@article{AIHPA_1989__50_4_377_0,
author = {Blanchet, Luc and Damour, Thibault},
title = {Post-newtonian generation of gravitational waves},
journal = {Annales de l'I.H.P. Physique th\'eorique},
volume = {51},
year = {1989},
pages = {377-408},
mrnumber = {1027227},
zbl = {0684.53059},
language = {en},
url = {http://dml.mathdoc.fr/item/AIHPA_1989__50_4_377_0}
}
Blanchet, Luc; Damour, Thibault. Post-newtonian generation of gravitational waves. Annales de l'I.H.P. Physique théorique, Tome 51 (1989) pp. 377-408. http://gdmltest.u-ga.fr/item/AIHPA_1989__50_4_377_0/
[1] For a recent general introduction to gravitational wave research see K. S. THORNE, in 300 Years of Gravitation, S. W. HAWKING and W. ISRAEL Eds., Cambridge University Press, Cambridge, England, 1987, pp. 330-458. | Zbl 0966.83515
[2] and , Astrophys. J., Vol. 215, 1977, p. 311; , in Gravitational Collapse and Relativity, H. SATO and T. NAKAMURA Ed., World Scientific, Singapore, 1986, pp. 350-368; and , Gen. Relativ. Gravit., Vol. 19, p. 1163, 1987.
[3] and , in Dynamical Spacetimes and Numerical Relativity, J. M. CENTRELLA, Ed., Cambridge University Press, Cambridge, England, 1986, p. 389; , in Gravitational Collapse and Relativity, H. SATO and T. NAKAMURA, Eds., World Scientific, Singapore, 1986, pp. 63-73. | MR 945480
[4] and , Astrophys. J., Vol. 253, 1982, p. 908; and , Phys. Rev. Lett., Vol. 52, 1984, p. 1348; , in Timing Neutron Stars, H. ÖGELMAN and E. P. J. VAN DEN HEUVEL, Eds., Kluwer, Dordrecht, 1989, p. 17.
[5] For a review and references, see , in 300 Years of Gravitation, S. W. HAWKING and W. ISRAEL Eds., Cambridge University Press, Cambridge, England, 1987, pp. 128-198.
[6] , Preuss. Akad. Wiss. Sitzber. (Berlin), 1918, p. 154. | JFM 46.1295.02
[8] We are following the terminology of T. DAMOUR, in Gravitation in Astrophysics, Cargèse, 1986, B. CARTER and J. B. HARTLE, Eds., Plenum, New York, 1987, pp. 3-62.
[9] and , Teoriya Polya, Nauka, Moscow, 1941.
[10] , Teoriya prostranstva. vremeni i tyagoteniya, Fizmatgiz, Moscow, 1955.
[11] and , Phys. Rev. Lett., Vol. 45, 1980, p. 1741; , Phys. Rev. Lett., Vol. 45, 1980, p.1745; , Astrophys. J., Vol. 250, 1981, p. L5; , and , Phys. Rev. Lett., Vol. 53, 1984, p. 1870; and , Phys. Rev. Lett., Vol. 55, 1985, p.265; and , Phys. Rev. D., Vol. 32, 1985, p.2557; , J. Math. Phys., Vol. 28, 1987, p. 668. | MR 593290
[12] and , Astrophys. J., Vol. 197, 1975, p. 717; , in Gravitazione Sperimentale, B. BERTOTTI Ed., Accademia Nazionale dei Lincei, Rome, 1977, p. 117. | MR 378687
[13] , Rev. Mod. Phys., Vol. 52, 1980, p. 299. | MR 569166
[14] and , Astrophys. J., Vol. 210, 1976, p.764; and , Astrophys. J., Vol. 220, 1978, p.1107; and , in Sources of Gravitational Radiation, L. SMARR Ed., Cambridge University Press, Cambridge, 1979, p. 383; , Phys. Rev. D, Vol. 19, 1979, p. 2897.
[16] , Sov. Astron., Vol. 28, 1984, p. 394.
[17] and , Phil. Trans. R. Soc. Lond. A, Vol. 320, 1986, p.379, hereafter referred to as paper I. | MR 874095 | Zbl 0604.35073
[18] , Proc. R. Soc. Lond. A, Vol. 409, 1987, p. 383, hereafter referred to as paper II. | Zbl 0658.35084
[19] and , Phys. Rev. D, Vol. 37, 1988, p. 1410, hereafter referred to as paper III. See the introduction of paper III for references to previous contributions to the problem of the matching between the near-zone and the wave-zone gravitational fields.
[20] , and , Mon. Not. R. Astro. Soc., 1990 (in press); and , Mon. Not. R. Astro. Soc., Vol. 239, 1989, p. 845. | MR 1165749 | Zbl 0671.70009
[21] , J. Math. Phys., Vol. 12, 1971, p.401; , Astrophys. J., Vol. 158, 1969, p. 997.
[22] and , Phys. Lett., Vol. 104A, 1984, p. 82.
[23] , and , Phys. Rev. D, Vol. 15, 1977, p. 2156. | MR 469046
[24] , Phil. Trans. R. Soc. Lond. A, Vol. 251, 1959, p.233; and , Proc. R. Soc. Lond. A, Vol. 289, 1966, p. 247; and , J. Phys. A, Vol. 2, 1969, p. 34. | MR 101146 | Zbl 0084.43906
[25] and , Mon. Not. Roy. Astron. Soc., Vol. 203, 1983, p.457; , Mon. Not. R. Astr. Soc., Vol. 222, 1986, p. 393. | MR 702586
[27] , Singular Perturbations-Ideas and Techniques, Springer-Verlag, New York, 1989 (in press). | MR 958913