The Schwarzschild Geometry: Part 3 - Comments

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Discussion Overview

The discussion revolves around the Schwarzschild Geometry, specifically focusing on the KS chart and its implications in general relativity. Participants explore the interpretation of lines of constant X and T, the evolution of spheres in spacetime, and the topology of the exterior of spherical bodies. The conversation includes technical explanations, conceptual clarifications, and speculative interpretations related to the geometry.

Discussion Character

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

Main Points Raised

  • Some participants discuss the usefulness of lines of constant X in the KS chart, suggesting they provide a smooth connected picture of the S2xR2 manifold.
  • Others argue that lines of constant T do not cover the whole chart and must be treated as split, leading to confusion about their interpretation.
  • A participant proposes that the term "evolution" in the context of lines of constant X refers to "evolution in time," and suggests postulating an observer's worldline for clarity.
  • There is a discussion about the nature of boundary hyperbolas in the chart, with conflicting views on whether they are spacelike or timelike.
  • Some participants propose an analogy between the evolution of spheres in the KS chart and the exterior of a spherical body, discussing the implications for the geometry and topology of such bodies.
  • There is mention of a minimum size for the exterior of a body below which the geometry must change, as mandated by the KS interior regions.

Areas of Agreement / Disagreement

Participants express differing views on the interpretation of lines of constant T and X, as well as the nature of boundary hyperbolas. The discussion remains unresolved with multiple competing interpretations and no consensus reached.

Contextual Notes

Participants note limitations in understanding the coverage of the chart and the distinctions between different types of lines. There are also unresolved questions regarding terminology and the implications of various interpretations.

  • #31
PeterDonis said:
The fact that the full Kruskal chart for Schwarzschild spacetime looks a lot like a spacetime diagram of an inertial chart in 1+1 Minkowski spacetime is misleading in this respect.
I take it as follows. An inertial chart in ##T,X## coordinates for 1+1 Minkowski spacetime (1 timelike + 1 spacelike dimension) has a diagram that actually extends on all over the ##T,X## plane (i.e. there is not any boundary like the two hyperbolas of Kruskal chart for Schwarzschild spacetime).

As you said for 1+1 Minkowski spacetime the "Kruskal" ##X## coordinate is basically the spherical polar ##r## . Since in this case there is 1 spacelike dimension only, the 'spherical polar ##r##' (i.e. ##X##) takes actually all values in the range ##(- \infty, + \infty)##.
 
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  • #32
cianfa72 said:
An inertial chart in ##T,X## coordinates for 1+1 Minkowski spacetime (1 timelike + 1 spacelike dimension) has a diagram that actually extends on all over the ##T,X## plane (i.e. there is not any boundary like the two hyperbolas of Kruskal chart for Schwarzschild spacetime).
Yes, that's correct. But here ##X## is not a radial coordinate; these coordinates are Cartesian, not spherical. In spherical coordinates the ##T, R## "plane" of Minkowski spacetime is only a half-plane, with ##0 \le R < \infty##.

cianfa72 said:
As you said for 1+1 Minkowski spacetime the "Kruskal" ##X## coordinate is basically the spherical polar ##r## . Since in this case there is 1 spacelike dimension only, the 'spherical polar ##r##' (i.e. ##X##) takes actually all values in the range ##(- \infty, + \infty)##.
No, it doesn't. Minkowski spacetime only goes from ##0 \le r < \infty##. But the maximally extended Schwarzschild spacetime in Kruskal coordinates goes from ##- \infty < X < \infty## even though ##X## is a radial coordinate in spherical coordinates, not a Cartesian coordinate.

So the Kruskal diagram for Schwarzschild spacetime in ##T, X## coordinates, with ##X## a "radial" coordinate in spherical coordinates (i.e., every point in the diagram represents a 2-sphere, and there are hyperbolic boundaries) looks like a standard spacetime diagram for Minkowski spacetime in Cartesian coordinates, i.e., ##X## is a Cartesian coordinate, not a radial coordinate (and if we take the diagram to represent 1+3 Minkowski spacetime, then every point in the diagram represents a 2-plane, not a 2-sphere, and there are no hyperbolic boundaries).

If we take the ##M = 0## case of Schwarzschild spacetime, and keep spherical coordinates, then the whole left half-plane of the Kruskal diagram for Schwarzschild spacetime disappears and only the right half-plane remains (with no hyperbolic boundaries).
 
  • #33
PeterDonis said:
No, it doesn't. Minkowski spacetime only goes from ##0 \le r < \infty##. But the maximally extended Schwarzschild spacetime in Kruskal coordinates goes from ##- \infty < X < \infty## even though ##X## is a radial coordinate in spherical coordinates, not a Cartesian coordinate.
So ##X## as radial coordiante in spherical coordinate can assume negative values ? (i.e. 2-spheres labeled with negative ##X## hence negative area) ?

