Black hole singularity, a time-like surface?

  • #1
Hill
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In "General Relativity: The Theoretical Minimum" (Susskind, Leonard; Cabannes, André), the surface corresponding to the black hole singularity is described as time-like. Why?
Below is the description from the book. I thought that hyperbolas in the right quadrant are time-like and hyperbolas in the upper quadrant are space-like. If it were so, the surface ##r=0## would be space-like, but the book says otherwise. -- ?
1703127344928.png
 
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  • #2
Hill said:
Below is the description from the book. I thought that hyperbolas in the right quadrant are time-like and hyperbolas in the upper quadrant are space-like.
You are correct. The singularity in a Schwarzschild black hole, which is what the diagram is showing, is spacelike. That is a huge error, which I am extremely surprised to see in that book.
 
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  • #3
PeterDonis said:
The singularity in a Schwarzschild black hole, which is what the diagram is showing, is spacelike.
I guess Susskind needs to read Wald, section 6.4, which explicitly states what I state in the quote above.
 
  • #4
On a Kruskal diagram, like on a Minkowski diagram, null lines slope at 45° and timelike lines are steeper than that.

The body text correctly notes that the singularity is more like a time than a place, though, meaning it is spacelike (any "now" must be a spacelike surface - or line in the case of the Schwarzschild singularity). So the caption is a typo that's got past the authors and editors.
 
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  • #5
Ibix said:
the caption is a typo
At least two of them, since "time-like" appears in both the Figure label and the paragraph of text beneath it.
 
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  • #6
Ibix said:
On a Kruskal diagram, like on a Minkowski diagram, null lines slope at 45° and timelike lines are steeper than that.

The body text correctly notes that the singularity is more like a time than a place, though, meaning it is spacelike (any "now" must be a spacelike surface - or line in the case of the Schwarzschild singularity). So the caption is a typo that's got past the authors and editors.
In other words, the hypersurfaces ##r=\text{const}## with ##r<r_{\text{S}}## are spacelike since the corresponding ##r##-lines are "normal vectors" of this hypersurface are time-like. It's often confusing, but one has to remember that a hypersurface is spacelike if the normalvector is timelike and vice versa. So I'd also say the singularity ##r=0## is a spacelike hypersurface rather than calling it time-like.
 
  • #7
May be they meant to say that it is like a moment of time. Many places at the same time.
 
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  • #8
But that's indeed a spacelike hypersurface ;-)), but I'm not too harsh with textbook authors concerning typos. Tell me a recipy how to produce typo-free textbooks ;-)).
 
  • #9
I'd call it "misspoken" rather than "typo". It doesn't matter really. I'm just glad that I've spotted it and that my understanding so far is correct.
 
  • #10
martinbn said:
Many places at the same time.
The text sort of says that, but the correct term for such a surface is "spacelike"--it's a surface that can be viewed as "space"--many places--at an instant of time.
 
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  • #11
Hmm... The book insists: 20 pages later, referring to this figure,
1703188108088.png

it says,
1703188187659.png
 
  • #12
Hill said:
The book insists: 20 pages later, referring to this figure
If by "upper quadrant" they mean the black hole region, this is of course wrong. The constant ##t## lines in the black hole region are timelike, and the constant ##r## hyperbolas are spacelike.

I am skeptical that these were typos. Based on my previous experience reading papers by Susskind, I suspect he is making up his own terminology (where "space-like" means "like a point in space" and "time-like" means "like an instant of time") and either hasn't bothered to check the literature, or doesn't think it matters. Which, given that this book is supposed to be for pedagogy, does not strike me as a sound strategy. I hope I'm wrong.
 
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  • #13
PeterDonis said:
If by "upper quadrant" they mean the black hole region
They do.
PeterDonis said:
his own terminology
Not in this case: earlier in the book he says,

1703201514714.png
 
  • #14
Some terrible search-and-replace disaster?

