메뉴 건너뛰기




Volumn 55, Issue 8, 1997, Pages 4848-4859

Chaos in Schwarzschild spacetime: The motion of a spinning particle

Author keywords

[No Author keywords available]

Indexed keywords


EID: 0001693720     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.55.4848     Document Type: Article
Times cited : (207)

References (44)
  • 8
    • 85038343015 scopus 로고
    • A435, 551 (1991).
    • (1991) , vol.A435 , pp. 551
  • 17
    • 84914783674 scopus 로고    scopus 로고
    • edited by S. W. Hawking and W. Israel (Cambridge University Press, Cambridge, England, 1987), p. 128
    • For a review, see, e.g., T. Damour, in 300 Years of Gravitation, edited by S. W. Hawking and W. Israel (Cambridge University Press, Cambridge, England, 1987), p. 128.
    • 300 Years of Gravitation
    • Damour, T.1
  • 18
    • 85038275312 scopus 로고    scopus 로고
    • C. M. Will, Report No. WUGRAV-94-3, (unpublished).
    • Will, C.M.1
  • 26
    • 85038309911 scopus 로고
    • A319, 509 (1970);
    • (1970) , vol.A319 , pp. 509
  • 27
    • 17144375956 scopus 로고
    • GRGVA8
    • Gen. Relativ. Gravit.4, 193 (1973); GRGVA8
    • (1973) Gen. Relativ. Gravit. , vol.4 , pp. 193
  • 28
    • 0001925949 scopus 로고
    • Isolated Gravitating Systems in General Relativity, edited by J. Ehlers (North-Holland, Amsterdam, 1979), p. 156
    • Philos. Trans. R. Soc. London 277, 59 (1974); in Isolated Gravitating Systems in General Relativity, edited by J. Ehlers (North-Holland, Amsterdam, 1979), p. 156.
    • (1974) Philos. Trans. R. Soc. London , vol.277 , pp. 59
  • 39
    • 85038276317 scopus 로고
    • A385, 229 (1983).
    • (1983) , vol.A385 , pp. 229
  • 43
    • 85038303571 scopus 로고    scopus 로고
    • To find a nonsingular “effective potential,” (Formula presented) should be smaller than (Formula presented)
    • To find a nonsingular “effective potential,” (Formula presented) should be smaller than (Formula presented).
  • 44
    • 0000941103 scopus 로고
    • Recently, it has been pointed out that deformation of a neutron star by a tidal force may change the innermost stable orbit in a binary system [see Lai, F. A. Raiso, and S. L. Shapiro, Astrophys. J.420, 811 (1994)]. It is one of the most important effects on observation of gravitational waves.
    • (1994) Astrophys. J. , vol.420 , pp. 811
    • Raiso, F.A.1    Shapiro, S.L.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.