Why the universe is not a black hole (merged)

Click For Summary

Discussion Overview

The discussion revolves around the question of whether the universe can be considered a black hole, particularly in the context of the Big Bang theory and the nature of singularities. Participants explore theoretical implications, the behavior of matter under extreme conditions, and the distinctions between black holes and the early universe.

Discussion Character

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

Main Points Raised

  • Some participants propose that the universe must have been inside a black hole during the Big Bang, questioning how it could expand beyond the original event horizon.
  • Others argue that the Big Bang does not equate to a black hole, citing that the density and conditions at the beginning allowed for rapid expansion, preventing collapse into a black hole.
  • A participant raises the question of why the universe did not form a supermassive black hole given its initial conditions, seeking clarification on the dynamics involved.
  • Concerns are expressed about the applicability of General Relativity (GR) at high densities, with some suggesting that quantum corrections may alter the expected outcomes of singularities.
  • There is a discussion about whether organizing matter to converge could lead to a naked singularity, with references to the cosmic censorship hypothesis suggesting that such singularities may not be possible.
  • Participants share links to external resources and technical papers that discuss the nature of singularities and the limitations of current theories.

Areas of Agreement / Disagreement

Participants express multiple competing views regarding the nature of the universe and its relationship to black holes. The discussion remains unresolved, with no consensus on whether the universe can be classified as a black hole or the implications of singularities.

Contextual Notes

Limitations include the dependence on interpretations of General Relativity and the unresolved nature of quantum corrections at extreme densities. The discussion reflects ongoing debates in theoretical physics regarding the early universe and black hole formation.

Roy Edmundson
Messages
8
Reaction score
0
The Whole Universe Must Be A Black Hole

The Big Bang Theory has the whole universe expanding from an initial size considerably smaller than an atoms nucleus. The universe at this stage must have all been inside a black hole with an event horizon radius of many light -years.

How is it that now the universe is much bigger than the size of the original event horizon - it has effectively escaped from a black hole - or is there still an event horizon out there somewhere at the edge of the universe?
 
Space news on Phys.org
The universe isn't a black hole. See for instance

http://math.ucr.edu/home/baez/physics/Relativity/BlackHoles/universe.html

Included subquestions are:

Why did the universe not collapse and form a black hole at the beginning?

Since I think this is the main question, I'll take the liberty of quoting this section of the FAQ, to motivate people who are interested to read the entire document:

Sometimes people find it hard to understand why the big bang is not a black hole. After all, the density of matter in the first fraction of a second was much higher than that found in any star, and dense matter is supposed to curve space-time strongly. At sufficient density there must be matter contained within a region smaller than the Schwarzschild radius for its mass. Nevertheless, the big bang manages to avoid being trapped inside a black hole of its own making and paradoxically the space near the singularity is actually flat rather than curving tightly. How can this be?

The short answer is that the big bang gets away with it because it is expanding rapidly near the beginning and the rate of expansion is slowing down. Space can be flat while space-time is not. The curvature can come from the temporal parts of the space-time metric which measures the deceleration of the expansion of the universe. So the total curvature of space-time is related to the density of matter but there is a contribution to curvature from the expansion as well as from any curvature of space. The Schwarzschild solution of the gravitational equations is static and demonstrates the limits placed on a static spherical body before it must collapse to a black hole. The Schwarzschild limit does not apply to rapidly expanding matter.

Other questions covered by this FAQ:

What is the distinction between the big bang model and a black hole?

Could the big bang be a black or white hole all the same?
 
If at one point, the entire universe as we know it, was confined to a volume smaller than that of an atom, why did it go "bang"?

With THAT much mass, crunched into so small a volume, why didn't it just form essentially "The Mother of All Super Massive Black Holes", and stay that way?
 
MonstersFromTheId said:
If at one point, the entire universe as we know it, was confined to a volume smaller than that of an atom,..

do you have a link to something I could see that supports that?
I'm curious where that idea comes from. The technical papers I see coming out these days tell a slightly different story.

More like: "We suspect that General Relativity breaks down and fails to apply in situations of very high density pressure, curvature... However if GR DID apply then it would say the observable universe was once confined in a very small volume...etc..."

I'll try to get a link. but have to go, do it when I get back.

================
Monsters, I have an idea for you!

google "kitp spacetime singularities"
that will get you
http://online.kitp.ucsb.edu/online/singular_m07/

these are videos of some of the latest work on curing the bigbang singularity.
It is a gilt-edge elite workshop at one of the US top institutes of theoretical physics
Why not get your money's worth?, because
if you are US taxpayer like me then your money went to NSF to pay for this elite workshop from Jan 8-26 this year
with people from Europe and all over and top US people
the whole thing basically motivated by the fact that the experts do not believe
that GR applies at very high density
they think that at very high density there are QUANTUM CORRECTIONS
(that could even e.g. make gravity a repulsive force at extreme density)
and a lot of experts, which you see here at the workshop, are groping for theoretical framework that will tell them
what the quantum corrections might be and that also could be tested in less extreme situations, and shown up if wrong.

