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Volumn 57, Issue 2, 1998, Pages 876-884

Spin effects in gravitational radiation back reaction. I. The Lense-Thirring approximation

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EID: 0040774903     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.57.876     Document Type: Article
Times cited : (35)

References (20)
  • 6
    • 0002833153 scopus 로고
    • The computations of 4 have been extended to the (Formula presented) approximation by L. Kidder, Phys. Rev. D 52, 821 (1995).
    • (1995) Phys. Rev. D , vol.52 , pp. 821
    • Kidder, L.1
  • 12
    • 85037241783 scopus 로고    scopus 로고
    • L. Á. Gergely and Z. Perjés, in Proceedings of the Virgo Conference, edited by I. Ciufolini and F. Fidecaro (World Scientific, Singapore, 1997)
    • L. Á. Gergely and Z. Perjés, in Proceedings of the Virgo Conference, edited by I. Ciufolini and F. Fidecaro (World Scientific, Singapore, 1997).
  • 15
    • 85037182157 scopus 로고    scopus 로고
    • L. Á. Gergely, Z. Perjés, and M. Vasúth (in preparation)
    • L. Á. Gergely, Z. Perjés, and M. Vasúth (in preparation).
  • 16
    • 85037191035 scopus 로고    scopus 로고
    • The parametrization of the Kepler orbit by the angle χ is close in spirit to Ptolemy’s idea of the equant. Both the equant and the orbit parameter are means for setting up a rule for determining the angular velocity of the orbiting body
    • The parametrization of the Kepler orbit by the angle χ is close in spirit to Ptolemy’s idea of the equant. Both the equant and the orbit parameter are means for setting up a rule for determining the angular velocity of the orbiting body.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.