Quantum Physics


Gravitational Diagram of a Non-Ideal Black Hole

Authors: Vladimir Leonov

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.

Comments: 4 Pages, 2 Figures

Download: PDF

Submission history

[v1] 2019-11-01 07:31:17

Unique-IP document downloads: 9 times

Vixra.org is a pre-print repository rather than a journal. Articles hosted may not yet have been verified by peer-review and should be treated as preliminary. In particular, anything that appears to include financial or legal advice or proposed medical treatments should be treated with due caution. Vixra.org will not be responsible for any consequences of actions that result from any form of use of any documents on this website.

Add your own feedback and questions here:
You are equally welcome to be positive or negative about any paper but please be polite. If you are being critical you must mention at least one specific error, otherwise your comment will be deleted as unhelpful.

comments powered by Disqus