How long does it take a black hole to gain seven billion solar masses?

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Discussion Overview

The discussion centers around the time it takes for a black hole to accumulate mass, specifically addressing the scenario of a black hole gaining seven billion solar masses. Participants explore theoretical aspects, observational evidence, and the implications of black hole formation in the context of the universe's age and material availability.

Discussion Character

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

Main Points Raised

  • Some participants suggest that black holes accumulate matter over long periods, with significant mass gain occurring only under certain conditions, such as starting with a massive star.
  • Others argue that the formation of supermassive black holes may have occurred rapidly in the early universe, potentially from primordial gas clouds rather than from stellar evolution.
  • There is a discussion about the probability of forming stellar black holes, with some participants noting that while massive stars are rare, they are still capable of forming black holes through supernova events.
  • Questions are raised regarding the mass thresholds for black hole formation and whether all black holes must originate from stars of a certain mass.
  • Some participants inquire about the effects of time dilation on the mass accumulation of black holes, particularly in relation to accretion processes and the perception of time by distant observers.
  • Concerns are expressed about the availability of material for black holes to accrete, suggesting that location within a galaxy may influence mass gain rates.
  • Participants note the mystery surrounding the existence of quasars and supermassive black holes in the early universe, highlighting the challenges in explaining their rapid formation.

Areas of Agreement / Disagreement

Participants express a range of views on the mechanisms and timelines for black hole mass accumulation, with no consensus reached on the specifics of formation processes or the implications of time dilation. The discussion remains unresolved regarding the exact conditions necessary for black hole growth and the probabilities associated with different mass ranges.

Contextual Notes

Limitations include uncertainties about the initial conditions for black hole formation, the dependence on definitions of mass thresholds, and unresolved questions regarding the mechanisms of accretion and time dilation effects.

poeteye
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We don't see matter rushing to a center point as though down a drain anywhere in the universe. Black holes' accumulation of matter must (except perhaps rare moments like a collision with another black hole) happen over a long period of time. Assuming a star, destined to be a black hole, began at a reasonable mass, say seven times our sun, how long would it take it to reach the billion times that mass at which black holes have been estimated today?
 
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poeteye said:
We don't see matter rushing to a center point as though down a drain anywhere in the universe.
You're right we don't ever see that per se, but we do see the effects of that in quasars, high-mass x-ray binaries, etc. Numerous cases are fairly conclusive that 'lots of matter down the drain' is what's happening.

poeteye said:
Black holes' accumulation of matter must (except perhaps rare moments like a collision with another black hole) happen over a long period of time.
Very true.

poeteye said:
Assuming a star, destined to be a black hole, began at a reasonable mass, say seven times our sun, how long would it take it to reach the billion times that mass at which black holes have been estimated today?
That would take far longer than the age of the universe. But if you were able to start with a star a few hundred times the mass of our sun (difficult to do that, and uncertain if its possible) it would take just about the age of the universe (and therefore would be possible).

This is an active question in research. One of the weird things is that we see quasars (super-massive black-holes) very early in the universe... which means they formed somehow, and very rapidly.
 
So am I right to say that most stellar Black holes have low probability at the current age of the universe ? sorry to hijack this thread.
 
ibysaiyan said:
So am I right to say that most stellar Black holes have low probability at the current age of the universe ?
Low probability of what?
 
Stellar mass black holes are not deemed particularly improbable. Hugely massive stars are relatively rare, but still exist in large numbers. These goliaths burn up their fuel and go supernova in millions, as opposed to billions of years for average mass stars such as the sun. And only massive stars are capable of going supernova. Conventional wisdom is stars in excess of about 8 solar masses are doomed to become stellar mass black holes. This, however, is not always the case. For example, a paper in 2005 reported a neutron star with a progenitor mass >40 solar masses [see arXiv:astro-ph/0509408v3]. Obviously, the star found a way to shed nearly all its mass before settling down as an unassuming, ordinary sized neutron star. This is, perhaps, the result of an asymmetric explosion, or processes during the supernova phase not yet understood. Perhaps, stellar mass black holes do not even arise from supernova. They may be the result of other processes, such as neutron star mergers in binary systems.
As far as supermassive black holes go, there is at least some evidence they may have skipped the whole star thing and formed directly from primordial gas clouds in the early universe. See, for example, http://www.universetoday.com/11734/never-a-star-did-supermassive-black-holes-form-directly/
 
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So you are saying that in order for the super massive black holes we see today to have accumulated the mass they have, they must have started out big? And why eight times bigger than the resultant black hole? Would you say all initially formed black holes had to have had original solar masses eight times as large?

if a single star originally formed a black hole it was likely nowhere near a billion solar masses but only a few hundred solar masses. The earliest it could have formed would be after the formation of stars began, so let's say the to gain the amount of weight we see today must have taken it less than 14 billion years, to gain 18 billion solar masses, so it was eating more than a sun a year?
 
Some good questions being asked here. Is there enough time since the Universe began to create Black holes as massive as 4 Million solar masses eg Sagittarius A* or the largest known black hole of 18 Billion solar masses?
 
Wouldn't this depend on the availability of material to suck up into the black hole? IE a black hole near the galaxy center would probably accumulate mass much quicker than one at the outer edge or in a much less dense area.
 
Many of the supermassive holes responsible for quasars are billions of light years from us, hence formed billions of years ago. At least some of them apparently formed in the first billion or so years after the big bang. Explaining how they came to be so massive in such a short time is a mystery. The universe was more crowded back then, but, it still is difficult to explain such massive bodies at such early times. How ever it happened, it happened in a hurry.

The 8 solar mass thing is the lower mass threshold for a star undergo core collapse. It is generally believed core collapse events are the most likely route to stellar mass black holes. But, the whole thing is rather complicated and involves a fair amount of guess work.

While I tend to shy from citing Wiki as a source, they have a pretty good write up here:
http://en.wikipedia.org/wiki/Stellar_evolution
I have fewer reservations about Astronomy Online, which also has nice article on the subject: http://astronomyonline.org/stars/blackhole.asp
 
  • #10
Anyone have any idea of whether or not there is even the remotest of possibilities (well okay, remotest within SOME reason, ie. not me quantum tunneling through a wall after one try) that super-massive black holes were originally primordial black holes during the pre-inflation era, and with inflation expanded to garguantuan size? It is especially puzzling to me, like Chronos said that quasers existed when they did. Not only that, the fact that they ONLY existed then.

I may sound like an utter moron, if so excuse me I've not heard anything about this or anything but just pondered it as something interesting to think about.
 
  • #11
Does anyone know if time dilation would slow the rate at which a BH can increase in mass, at least through known mechanisms like accretion or collision? This was one of the reasons I posted the question "time (seen by distant observer) for matter to fall to the event horizon of black hole". Or, am I thinking about this incorrectly?
 
  • #12
Jonathan, that's my point exactly. We see things enter a black hole very, very slowly due to time dilation. Also, black holes undergo tremendously long rests where they are not feeding at all -- even the ones from the first billion years of the universe behave this way, even though matter was denser then.
And will everyone please look up at Tanalorn's concise re-phrasing of the question?
 

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