Authors: Vladimir Leonov
In , 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.
Comments: 4 Pages, 2 Figures
[v1] 2019-11-01 07:31:17
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