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The Newtonian limit

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Part of the book series: Lecture Notes in Physics ((LNP,volume 205))

Abstract

We discuss in detail the development of the Newtonian and post-Newtonian approximations to general relativity. By using an initial-value approach, we are able to show that the post-Newtonian hierarchy through gravitational-radiation-reaction order is an asymptotic approximation to general relativity, thereby verifying the validity of the quadrupole formula for radiation reaction. We also show with equal rigor that the radiation from nearly-Newtonian systems obeys the far-field quadrupole formula (Landau-Lifshitz formula).There are no divergent terms in these approximations at any order, although logarithmic terms in the expansion parameter do appear at high order. We discuss the relationships of observables to post-Newtonian quantities by the method of osculating Newtonian orbits. Finally we discuss the role exact solutions may play in shedding light on some of these questions.

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References

  1. See for example, C. W. Misner, K. S. Thorne, & J. A. Wheeler, Gravitation (Freeman, San Francisco, 1973) or B. F. Schutz, A First Course in General Relativity (Cambridge University Press, Cambridge, 1984). We adopt the sign and notation conventions of Misner, et al, op cit.

    Google Scholar 

  2. J. Ehlers, A. Rosenblum, J. N. Goldberg, & P. Havas, Astrophys. J. 208, L77 (1976).

    Google Scholar 

  3. E. Cartan, Ann. É cole Norm. Sup. 40, 325 (1923) and 41, 1 (1924); see Misner, et al, op cit. (ref. 1) for an exposition.

    Google Scholar 

  4. S. Chandresekhar, Astrophys. J. 142, 1488 (1965); S. Chandrasekhar & Y. Nutku, Astrophys. J. 158, 55 (1969); S. Chandrasekhar & E. P. Esposito, Astrophys. J. 160, 153 (1970). Radiation reaction itself was also studied at this time by W. L. Burke, J. Math. Phys. 12, 401 (1971).

    Google Scholar 

  5. See Misner, et al, op cit.(ref.1).

    Google Scholar 

  6. L. D. Landau & E. M. Lifshitz, Classical Theory of Fields (Addison-Wesley, Reading, Mass., 1971).

    Google Scholar 

  7. See for example G. D. Kerlick, Gen. Rel. Grav. 12, 467 and 521 (1980).

    Google Scholar 

  8. M. Walker & C. M. Will, Astrophys. J. 242, L129 (1980).

    Google Scholar 

  9. B. F. Schutz, Phys. Rev. D 22, 249 (1980).

    Google Scholar 

  10. T. Futamase & B. F. Schutz, Phys. Rev. D 28, 2363 (1983).

    Google Scholar 

  11. T. Futamase, Phys. Rev. D 28, 2373 (1983).

    Google Scholar 

  12. T. Futamase & B. F. Schutz (in preparation).

    Google Scholar 

  13. J. L. Anderson & T. C. Decanio, Gen. Rel. Grav. 6, 197 (1975).

    Google Scholar 

  14. Note that this formula was incorrectly written down in ref. 10. This had no effect on subsequent equations.

    Google Scholar 

  15. B. Paczynski, B. & R. Sienkiewicz, Astrophys. J. 268, 825 (1983)

    Google Scholar 

  16. S. Chandrasekhar, Phys. Rev. Lett. 24, 611 (1970); J. L. Friedman & B. F. Schutz, Astrophys. J. 222, 281 (1978).

    Google Scholar 

  17. E. F. L. Balbinski & B. F. Schutz, Mon. Not. R. astr. Soc. 200, 43P (1982)

    Google Scholar 

  18. R. A. Saenz & S. L. Shapiro, Astrophys. J. 221, 286 (1978) and 229, 1107 (1979).

    Google Scholar 

  19. J. H. Taylor & J. M. Weisberg, Astrophys. J. 253, 908 (1982); V. Boriakoff, D. C. Ferguson, M. P. Haugan, Y. Terzian & S. Teukolsky, Astrophys. J. 261, L101 (1982).

    Google Scholar 

  20. B. F. Schutz in X. Fustero & E. Verdaguer, eds., Relativistic Astrophysics and Cosmology (World Scientific Publishers, 1984), p.35.

    Google Scholar 

  21. B. F. Schutz, Mon. Not. R. astr. Soc. 207, 37P (1984).

    Google Scholar 

  22. H. Stephani, General Relativity (Cambridge University Press, Cambridge, 1982).

    Google Scholar 

  23. R. A. Isaacson, Phys. Rev. 166, 1263 and 1272 (1968).

    Google Scholar 

  24. W. L. Burke, op cit.(ref.4); R. E. Kates, Phys. Rev. D 22, 1871 (1980); and J. L. Anderson, R. E. Kates, L. S. Kegeles & R. G. Madonna, Phys. Rev. D 25, 2038 (1982).

    Google Scholar 

  25. J. Winicour, J. Math. Phys. 24, 1193 (1983), and to be published.

    Google Scholar 

  26. Balbinski & Schutz, op cit. (ref. 16); and E. F. L. Balbinski, S. L. Detweiler, L. Lindblom, and B. F. Schutz, to be published.

    Google Scholar 

  27. T. Damour & N. Deruelle, C. R. Acad. Sci.Ser. B 293, II 5037 (1981)and 677 (1981); T. Damour in N. Deruelle and T. Piran, eds., Gravitational Radiation (North-Holland, Amsterdam, 1983), p.59.

    Google Scholar 

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C. Hoenselaers W. Dietz

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© 1984 Springer-Verlag

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Schutz, B.F. (1984). The Newtonian limit. In: Hoenselaers, C., Dietz, W. (eds) Solutions of Einstein's Equations: Techniques and Results. Lecture Notes in Physics, vol 205. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-13366-6_17

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  • DOI: https://doi.org/10.1007/3-540-13366-6_17

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-13366-7

  • Online ISBN: 978-3-540-38922-4

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