.