Formation of Naked Singularities

In summary: The event horizon is a property of the spacetime ... so if there's no event horizon, there's no black hole.In summary, the theoretical formation of naked singularities involves a rotating black hole with a high enough angular momentum that the event horizons merge and disappear, revealing the singularity. This singularity has a curvature that diverges to infinity and any lines going to it will end there. However, without an event horizon, the singularity is not considered a black hole.
  • #1
Itai Blank
8
0
Hi!
I've been trying to find explanations about the theoretical formation of naked singularities,
and all I could come up with was Wikipedia, and frankly, the explanation didn't "set" in my mind, I couldn't really visualize it. It reads:

"From concepts drawn of rotating black holes, it is shown that a singularity, spinning rapidly, can become a ring-shaped object. This results in two event horizons, as well as an ergosphere, which draw closer together as the spin of the singularity increases. When the outer and inner event horizons merge, they shrink toward the rotating singularity and eventually expose it to the rest of the universe."

When they say the two event horizons merge, that's the part that I can't get right, I mean, why do they shrink towards the center? why do they draw closer? Is it because of the geometric transformations to the singularity? Why two, actually? wouldn't one conceal it from the entire universe? I seriously need clarification on this...

-Itai
 
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  • #2
Welcome to PF!

Itai Blank said:
When they say the two event horizons merge, that's the part that I can't get right, I mean, why do they shrink towards the center?

Hi Itai! Welcome to PF! :smile:

They don't shrink towards the centre, they shrink towards each other, at r = M.
… why do they draw closer? … Why two, actually? wouldn't one conceal it from the entire universe? I seriously need clarification on this...

They draw closer because that's what the maths says.

The signature of ordinary space is +--- but the signature changes when you go through an event horizon.

The Kerr solution (rotating black hole) has one signature change (angular momentum = 0), two signature changes (0 < angular momentum < M), or none (angular momentum ≥ M).

To be more specific: for a rotating black hole with mass M and angular momentum aM, the coefficient of dr2 in the metric has a factor 1/(r2 - 2Mr + a2), and therefore changes sign at r = M ± √(M2 - a2), and these sign changes are at r = 2M (and 0) for a = 0, they converge as a increases, eventually disappearing when they merge at r = M for a = 1. :wink:
… Is it because of the geometric transformations to the singularity? …

I don't know what you mean by "geometric transformations to the singularity" :redface:

The singularity is always at r = 0, nowhere near where the event horizons merge at r = M.

It is geometrically a point when a = 0, and a ring when a > 0, but it's always at r = 0. This apparent contradiction (a ring of zero radius) is because r isn't actually a very sensible coordinate. :rolleyes:
 
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  • #3
Ok, thanks.
But still, why do two event horizons form in the first place? I mean, how does the fact that the black hole is shaped as a ring make that happen?
tiny-tim said:
They don't shrink towards the centre, they shrink towards each other, at r = M.
It says there "...they shrink toward the rotating singularity, eventually exposing it to the rest of the universe"
Is that just incorrect?
 
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  • #4
Itai Blank said:
But still, why do two event horizons form in the first place? I mean, how does the fact that the black hole is shaped as a ring make that happen?

It doesn't.

The event horizons and the ring singularity don't cause each other, they are both caused by the metric.

(and one event horizon, with a non-ring singularity, virtually never happens … it would require the black hole to have exactly zero angular momentum, which is virtually impossible)
 
  • #5
Oh, ok, thanks, clearly I have to learn a bit more about this whole thing.
I guess the explanation in Wikipedia wasn't quite accurate, because it differed from what you've told me.

Thanks anyway :)
 
  • #6
I just thought of another issue.. If there is no event horizon, It means an object can escape he singularity, right? So if the escape velocity is now less than the speed of light, by what definition is the singularity a singularity?
 
  • #7
I just thought of another issue.. If there is no event horizon, It means an object, or say, a photon, can escape the singularity, right ? So if the escape velocity is now less than the speed of light, by what definition is the singularity a singularity?

