Distance Between Two Bodies: Am I Correct?

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Discussion Overview

The discussion revolves around the concept of distance between two bodies in the context of General Relativity (GR). Participants explore the definitions and implications of measuring distance in spacetime, addressing both spatial and spacetime distances, and the challenges associated with these measurements.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation

Main Points Raised

  • Some participants argue that the question of distance between two bodies in GR may not make sense due to the dynamic nature of spacetime and the movement of bodies.
  • Others propose that while distance in space can be defined, the challenge lies in determining the appropriate "slice" of spacetime to consider as "space."
  • A participant mentions that it is possible to define the length of a curve in an invariant way using geodesics, but notes that multiple geodesics may connect two points, leading to a multi-valued distance function.
  • There is a discussion about the distinction between "spatial" distance and "spacetime" distance, with some participants seeking clarification on which concept is being referenced.
  • One participant introduces the concept of "radar distance," which defines distance based on the time taken for a light signal to travel to an object and back, highlighting the practical implications of measuring distance in GR.
  • Another point raised is the necessity of establishing a coordinate system to separate distance from time, suggesting that a vector field can help define distance in relation to time.
  • Some participants note that observers who are spacelike related cannot agree on a distance measurement due to the lack of common classical physics.

Areas of Agreement / Disagreement

Participants express differing views on the definition and implications of distance in GR, with no consensus reached on the best approach to measuring distance between bodies. The discussion remains unresolved regarding the nature of spatial versus spacetime distances.

Contextual Notes

Limitations include the dependence on the choice of coordinate systems, the ambiguity in defining "space," and the potential for multiple geodesics connecting points in spacetime, which complicates the measurement of distance.

blue_sky
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In full GR, if somebody ask me what is the distance between two bodies I do not think that the question make sense.
If I use a signal traveling at c when the signal hit the body, in general, it is not in the original point where he was when the question was asked and when the signal is back the body is in a different point too.

Am I correct?

blue
 
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Distance in space is perfectly well defined. What isn't well defined is exactly what "slice" of spacetime we should call "space".

(What I called "space" in the first sentence should actually be called "a spacelike hypersurface of spacetime").
 
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It is possible to define the length of a curve in an invariant way. So take two points in spacetime, and find a geodesic between them. Then compute the length of the geodesic. The problem with this approach is that there is in general more than one geodesic connecting those points. So your distance function might be multi-valued. It is however, the natural generalization of what we do in flat spacetime.

The formal name for this distance function is Synge's biscalar or Synge's world function.
 
Stingray said:
It is possible to define the length of a curve in an invariant way. So take two points in spacetime, and find a geodesic between them. Then compute the length of the geodesic. The problem with this approach is that there is in general more than one geodesic connecting those points. So your distance function might be multi-valued. It is however, the natural generalization of what we do in flat spacetime.

The formal name for this distance function is Synge's biscalar or Synge's world function.

I was referring to "spatial" distance while in your explanation i think you are referringt to the space-time distance. Am I right?

blue
 
Fredrik said:
Distance in space is perfectly well defined. What isn't well defined is exactly what "slice" of spacetime we should call "space"

If what slice of spacetime we should call "space", can I say "spatial" distance is not well defined too?

blue
 
blue_sky said:
I was referring to "spatial" distance while in your explanation i think you are referringt to the space-time distance. Am I right?

Yes, I meant spacetime distance. Points in GR are points in both space and time.

I reread your original post, and you're asking about the distance between objects, not points (sorry). The answer is then long and complicated... Here goes anyways:

Everything in relativity should be thought of as occurring in spacetime, not space. So each body traces out a timelike line. There are several ways you can define distances, but it depends on what exactly you want to do.

The simplest definition supposes the existence of some given reference frame where there exists a particular time parameter. Find the coordinates of each body at a fixed time t, and then compute the geodesic distance between those points. This definition is not unique at all, so there's really no point in using it unless you are trying to understand the results of some (thought) experiment done in a known reference frame.

Next, you can pick a particular value of proper time for one of the bodies, t. Call its position in spacetime at that time z1(t). Now look at the set of (spacelike) geodesics which start at z1(t) and are orthogonal to that body's four-velocity (this is well-defined despite being nonlocal). At least one of these will intersect the other body's worldline. Compute the geodesic distance between that point of intersection and z1(t) to get a distance. This is really very similar to the first method. The difference is that I'm effectively defining a preferred coordinate system by using the rest frame of one of the bodies. This is a very natural thing to do, and is an invariant. There are cases, however, where the prescription fails to work for various reasons. It's usually ok though.

There are other definitions, but they get more complicated (for example, there is one based on null separated points between the two worldlines that is very useful when calculating electromagnetic fields).
 
blue_sky said:
If what slice of spacetime we should call "space", can I say "spatial" distance is not well defined too?
Yes. Since the concept of "space" isn't well defined, the concept of "spatial distance" isn't either.
 
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There is the further problem of relating the units of mass, length and time used in the metric and the field equation to actual measurements that might be made in a laboratory. In GR we assume that these units are constant, but that is an assumption that might not hold. Weyl conformal transformations of the metric re-interpret these units for laboratories separated across space-time curvature.
The key question is "How do you measure it?"
In the 1930's Milne introduced the concept of "radar distance", that defined distance by the time taken for a light signal to leave Earth and be reflected back by the object in question. Not bad seeing radar wasn't invented until a decade later!
This reduced distance measurements to own clock measurements, something we could measure if we could wait long enough!
Garth
 
blue_sky said:
In full GR, if somebody ask me what is the distance between two bodies I do not think that the question make sense.
If I use a signal traveling at c when the signal hit the body, in general, it is not in the original point where he was when the question was asked and when the signal is back the body is in a different point too.

Am I correct?

blue

What you have to do to define distance in GR is to set up a coordinate system that's good enough to separate out distance from time.

The easiest way of doing this is to define a vector that points in the time direction for every observer, a vector field.

Distance will then be perpendicular to time, everywhere.

You can then use standard rulers to measure distance, once you've set up the coordinate system.

In cosmology, I think people tend to use a coordinate system where the time direction is defined to be that which gives the appearance of isotropy of the universe.
 
  • #10
blue_sky said:
In full GR, if somebody ask me what is the distance between two bodies I do not think that the question make sense.
If I use a signal traveling at c when the signal hit the body, in general, it is not in the original point where he was when the question was asked and when the signal is back the body is in a different point too.

Am I correct?

blue

Two observers who are spacelike related to each other do not have any (classical) physics in common, so you are right that they couldn't unambiguously establish the length of the distance between them by operational means.
 

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