Early Black Hole can act as Koasar seeds

Recently, many groups about the early Black Hole (PBHS) have been making ideas. Part of it is due to their candidates as a potential source of dark matter. But, if they were present, they had other characters to play in the early universe. According to a recent draft paper issued on Archeo Pre -print server can be as one of the characters of Jeremy Mold and Adam Baton of Sonburn University, which eventually forms both Kosar and Radio Galaxy.

In the first few thousand years, the PBHS began very soon in the universe. Instead of being created by the collapse of a large star, most of the modern black holes that we think about are created by minor contradictions in the radiation environment that currently form the entire universe. In the backdrop of the universe microwave, we see the contradictions as a small fluctuation in the signal that is still reaching the ground, though no one has tied these contradictions to the formation of PBHS so far.

But if the PBHS was initially present, his gravity could serve as a “seed” to achieve more gas and dust, which could allow him to grow in the most mask black holes in the center of the brightest famous objects in the universe. Over time, their lights are different, and the person who describes this change is an important piece of mathematics (QLF), an important piece of mathematics that shows how to produce Kaasar and how to affect the formation of galaxies around him.

The important thing is, the mathematics behind the QLF, which is described by the observations of itself, is clean with the predictions presented by this theory, which shows that PBHS acts like a badge that is produced in Koasar. It also fits a mathematical formula called the Shechatter Function, giving more reputation to the theory. But the important thing is that it also offers a solution in which Koasar is fuel in the first place.

Small galaxies can be fuel that brightens Koasar when they swallow them, even though they will be hidden to us at such a distance. Since the super mask black hole in the middle of the Koasar eats all galaxies nearby, it slowly begins to lose its light, tracking the QLF curves, which shows that it is likely to be less bright (ie, high red shift).

Another interesting result of the theory presented in the paper is a tie between the toss and radio galaxies, a type of galaxy that has a strong burst in the radio spectrum. If the theory of being “seed” through ancient black holes is correct, then they can eventually result in a radio galaxy when they are calm and eat all the matter near them.

To prove this point, the authors noted that there are similarities between the lighting functions of the radio and radio galaxies along with the overall dimensions of the radio galaxies. Since they are reduced, although they also go too long, the expected life of a radio galaxy is 10 times higher than a kosar.

Although this theory we have so far aligned well with most of the observational data collected on kosos and radio galaxies, it also offers some predictions to prove ourselves wrong. First of all, this shows that Koasar can be used as standard candles to measure cosmological distances, a title that is currently with Type IA Supernova due to his standard brightness. The origin of Koasar from PBHS can prove a baseline from which to understand their brightness. Eventually, allows them to be used as a standard candle.

Perhaps more wrong, the James Webpace telescope will be able to find information about Kaasar more than ever before. If the new data is in accordance with the predictions made by theory, then, according to the ideologies version of the scientific procedure, it will also lead to success in other scientists.

The web may release any data that can prove the theory or prove it wrong, but it is always good to have a universe with a clear prediction in the universe. As a result, cosmologists have achieved another way to measure the distance and get better understanding of the galaxy formation in the early universe, it will be just an extra bonus.