Insights The Schwarzschild Geometry: Part 3 - Comments

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The discussion focuses on the Schwarzschild Geometry and its implications in general relativity (GR). Participants address a minor error in the original post regarding the assumption of the GR model's validity for all r > 0, clarifying it should be "we will" instead of "here will will." They explore the significance of lines of constant X and T in the Kruskal-Szekeres (KS) chart, emphasizing that these lines represent timelike worldlines of observers and illustrate the manifold's topology as S² x R². The conversation also touches on the differences between the KS congruence and ordinary body congruences, noting that the exterior of a spherical body cannot be smoothly reduced to a point body. Overall, the thread delves into the intricate relationships between geometry, topology, and physical interpretations in GR.
  • #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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