I thought it may mean that the event horizons are still there, only below the surface of the formerly-black hole... But that would make the singularity not really naked, would it? Although, the effects in the immediate area of the singularity could be observed...
Am I making ANY sense at all?
 
  • #8
Itai Blank said:
I just thought of another issue.. If there is no event horizon, It means an object can escape he singularity, right? So if the escape velocity is now less than the speed of light, by what definition is the singularity a singularity?

Its a singularity because the cuvature diverges to infinity.

Naked singularities are non-physical in general. In terms of the solution for a rotating black hole i think the naked siguarity wound repel matter that fell towards it because it has such a high angular momentum. But by the same logic such a singularity couldn't form from a gravitational collapse because the angular momentum would prevent it.
 
  • #9
Itai Blank said:
I just thought of another issue.. If there is no event horizon, It means an object, or say, a photon, can escape the singularity, right ? So if the escape velocity is now less than the speed of light, by what definition is the singularity a singularity?

There's no such thing as escape velocity (for a black hole) … a black hole isn't like a waterfall (and light isn't like fish!).

The definition of a black hole singularity is that any line going to the singularity ends there.

Lines not going to the singularity (however close they may get) don't have to end.
I thought it may mean that the event horizons are still there, only below the surface of the formerly-black hole... But that would make the singularity not really naked, would it? Although, the effects in the immediate area of the singularity could be observed...
Am I making ANY sense at all?

Nope. :redface: Sorry! :smile:
 
  • #10
If it's not too much trouble, could you try to explain the whole process of the creation of a naked singularity? Maybe a complete explanation will do better than asking about specific parts..
 
  • #11
(in post #2 above, I left out a "squared", and it should read "two signature changes (0 < angular momentum < M2), or none (angular momentum ≥ M2)" :redface:)
Itai Blank said:
If it's not too much trouble, could you try to explain the whole process of the creation of a naked singularity? Maybe a complete explanation will do better than asking about specific parts..

It's very simple …

a naked singularity is created the same way as an ordinary one …

the only difference is that if the angular momentum J is greater than the mass squared (M2), then the event horizons (which would be at r = M(1 ± √(1 - (J/M2)2)) cannot exist. :smile:
 
  • #12
Ok thanks.. that just about does it for now...
I'll understand it better in a few years after receiving
formal university education :D...

Just one last thing though...
The curvature of spacetime, is, essentially what we call gravity.
So if the curvature goes to infinity at the singularity, It's still not clear to me
how light can be emitted from it...
Does the fast rate of rotation change the curvature around it?

If the answer is no, please do try to give the actual reason, and please bare with me,
It's not like I've studied this for years, I've only recently become aware of this theoretical phenomenon.
 
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Related to Formation of Naked Singularities

1. What is a naked singularity?

A naked singularity is a hypothetical point in space where the gravitational pull is infinite, and the laws of physics break down. Unlike a black hole, a naked singularity does not have an event horizon, which means that it can be observed from the outside.

2. How are naked singularities formed?

Naked singularities are formed when massive stars collapse under their own gravity. As the star's core collapses, it reaches a point where the gravitational pull becomes infinitely strong, and the matter is compressed into a single point of infinite density.

3. Can naked singularities be observed?

Currently, there is no evidence of the existence of naked singularities, and they are only theoretical objects. However, some theories suggest that they could be observed indirectly through their effects on surrounding matter.

4. What are the implications of naked singularities?

If naked singularities do exist, they could have significant implications for our understanding of the universe. They could challenge the laws of physics and the concept of determinism, as they represent a breakdown of our understanding of how the universe works.

5. Is it possible to prevent the formation of naked singularities?

Currently, there is no known way to prevent the formation of naked singularities. However, studying them and understanding their properties could lead to advancements in our understanding of gravity and the behavior of matter under extreme conditions.

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