Astrophysics

   

Preference for Dual Herbig Haro Black Hole Consumption by the Central MW Black Hole, Leaving Plasma Jets Behind.

Authors: Leo Vuyk

Recent observations by the new MeerKat telescope system show unprecedented details of Herbig Haro jet alike objects around the central black hole of our Milky Way. According to the Quantum FFF Model, Herbig Haro jets are connected between the central baby star and both Stellar Anchor Black Holes ( SABHs) , which are responsible for the spacetime polarization forming a kind of vacuum/ ether pressure cooker, for fast star formation in between the two SABHs. It is well known, that all black holes are the same as electric charged dark matter, able to attract each other up to a certain distance and forming a plasma bar in between, which evaluate later into dual plasma jets, keeping the two black holes at a certain mass related distance. However only black holes of the same gravitational potential ( nuclear quantum knot size) are able to perform such a process, leading to so called Herbig Haro systems. If different sized black holes approach each other, it is assumed that the smallest black hole is able to split the larger one into two equal sized quantum knots, which will form a stable Herbig Haro system with star or even failed star formation in between. Also well known is, that the smallest black holes in galaxies seem to have a preference for group around the central galaxy position, which mostly is equipped with a central black hole. The central black hole is supposed to be the gate to the end of the galaxy and even the universe itself into a big crunch black hole as a start for a new cyclic multiverse.. As a consequence, the central black hole seem to feed mostly on the smaller dual Herbig Haro black holes, which is probably the origin of the numerous remaining former plasma jets which are found in the MeerKat ( precursor releases) observations.

Comments: 25 Pages.

Download: PDF

Submission history

[v1] 2018-07-25 08:33:21

Unique-IP document downloads: 7 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