Abstract
Gravitational radiation in a variant of the bimetric theory of gravitation is investigated in the case of slow motions and weak fields. Questions of the propagation velocity, polarization, and generation of a weak gravitational wave are considered. The Peters-Matthews coefficients and the dipole emission coefficient are determined.
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REFERENCES
R. M. Avagyan (Avakian) and L. Sh. Grigorian, Astrophys. Space Sci., 146, 183 (1988).
R. M. Avagyan and A. H. Yeranyan, Astrofizika, 43, 303 (2000).
R. M. Avagyan and A. H. Yeranyan, Astrofizika, 43, 493 (2000).
C. M. Will, Theory and Experiment in Gravitational Physics, Cambridge Univ. Press, Cambridge, Eng.ñNew York (1981).
G. S. Sahakyan, SpaceñTime and Gravitation [in Russian], Erev. Gos. Univ., Yerevan (1985).
A. A. Logunov and M. A. Mestvirishvili, Relativistic Theory of Gravitation [in Russian], Nauka, Moscow (1989).
N. Rosen, Ann. Phys., 84, 455 (1974).
D. M. Eardley and D. L. Lee, Phys. Rev., D8, 3308 (1973).
L. D. Landau and E. M. Lifshitz, Field Theory [in Russian], Nauka, Moscow (1988) [The Classical Theory of Fields, 4th ed., Pergamon Press, New York (1976)].
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Avagyan, R.M., Yeranyan, A.H. Variant of the Bimetric Theory of Gravitation. III. Gravitational Radiation. Astrophysics 43, 482–486 (2000). https://doi.org/10.1023/A:1010979211002
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DOI: https://doi.org/10.1023/A:1010979211002