On the Schwarzschild model for gravitating objects of the Universe
Д. Н. Дойков, Volodymyr Kiosak
Abstract
The paper treats Schwarzschild spaces as a model for gravity features. We study a wrapped product of metrics of Schwarzschild spaces. The paper demonstrates that there are two substantial components and coeffcients can be calculated basing on the physical considerations. We treated a phenomenon of gravitational distortion of beams, moving from periphery of the Universe to the terrestrial observer. The centers of active galactic nuclei (AGN) were selected as point sources of such quanta. The galaxies were selected as distant as possible due to the limitations on the registered distance. We defined the spatial properties of the quanta trajectories depending on the distribution of galaxies along the way of the beam.