In particular I would suggest looking at Ashtekar and Bojowald's HTML lecture notes, just click on their name on the menu,
and if you like the slides then you can watch the video of them talking from those lecture notes.
http://online.kitp.ucsb.edu/online/singular_m07/ashtekar/
http://online.kitp.ucsb.edu/online/singular_m07/bojowald/

But you can watch Gary Horowitz do his thing (he laughs a bit too much), or Ted Jacobsen, or whoever. It doesn't matter.

One possible answer to your question "why didnt it all collapse to hole?"
is that the whole "singularity" scenario is based on classic 1915 GR and it is widely suspected GR does not apply
and so people are working on various modifications and quantum corrections
where the game is to have a framework that you can TEST with what you can observe, like the CMB and solar system stuff, and galaxy-count structure formation stats, but that also says something about things you can NOT observe.

there are other explanations why it didnt collapse to hole, but I am saying first off to doubt the classical scenario.
===================

Another answer to your question would be to see this excellent post by PERVECT
https://www.physicsforums.com/showpost.php?p=1311838&postcount=2

Here Pervect refers to the FAQ at John Baez website to explain just using basic stuff like Heisenberg uncertainty
and the fact that Schwarzschild BH solution is a static solution. That solution is excellent.
But it doesn't mention the huge ferment going on around quantum corrections to the theory of General Relativity
which is ultimately aimed at getting at what REALLY HAPPENED around the time expansion began. there is some new physics brewing which
I think its good to know about.
 
Last edited:
Thanks Pervect.

I visited the link you quoted and read it all.

Presumably the non-application of the Schwartzchild radius to rapidly expanding matter also applies the other way round?

Suppose we organised 1/2 the matter in the universe to converge on a point in space with no prior black hole, then if the material is approaching fast enough it will reach the centre before a black hole event horizon forms ?
 
Cool! Tx!

As for where I heard that "...at one point, the entire universe as we know it, was confined to a volume smaller than that of an atom,.."

Mostly I've read, almost offhand comments to that effect, in places like NY Times articles, articles on MSNBC.com, etc., where you'll get one line that will say something along those lines, as part of the background to explaining something else.

That point, when made, is rarely, if ever, attributed to a source (which is why I wanted to ask about it in here, reporters often find themselves trying to explain something they don't quite understand themselves in science articles, so -- go fact check with a better source says me).

Anyway, THANKS FOR THOSE LINKS! I'm dyin' to go watch, listen, and read about this.
 
I've merged this thread with a very similar thread on the same question
 
Roy Edmundson said:
Thanks Pervect.


Suppose we organised 1/2 the matter in the universe to converge on a point in space with no prior black hole, then if the material is approaching fast enough it will reach the centre before a black hole event horizon forms ?
Not knowing a great deal i was wondering if that is what they would call a naked singularity.

Are naked singularities possible.
 
Last edited:
ukmicky said:
Not knowing a great deal i was wondering if that is what they would call a naked singularity.

Are naked singularities possible.

The cosmic censorship hypothesis suggests that naked singularities are not possible, but I don't think this has been proven.

Naked singularities are singularities without an event horizon, and aren't related to the original question. One way that naked singuarities could arise is by a black hole spinning above a certain critical rate. It can be shown that a black hole cannot be "spun up" from an ordinary black hole into a naked singularity, but as far as I know the question of whether naked singularities can form out of collapsing matter is somewhat open (the cosmic censorship hypothesis is still a hypothesis).

I can't really answer Roy's original question cited by umicky above, unfortunately. It's a bit too detailed, and would involve many finicky details to answer, such as:

Do we use the absolute horizon or apparent horizon? How do you definie simultaneity between the event in the center and the horizon, (simultaneity is relative)? What's the exact distribution of matter?
 

Similar threads

  • · Replies 7 ·
Replies
7
Views
4K
  • · Replies 14 ·
Replies
14
Views
4K
  • · Replies 29 ·
Replies
29
Views
3K
  • · Replies 12 ·
Replies
12
Views
3K
  • · Replies 24 ·
Replies
24
Views
3K
  • · Replies 36 ·
2
Replies
36
Views
7K
  • · Replies 25 ·
Replies
25
Views
4K
  • · Replies 9 ·
Replies
9
Views
3K
  • · Replies 4 ·
Replies
4
Views
2K
  • · Replies 15 ·
Replies
15
Views
3K