##t## is a spacelike coordinate inside the horizon which means that lines of constant ##t## (on this 1+1d diagram) are time-like, and vice-versa outside.
 
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  • #15
That's an amazing mistake in a (pre-)introductory textbook then. It's anyway confusing with space-like vs. time-like concerning 3D hypersurfaces (already in SR but the more in GR).

The right local criterion is that a hypersurface is called space-like if the normal vectors are time-like.

In the usual Schwarzschild coordinates for ##r<r_{\text{S}}## the ##t##-coordinate is space-like and the ##r##-coordinate is time-like (which adds to the confusion, because it's labelled ##t## for "time" and ##r## for "radial coordiante" due to the fact that ##t## is the time-like coordinate and ##r## a space-like coordinate outside the event horizon, i.e., for ##r>r_{\text{S}}##).

Now for the hypersurfaces defined by ##t=\text{const}## the lines ##(r,\vartheta,\varphi)=\text{const}##, i.e., the ##t##-lines are spacelike for ##r<r_{\text{S}}##, and they are the "hypersurface normal vectors", and thus these hypersurfaces are time-like.
 
  • #16
Ibix said:
Some terrible search-and-replace disaster?
Y'know, the more I think about it the more plausible this hypothesis becomes.
 
  • #17
Hill said:
earlier in the book he says
In itself that quote could be consistent with standard terminology, since the signs of squared intervals depend on what metric signature convention you adopt. In standard terminology, the quote you give is simply describing the standard timelike signature convention.

But if all he's doing is using the standard timelike signature convention, then he's using it wrong in the other quotes you give. So he can't just be using standard terminology.
 
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  • #18
PeterDonis said:
In itself that quote could be consistent with standard terminology, since the signs of squared intervals depend on what metric signature convention you adopt. In standard terminology, the quote you give is simply describing the standard timelike signature convention.

But if all he's doing is using the standard timelike signature convention, then he's using it wrong in the other quotes you give. So he can't just be using standard terminology.
He uses the standard terminology everywhere else. Here are some examples:

1703472206063.png


1703472246406.png


1703472288111.png
 
  • #19
Hill said:
He uses the standard terminology everywhere else. Here are some examples
Interesting, so his usage is inconsistent. That would seem to be a point in favor of the "typo" theory.
 
  • #20
Ibix said:
Some terrible search-and-replace disaster?
If it were that one would expect it to show up in the example @Hill gave in post #18, but it doesn't.
 

FAQ: Black hole singularity, a time-like surface?

What is a black hole singularity?

A black hole singularity is a point in space where the gravitational field becomes infinite, leading to a breakdown in the laws of physics as we currently understand them. It is the core region of a black hole where density and curvature of spacetime become infinite.

Is a black hole singularity a time-like surface?

No, a black hole singularity is not a time-like surface. A singularity is typically considered a point-like or space-like entity where time and space as we know them cease to exist in their conventional forms. A time-like surface, on the other hand, is a surface where time is a dominant dimension, which is not applicable to the singularity itself.

How does general relativity describe black hole singularities?

General relativity predicts the formation of singularities when massive stars collapse under their own gravity. The equations of general relativity indicate that at the singularity, gravitational forces cause spacetime to curve infinitely, leading to undefined physical quantities such as infinite density and zero volume.

Can we observe a black hole singularity directly?

No, we cannot observe a black hole singularity directly. The singularity is hidden behind the event horizon, which is the boundary beyond which no light or information can escape. Observations are limited to the effects of the black hole on its surroundings, such as the behavior of nearby matter and the emission of X-rays.

What are the implications of black hole singularities for the laws of physics?

Black hole singularities pose significant challenges for the laws of physics, particularly general relativity and quantum mechanics. At the singularity, the known laws of physics break down, and a unified theory of quantum gravity is required to fully explain the phenomena occurring at these extreme conditions. This has led to ongoing research in theoretical physics to reconcile these inconsistencies.

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