Early Universe massive Black Holes question

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Discussion Overview

The discussion revolves around the formation of massive black holes in the early Universe, particularly focusing on the conditions that may have allowed for their existence and growth. Participants explore theoretical frameworks, the role of dark matter and dark energy, and the mechanisms behind the formation of supermassive black holes.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • One participant questions whether the density of dark matter or dark energy could have been sufficient to form massive black holes in the early Universe.
  • Another participant clarifies that dark energy's effects were negligible during the early Universe, becoming significant only billions of years later.
  • Some participants mention that current theories allow for the existence of primordial black holes.
  • There is discussion about the unclear mechanisms behind the formation of supermassive black holes, with one participant noting that the effective density can be very low.
  • Another viewpoint suggests that earlier supermassive black holes could have been primordial or that ordinary black holes might grow at faster rates than previously thought.
  • Participants note correlations between the size of supermassive black holes and their host galaxies, indicating a potential common evolutionary factor.
  • Links to recent research and articles are shared to provide additional context and data on the topic.

Areas of Agreement / Disagreement

Participants express differing views on the role of dark energy and the mechanisms of black hole formation, indicating that multiple competing theories and uncertainties remain in the discussion.

Contextual Notes

There are unresolved questions regarding the definitions and proportions of matter types involved in black hole formation, as well as the specific conditions in the early Universe that may have influenced their growth.

ShadowKraz
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I've spent the past few days trying to find an answer to a question I have about the formation of massive black holes in the early Universe. It is possible that my search parameters were poorly formulated.
As I understand the issue, according to our current theories, massive black holes 'should not' have formed as early as we are detecting them. Obviously they did form otherwise the issue would not arise.
Is it possible that the density of dark matter, dark energy, or both was sufficient at some point during the early Universe to form these black holes? Or is my understanding that flawed?
 
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How massive is massive? A ton? A moon? A galaxy?
 
Vanadium 50 said:
How massive is massive? A ton? A moon? A galaxy?
Oops, my bad, I meant to type 'supermassive black holes', as found in the cores of most of the galaxies we have observed.
 
Mordred said:
Our theories do allow for primordial BHs
https://arxiv.org/abs/2211.05767
My apologies, please see comment #4. I'll read the linked paper tonight; it looks very interesting, thank you.
 
ShadowKraz said:
Is it possible that the density of dark matter, dark energy, or both was sufficient at some point during the early Universe to form these black holes?
Why would you think that dark energy has anything to do with black holes in the early universe? The effects of dark energy at that time were negligible. Only after billions of years did it start to have any significant effect, most notably after about 7 or 8 billion years when it became a more dominant force than gravity for unbound systems.
 
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The mechanism of formation of supermassive black holes is not understood. The effective density of such objects (ignoring the issues with even defining that) can be as low as that of air. So while the description "too much mass got into too small a space" sounds tautological, that's not a bad description.

The too much matter could be gas, stars, black holes, or dark matter in some proportion. I do not believe there is consensus about what that proportion is.
 
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I think we don't know whether these earlier supermassive black holes were primordial black holes that grew, or whether "ordinary" black holes could grow at much faster rates than we think. The mean density of the universe was 1000's of times greater than today, so maybe there were mechanisms that would allow them to grow rapidly. Or maybe they were very large early stars that transitioned to black holes through direct collapse. It's ongoing research.
 
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There are correlations between the size and properties of a galaxy's SMBH and its galactic bulge. That suggests there is some common factor in the evolution of both structures.
 
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  • #10
phinds said:
Why would you think that dark energy has anything to do with black holes in the early universe? The effects of dark energy at that time were negligible.
Because I hadn't found any information on that. Now I know, thank you.
 
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  • #11
More data on early galaxies and black holes from JWST. Here seems as good as place as any to put it.

https://iopscience.iop.org/article/10.3847/2041-8213/ad55f7

"At face value, this implies that these black holes are over massive relative to their stellar components and that the stellar components must continue to grow over the next 13 Gyr in order to produce the relationship observed today."

There is a "however" in there but I will let you read it.

An article for us laymen

https://phys.org/news/2024-06-tiny-bright-dawn-universe-baffle.html
 
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