Causality principle in the relativistic theory of gravitation

Institute of High Energy Physics, Serpukhov. Translated from Teoreticheskaya i Matematicheskaya Fizika, Vol. 88, No. 3, pp. 459–466, September, 1991.     

The fundamental principles of the relativistic theory of gravitation

Moscow State University. Translated from Teoreticheskaya i Matematicheskaya Fizika, Vol. 86, No. 1, pp. 3–15, January, 1991.     

Spherical gravitational waves in the relativistic theory of gravitation

The conservation laws are used to find the dependence of the energy transported by a spherical gravitation disturbance (emitted by a centrally symmetric body on the transition between two static states) on the distance from the source. The observability of such a wave is discussed.N. A. Voznesenskii Leningrad Finance and Economics Institute. Translated from Teoreticheskaya i Matematicheskaya Fizika, Vol. 91, No. 2, pp. 346–352, May, 1992.     

Solution of the equations of the relativistic theory of gravitation for equilibrium massive bodies with allowance for their equations of state

The solutions of the equations of the relativistic theory of gravitation that describe the equilibrium state of a spherically symmetric isolated massive body are analyzed. It is shown that if the mass of the body is greater than the critical value equilibrium states do not exist; the minimum sizes of such bodies are always greater than the Schwarzschild sizes. We investigate the equilibrium sizes, the structure of the exterior gravitational field, and the distributions of the interior pressures and densities in the case of characteristic astrophysical objects such as the earth, Jupiter, the sun, neutron stars, and white dwarfs. The results agree satisfactorily with observations.Moscow State University. Translated from Teoreticheskaya i Matematicheskaya Fizika, Vol. 94, No. 1, pp. 122–139, January, 1993.     

On the constraint equation in the relativistic theory of gravitation

Expressions for covariant and contravariant components of the metric tensor for the effective Riemann space-time and for its determinant are constructed on the basis of the relations of tensor algebra.Translated from Teoreticheskaya i Matematicheskaya Fizika, Vol. 105, No. 3, pp. 508–511, December, 1995.     

Centrally symmetric problem in the relativistic theory of gravitation with μ terms

Moscow State University. Translated from Teoreticheskaya i Matematicheskaya Fizika, Vol. 82, No. 2, pp. 304–312, February, 1990.     

Inequivalence of inertia of rotation and of Kerr-Newman gravitation in the relativistic theory of gravitation

Scientific-Research Institute of Nuclear Physics at the Moscow State University. Translated from Teoreticheskaya i Matematicheskaya Fizika, Vol. 80, No. 3, pp. 474–480, September, 1989.     

Nonstatic solutions of Kazner type in the relativistic theory of gravitation

A nonstatic solution of Kazner type to the system of equations (1)–(2) satisfying all requirements of the relativistic theory of gravitation is constructed.Moscow State University. Translated from Teoreticheskaya i Matematicheskaya Fizika, Vol. 91, No. 1, pp. 173–176, April, 1992.     

Nonsingular configurations of field systems in the relativistic theory of gravitation

Scientific-Research Institute of Nuclear Physics at the Moscow State University. Translated from Teoreticheskaya i Matematicheskaya Fizika, Vol. 88, No. 3, pp. 467–476, September, 1991.