Proper Distance, Rest Length: What to Know

In summary, the proper distance between two spacelike separated events in special relativity can be determined by the rest length of a rod connecting the events in an inertial frame. This frame can always be found by choosing the spacelike vector as one of the basis vectors. However, in general relativity, this method may not work as there may not be a unique way to measure the distance between two spacelike points due to the lack of global inertial frames.
  • #1
JD96
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Hello,

Could someone check my following statement: The proper distance between two spacelike separated events can be thought of as the rest length of a rod that connects both events in an inertial frame in which both events happen simultaneous.

Thanks in advance!
 
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  • #2
That's correct, and you can always find this frame of reference, by choosing the spacelike vector as one of the basis vectors of an inertial reference frame in Minkowski space.
 
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  • #3
Okay, that makes sense :) Thanks for the quick reply!
 
  • #4
One should note that this does not necessarily work in GR. In SR where there are global inertial frames, one can always define a rest frame for such a rod, in GR if the two space like points are too far apart, there may not be a unique way to measure the distance between them (different "straight line paths" may connect the same two points).
 
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  • #5


Yes, your statement is correct. The proper distance between two spacelike separated events is the distance measured by an observer at rest in the same inertial frame as the events. It can also be thought of as the rest length of a rod connecting the two events in that frame. This distance is independent of the relative motion of the observer and the events, making it an important concept in understanding the geometry of spacetime.
 

FAQ: Proper Distance, Rest Length: What to Know

1. What is proper distance?

Proper distance, also known as comoving distance, is a measure of the distance between two objects in the universe at a given point in time, taking into account the expansion of the universe. It is different from the physical distance, as it considers the change in distances due to the expansion of space.

2. How is proper distance calculated?

Proper distance is calculated by using the formula D = c * ∫(t0, t1) dt / a(t), where c is the speed of light, t0 is the time of emission, t1 is the time of observation, and a(t) is the scale factor of the universe at a given time. This formula takes into account the expansion of space and provides a more accurate measurement of distance.

3. What is the difference between proper distance and rest length?

Rest length is the length of an object when it is at rest, meaning it is not moving or being affected by the expansion of the universe. Proper distance, on the other hand, takes into account the expansion of space and can be larger than the rest length due to the stretching of space over time.

4. Why is proper distance important in cosmology?

Proper distance is important in cosmology because it provides a more accurate measurement of distances between objects in the universe. It is essential in understanding the large-scale structure of the universe and how it has evolved over time. Proper distance also plays a crucial role in determining the expansion rate of the universe and the overall geometry of the universe.

5. Can proper distance be measured?

Yes, proper distance can be measured using various techniques, such as redshift measurements, gravitational lensing, and parallax. However, these measurements require advanced technology and precise calculations, as proper distance is constantly changing due to the expansion of the universe. Therefore, it can be challenging to measure accurately over large distances.

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