Author： Avagyan R.M. Yeranyan A.H.
Publisher： Springer Publishing Company
ISSN： 0571-7256
Source： Astrophysics, Vol.43, Iss.4, 2000-10, pp. : 482-486
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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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