Can a primitive galaxy nova or supernova?

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Discussion Overview

The discussion explores the possibility of a primitive galaxy undergoing nova or supernova events, and the implications of such processes for star production and quasar formation. Participants examine the mechanisms behind these phenomena and their relevance to the early universe, particularly in relation to supermassive black hole formation.

Discussion Character

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

Main Points Raised

  • Some participants question whether the processes driving nova or supernova events can be present throughout an entire galaxy.
  • One participant suggests that if a significant mass of a galaxy collapses, it could lead directly to a black hole without intermediate stages like star formation.
  • Another participant argues that the collapse of a galaxy's mass would occur slowly and non-uniformly, potentially resulting in the formation of stellar-mass black holes rather than a direct collapse into a supermassive black hole.
  • Concerns are raised regarding the formation of supermassive black holes in the early universe, particularly in relation to the Eddington limit, which restricts the growth rate of black holes due to photon pressure.
  • Participants discuss the concept of "fragmentation" in the context of early universe star formation and its implications for understanding black hole formation.

Areas of Agreement / Disagreement

Participants express differing views on the mechanisms of galaxy collapse and black hole formation, indicating that multiple competing perspectives remain without consensus on the processes involved.

Contextual Notes

Limitations include the lack of a clear description of how fragmentation proceeds in the early universe and the unresolved nature of the mechanisms that could allow supermassive black holes to form rapidly after the big bang.

Who May Find This Useful

This discussion may be of interest to those studying astrophysics, particularly in the areas of galaxy formation, black hole physics, and the early universe.

Loren Booda
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Can a primitive galaxy nova or supernova? Might the former process be involved with star production or the latter with a quasar?
 
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Can that which drives a nova or supernova be present thoughtout a galaxy?
 
Huh? A whole galaxy? Its not even March, much less April 1.
 
Perhaps, if a significant mass of a galaxy collapses, it does so all they way to a black hole (quasar?) without any obvious stages like a star. However would we describe the formation of our Galaxy's supermassive black hole in terms of its effect on the outlying galactic nucleus?
 
Loren Booda said:
Perhaps, if a significant mass of a galaxy collapses, it does so all they way to a black hole (quasar?) without any obvious stages like a star.

This doesn't happen.

Collapse of any appreciable portion of a galaxy's mass would proceed so slowly and non-uniformly as to either not directly collapse into a black hole or simply create one (or even several) stellar-mass black hole with accreting matter.

You cannot create a stellar object above ~150 solar masses anyways, because the increase in temperature as the cloud collapses causes it to expand again. As far as I know, collapse of masses larger than this must proceed via fragmentation rather than a unified collapse.
 
Nabeshin,

"Fragmentation" suggests what I had been looking for. How does this proceed in the early universe?
 
A good read might be
Might we eventually understand the origin of the dark matter velocity anisotropy?
http://arxiv.org/abs/0812.1048
Im not suggesting this is particularly mainstream, but might be along the lines you are thinking.
 
Loren Booda said:
Nabeshin,

"Fragmentation" suggests what I had been looking for. How does this proceed in the early universe?

I'm not sure if there's a very good description of how this proceeds, especially in the early universe. I don't exactly keep up with published papers, and know of no good explanation off the top of my head.
 
This touches on an important issue:

how do supermassive black holes (SMBH) form so quickly in the early universe?

We've detected quasars, whose energy output suggests that they are powered by SMBHs with a mass of [itex]10^9 M_{sun}[/itex], and that show redshifts greater than 6. This implies that a SMBH must have formed less than a billion years after the big bang. Why is this a problem? Accretion onto SMBHs is limited. If the accretion disk around a SMBH produces too much light then the photon pressure will overwhelm gravity and push the accreting matter away--thus the Eddington limit is born. Thus you can guess how fast the SMBH can grow and, sure enough, they can't grow fast enough to reach [itex]10^9 M_{sun}[/itex] in a billion years.

This why workers are seeking ways to circumvent the Eddington limit either by the collapse of mini dark matter halos (similar to what your saying) much more massive than a solar mass or other means.
 

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