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Which came first: black holes or stars?


"This set of illustrations explains how a large black hole can form from the direct collapse of a massive cloud of gas within a couple of hundred million years after the Big Bang. Cold streams of gas can lead to the direct collapse of a "seed" black hole of several tens of thousands (at least) of solar masses, which can form even prior to any stars forming in the surrounding young galaxy. As the galaxy and black hole grow, eventually the stellar mass content will outweigh the more slowly-growing black hole. This is strongly favored, observationally, over the primordial black hole scenario." (BigThink, Ask Ethan: Did black holes form directly from the Big Bang?)

In theoretical models, there were so-called primordial black holes in the universe's dark ages. Those primordial black holes formed the quantum dots in energy flow. After that, the Schwinger effect, or wave-particle duality, formed the first particles from crossing whirls in the radiation field. Those primordial black holes were so-called  "Kugelblitz" black holes. So, primordial black holes formed straight from energy or wave movement. 



Dark energy can form Kugelblitz black holes. 


The term "Kugelblitz" (or "Kugelblitz black hole")  means a theoretical black hole, that formed straight from the wave movement. Theoretically, all wave movement including dark energy and gravity waves can form the Kugelblitz. 

The idea of the "Kugelblitz" black holes is that all wave movement can form Kugelblitz. And if we follow this route, the dark energy can also form Kugelblitz black holes. When we think about the black hole formation, the black hole can form around almost every object. The requirement is that the environment around the object is stable enough, that it can pull enough material around it. The requirement is that the object is so massive. 

That it can eliminate the outcoming radiation effect. Outside the galaxy clusters, the environment is very static. In that static environment, the object can collect material around it, and if the fusion reactions do not begin the mass can transform into a black hole, if the starwind or some other cosmic phenomenon will not blow the material away. Same way if the interplanetary nebula collapses too fast, or some massive stars collide, that can form a situation, where the object turns into a black hole. 



Quasi-stars (or black hole stars): the enormous theoretical energy sources from the early universe. The intermediate-mass black holes could be remnants of the quasi-stars. And the researchers confirmed that the Omega Centauri hosts an intermediate-class black hole. And that proved those black hole-types existence. 

The reason why the intermediate class black holes are interesting is, that they can tell how large stars can be. The supermassive black holes can form when the interplanetary or interstellar nebula collapses. The intermediate black holes can form when the blue "O" or "B" type massive stars collide with some other massive stars. Or the collision can happen between two stellar class black holes or neutron stars. 

In some interesting models, the neutron star falls into the star. A neutron star will pull the star against it. And that energy can press it into the black hole. If the star's shell orbits the black hole at a very high speed it can form a so-called quasi-star.

Quasi-star is the star that gets its energy from black holes. It's possible, that qausistars existed in a young universe.  And Omega Centauri's intermediate-mass black hole supports that theory. 




"A spiraling wind helps the supermassive black hole in galaxy ESO320-G030 to grow, assisted by magnetic fields. In this illustration, the core of the galaxy is dominated by a rotating wind of dense gas leading outwards from the (hidden) supermassive black hole at the galaxy’s very center. The motions of the gas, traced by light from molecules of hydrogen cyanide have been measured with the ALMA telescope. Credit: M.D. Gorski/Aaron Geller/Northwestern University/CIERA." (ScitechDaily, Magnetic Winds Drive Supermassive Black Hole Growth in Nearby Galaxy)


The magnetic fields and material feed black holes. 


The black hole is in its gravitational pothole. The pothole is very deep. And that's why black holes are not moving quite easily. The thing that makes objects move is the asymmetry in the pothole around particles. The asymmetry causes the energy pothole to start to travel through the universe, and the particle follows the pothole. 

A black hole grows if it gets more energy than it releases. The magnetic fields and magnetic winds pump energy into the material disk and black hole's halo. That process makes the black hole grow. Black holes pull material and wave movement inside them. And when that wave movement travels through that material and transition disk it increases its energy level. A black hole grows as long as its halo and material disk pumps energy into it. When the energy level in the material disk and halo turns lower than in the black hole, the black hole turns smaller. 

This thing is one of the reasons, why the black hole is so special and why it looks like what it looks. The energy asymmetry in the structures around black holes press the black hole, like a hand, that presses a balloon there is a little bit of water. If the hand presses the balloon in the middle of it, that means water travels to both sides of the hand. That means the fields inside the event horizon look like the dumbbell. That structure is one of the reasons why black holes send so-called relativistic jets. 


https://bigthink.com/starts-with-a-bang/black-holes-direct-big-bang/


.https://scitechdaily.com/magnetic-winds-drive-supermassive-black-hole-growth-in-nearby-galaxy/


.https://scitechdaily.com/omega-centauri-a-galaxy-core-frozen-in-time-reveals-its-black-hole/


https://en.wikipedia.org/wiki/Kugelblitz_(astrophysics)


https://en.wikipedia.org/wiki/Stellar_classification

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