PeterDonis said:
So the Kruskal diagram for Schwarzschild spacetime in ##T, X## coordinates, with ##X## a "radial" coordinate in spherical coordinates (i.e., every point in the diagram represents a 2-sphere, and there are hyperbolic boundaries) looks like a standard spacetime diagram for Minkowski spacetime in Cartesian coordinates, i.e., ##X## is a Cartesian coordinate, not a radial coordinate (and if we take the diagram to represent 1+3 Minkowski spacetime, then every point in the diagram represents a 2-plane, not a 2-sphere, and there are no hyperbolic boundaries).

If we take the ##M = 0## case of Schwarzschild spacetime, and keep spherical coordinates, then the whole left half-plane of the Kruskal diagram for Schwarzschild spacetime disappears and only the right half-plane remains (with no hyperbolic boundaries).
ok got it !
 
  • #34
cianfa72 said:
So ##X## as radial coordiante in spherical coordinate can assume negative values ?
The ##X## coordinate in Kruskal coordinates in Schwarzschild spacetime can, yes. (Questions about coordinates are meaningless unless you specify which particular chart and which spacetime.) But while the Kruskal ##X## is a radial coordinate, it's not the same radial coordinate as ##r##. (In Kruskal coordinates ##r## is not even a coordinate, it's a function of the coordinates. See below.)

cianfa72 said:
(i.e. 2-spheres labeled with negative ##X## hence negative area) ?
The 2-spheres labeled with negative ##X## do not have negative area. ##X## is not an "areal radius"; a radial coordinate does not have to have a direct relationship with area of 2-spheres. The areal radius ##r## in Kruskal coordinates is a function of both the Kruskal ##X## and the Kruskal ##T##. I believe I give the function in the Insights article.
 
  • #35
PeterDonis said:
The 2-spheres labeled with negative ##X## do not have negative area. ##X## is not an "areal radius"; a radial coordinate does not have to have a direct relationship with area of 2-spheres. The areal radius ##r## in Kruskal coordinates is a function of both the Kruskal ##X## and the Kruskal ##T##. I believe I give the function in the Insights article.
Ah ok, so why is Kruskal ##X## coordinate called 'a radial coordinate? Just because -- as pointed out in the Insight -- it is given as transformation from ##(t,r)## coordinates of Schwarzschild chart ?
 
  • #36
cianfa72 said:
so why is Kruskal ##X## coordinate called 'a radial coordinate?
Because, as noted, the points in the Kruskal diagram label 2-spheres, not 2-planes. Since ##X## is spacelike everywhere, and does not point along any of the 2-spheres, it must point in a radial direction.
 
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  • #37
PeterDonis said:
Since ##X## is spacelike everywhere, and does not point along any of the 2-spheres, it must point in a radial direction.
In other words since the metric in Kruskal coordinates ##(T,X,\theta,\phi)## is diagonal then ##\partial_X## is orthogonal both to ##\partial_{\theta}## and ##\partial_{\phi}## hence it does not point along any of the 2-spheres.
 
  • #38
cianfa72 said:
since the metric in Kruskal coordinates ##(T,X,\theta,\phi)## is diagonal then ##\partial_X## is orthogonal both to ##\partial_{\theta}## and ##\partial_{\phi}## hence it does not point along any of the 2-spheres.
Yes. Although you can see that the 2-spheres in any spherically symmetric spacetime are orthogonal to the other two spacetime dimensions by purely invariant reasoning. The argument is simple: suppose that there were some vector field in the spacetime not lying within the 2-spheres (i.e., not expressible as a linear combination of the 2-sphere basis vectors) but also not orthogonal to the 2-spheres (i.e., nonzero inner product with some vector on each of the 2-spheres). This would be mathematically equivalent to having a vector field on a 2-sphere that is nonzero everywhere, which is impossible by the "hairy ball" theorem. So the remaining 2 dimensions of the spacetime must be everywhere orthogonal to the 2-spheres. (I first encountered this argument in MTW; I don't know what other GR textbooks describe it.)
 
  • #39
PeterDonis said:
suppose that there were some vector field in the spacetime not lying within the 2-spheres (i.e., not expressible as a linear combination of the 2-sphere basis vectors) but also not orthogonal to the 2-spheres (i.e., nonzero inner product with some vector on each of the 2-spheres).
ok, that would mean that such a vector field would always have a nonzero component lying within the 2-spheres.

PeterDonis said:
This would be mathematically equivalent to having a vector field on a 2-sphere that is nonzero everywhere, which is impossible by the "hairy ball" theorem.
By the same argument at some point on each 2-sphere the basis vector fields (coordinate basis) ##\partial_{\theta}## and ##\partial_{\phi}## must vanish (not at the same point). Is it related to the reason why it is impossible to map a complete 2-sphere with only one chart ?
 
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  • #40
cianfa72 said:
that would mean that such a vector field would always have a nonzero component lying within the 2-spheres.
Yes, exactly. And that is impossible by the hairy ball theorem: it is impossible to have a vector field on a 2-sphere that is everywhere nonzero.

cianfa72 said:
By the same argument at some point on each 2-sphere the basis vector fields (coordinate basis) ##\partial_{\theta}## and ##\partial_{\phi}## must vanish (not at the same point). Is it related to the reason why it is impossible to map a complete 2-sphere with only one chart ?
Yes, it is the reason why it is impossible to map a complete 2-sphere with only one chart.
 
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