Schwarzschild solution and velocity of stationary observer

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Discussion Overview

The discussion revolves around the concept of velocity as it pertains to a stationary observer in the context of the Schwarzschild solution in general relativity. Participants explore the implications of different coordinate systems on the measurement of velocity, particularly focusing on the observer's own four-velocity and how it relates to the Schwarzschild metric.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant expresses confusion about how velocity is perceived from different reference frames, particularly in relation to the Schwarzschild solution.
  • Another participant asserts that an observer's own four-velocity is always (1,0,0,0), but this is contested as being true only in special relativity.
  • There is a discussion about the relationship between coordinate systems and the calculation of velocity, with a reference to the equation U^\mu U^\nu g_{\mu \nu} = -1.
  • Some participants suggest that the velocity calculated from the Schwarzschild metric may not represent what the observer measures themselves.
  • A later reply indicates that the equation holds in any coordinate system, including Schwarzschild coordinates, and emphasizes the independence of tensor equations from specific coordinates.
  • Participants reference external resources, such as a Wikipedia page, to clarify concepts related to static observers in the Schwarzschild vacuum.

Areas of Agreement / Disagreement

There is no consensus on the interpretation of the observer's four-velocity in general relativity versus special relativity. Participants express differing views on how to understand and calculate velocity in the context of the Schwarzschild solution.

Contextual Notes

Some participants acknowledge the need for clarity regarding the application of the four-velocity equation in various coordinate systems, and there are indications of uncertainty about the implications of using different metrics.

dianaj
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Hey all,

I suddenly find myself very confused about velocity and coordinate systems. I have a feeling this is very simple, but sometimes the mind just curls up, you know? ;)

When you ask what an observer observe, you need to see things from his point of view - his reference frame. And his reference frame must be a frame moving with him. But this reference frame can look very different depending on what coordinates he choose, right? So this frame can e.g. be an inertial frame, but it can also be some weird twisted frame, right?

Consider the Schwarzschild solution and a stationary observer at a distance r from the center (beyond 2GM). He must of course be using some sort of thrust to stay still.

Now, my book says: "Work in inertial coordinates such that the observer is in the rest frame. Then the velocity of the observer is U = (1,0,0,0)." So the observer, using inertial coordinates, sees himself as having velocity U=(1,0,0,0)?

Another place in my book, the velocity of this stationary observer is described as

U=((1-\frac{2GM}{r})^{-1/2},0,0,0)

This is obviously in a coordinate system where the metric is the Schwarzschild metric itself. So this is another kind of reference frame. But is this what the observer himself measures? I think I have a tendency to consider a omnipresent observer looking down at the whole S.T., and I think I have considered

U=((1-\frac{2GM}{r})^{-1/2},0,0,0)

as the velocity that this omnipresent observer sees the stationary observer having. But this is wrong, right?

So basically, when you want to know your velocity, you choose a coordinate system, find the corresponding metric and then calculate the velocity from the relation

U^\mu U^\nu g_{\mu \nu} = -1.

And what you find is the velocity that you see yourself having. Right?
 
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An observer's own four-velocity is always (1,0,0,0), isn't it?
 
dianaj said:
So basically, when you want to know your velocity, you choose a coordinate system, find the corresponding metric and then calculate the velocity from the relation

U^\mu U^\nu g_{\mu \nu} = -1.

And what you find is the velocity that you see yourself having. Right?

Yes.

Edit: Ooops, I meant just the LHS, not sure if the RHS is right - does it work out in Schwarzschild coordinates?
 
Last edited:
atyy said:
Yes.

Edit: Ooops, I meant just the LHS, not sure if the RHS is right - does it work out in Schwarzschild coordinates?

The equation holds in any coordinate system, so it works in Schwarzschild coordinates as well. This is the neat thing about tensors equations and scalars - they don't care much about coordinates. :)
 
Jonathan Scott said:
An observer's own four-velocity is always (1,0,0,0), isn't it?

No, only in special relativity.
 
dianaj said:
No, only in special relativity.

OK - I guess the way I learned GR it had never occurred to me to use "own velocity" in a different way from SR.
 
dianaj said:
The equation holds in any coordinate system, so it works in Schwarzschild coordinates as well. This is the neat thing about tensors equations and scalars - they don't care much about coordinates. :)

OK, good, that's what I thought from Fermi-Walker transport, but sometimes I need to do the computation in another coordinate system for a sanity check :)
 

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