Time in a black hole and Weyl curvature

Click For Summary

Discussion Overview

The discussion revolves around the nature of time in black holes, particularly in relation to Kip Thorne's statements about time flow near and inside black holes, as well as the concept of white holes and their theoretical implications. Participants explore the Schwarzschild metric and its significance in understanding these phenomena, along with comparisons to cosmological events like the big crunch.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants reference Kip Thorne's assertion that time slows near the event horizon of a black hole and flows downward towards the singularity, questioning the implications of this for classical time symmetry.
  • One participant suggests that the description of time flow in black holes may also apply to a "big crunch," raising questions about the relationship between Weyl curvature and the direction of time.
  • Another participant discusses the Schwarzschild metric, noting that at the event horizon, the metric becomes singular, leading to a change in the roles of space and time coordinates inside the black hole.
  • There is a mention of white holes as the time reversal of black holes, with some participants expressing skepticism about the physical reality of white holes compared to black holes.
  • One participant questions whether every black hole solution has a corresponding white hole solution, despite the theoretical nature of white holes.

Areas of Agreement / Disagreement

Participants express differing views on the nature and implications of white holes, with some considering them merely mathematical constructs while others suggest they could correspond to physical entities. The discussion remains unresolved regarding the existence and nature of white holes in relation to black holes.

Contextual Notes

Participants note the limitations of the discussion, including the lack of consensus on the physical reality of white holes and the implications of the Schwarzschild metric. There are also references to specific works and theories without providing definitive conclusions.

Naty1
Messages
5,605
Reaction score
40
Kip Thorne says (Lecture in 1993 Warping Spacetime, at Stephan Hawking's 60th birthday celebration, Cambridge, England,)

The flow of time slows to a crawl near the horizon, and beneath the horizon time becomes so highly warped that it flows in a direction you would have thought was spacial: it flows downward towards the singularity. That downward flow, in fact, is why nothing can escape from a black hole. Everything is always drawn inexorably towards the future, and since the future inside a black hole is downward, away from the horizon, nothing can escape back upward, through the horizon.

Comments, interpretations, appreciated.

I thought classical time was always symmetric ...apparently not. Is this same description applicable to a "big crunch" as well? Apparently Weyle curvature at the big bang and black holes seems to go to infinity while at the big crunch it's essentially zero...how does that relate to this "direction" of time??
 
Last edited:
Physics news on Phys.org
I think it's a white hole.
http://casa.colorado.edu/~ajsh/schww.html
 
Hi all!
I think the keypoint of Thorne's statement can be found in the form of the Schwarzschild metric
ds_S^{2} = \left(1-\frac{2M}{r} \right) dt^2 - \left(1-\frac{2M}{r} \right)^{-1} dr^2 - r^2 d \Omega^2
as you can see at the event orizon, located at r_S = 2 M the metric becomes ill defined, i.e. singular. This peculiarity divides the whole space-time in two regions. The outer one which is asymptotically flat, i.e. ds_S^2 \rightarrow dt^2 - \( d \vec{r} \)^2, describing the space surrounding the black hole. And the inner region, which is properly the black hole, a region in which the relative signs of dt^{2} and dr^{2} change. This is the fact pointed out by Thorne. That inside the black hole the space coordinate acts as the temporal one and viceversa, from a causal point of view. More specifically you have that that all the trajectories pointing outward the center can only reach, asymptotically the event horizon.
Hope this helps...forgive my english...
 
Atyy...Kip specifically refers to black holes and I should have made that clear...my quote above is from page 93, THE FUTURE OF THEORETICAL PHYSICS AND COSMOLOGY, 1993
I'll have to check the white hole reference tomorrow...

ALLE: GREAT INSIGHT...Thorne happens to state the Schwarzschild solution you posted (in a slightly different form) earlier in his talk...I'll bet THAT IS what he is referring to...makes sense...
 
I meant that a white hole is the time reversal of a black hole.
 
atyy said:
I meant that a white hole is the time reversal of a black hole.

Mmh...i don't think it is so simple...i mean, a black hole is a physical entity (or, at least, we hope so...) while its white counterpart it's only a mathematical tool needed to cover the entire space-time manifold with the fewest possible number of charts. Indeed I think that Wheeler prooved (sorry but no references...) that a collapsing star cannot create a white hole since the time is not symmetric in the collapsing process. So handle with care...

@Naty: Can you post or link the form of the metric choosen by Thorne? Thnx
 
There are comments regarding this in the first paragraph of
The arrow of time, black holes, and quantum mixing of large N Yang-Mills theories
Guido Festuccia, Hong Liu
http://arxiv.org/abs/hep-th/0611098

I know in the Schwarzschild solution, a white hole is the formal time reverse of a black hole, but I wonder whether it is true that for every black hole solution, there is a corresponding white hole solution (in theory, although it may not be realized in nature)?
 

Similar threads

  • · Replies 22 ·
Replies
22
Views
2K
  • · Replies 40 ·
2
Replies
40
Views
4K
  • · Replies 20 ·
Replies
20
Views
3K
  • · Replies 51 ·
2
Replies
51
Views
6K
  • · Replies 14 ·
Replies
14
Views
2K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 15 ·
Replies
15
Views
3K
  • · Replies 67 ·
3
Replies
67
Views
6K
  • · Replies 35 ·
2
Replies
35
Views
5K
  • · Replies 25 ·
Replies
25
Views
5K