viXra:1911.0006 submitted on 2019-11-01.
Abstract.
In [1], we
examined the parameters and properties of an ideal black hole. The ideal
black holes characterized discontinuities of the
quantized space-time on the surface of the black hole. Its
formation is completed. Such a black hole is completely invisible. Non-ideal black
holes do not have discontinuities of quantized space-time on the surface of a
black hole. Its formation is not completed. Such a black hole has a visible
glow due to the reflection of photons from its surface. We describe the state
of a black hole by a system of equations in the form of a two-component
solution of the Poisson equation for the quantum density of the medium and
gravitational potentials. An analysis of the spherical deformation of quantized
space-time allows us to look inside a black hole and describe its external
gravitational field.
Keywords: black hole, ideal black holes, non-ideal black
holes, quantum density, gravitational compression, deformation vector,
gravitational forces.
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