Time like spacetime interval, proper time, and time dilation

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SUMMARY

The discussion centers on the relationship between time like spacetime intervals, proper time, and time dilation, emphasizing that proper time is invariant for both stationary and traveling observers. It is established that while the proper time between ticks of identical clocks is invariant, the relativity of simultaneity affects how observers perceive time dilation. The conversation also clarifies that proper time and coordinate time are distinct, with the former being the "distance" along a clock's worldline, while the latter is dependent on the observer's frame of reference. The discussion concludes that the twin paradox is not a true paradox when relativity of simultaneity is properly accounted for.

PREREQUISITES
  • Understanding of proper time and coordinate time in the context of special relativity.
  • Familiarity with the concept of time dilation and the relativity of simultaneity.
  • Knowledge of Minkowski diagrams for visualizing spacetime intervals.
  • Basic grasp of synchronization conventions, particularly Einstein's synchronization.
NEXT STEPS
  • Study the implications of the twin paradox in special relativity.
  • Learn about Minkowski diagrams and their application in visualizing spacetime events.
  • Research different clock synchronization methods beyond Einstein's convention.
  • Explore the mathematical formulation of time dilation and its applications in physics.
USEFUL FOR

This discussion is beneficial for physicists, students of relativity, and anyone interested in the intricacies of time measurement and synchronization in the context of special relativity.

  • #31
Possibly you need to take a step back. Maybe the notion of being "at rest" is not what you really want to talk about.

You had been suggesting that a remote object is "at rest" if it remains at a constant distance (constant round trip light time) from a selected local object. There is a term used to characterize a set of objects that maintain a fixed distance from one another: Born Rigidity
 
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  • #32
cianfa72 said:
That's good fo SR I believe. What about in the context of GR ?
In GR you don’t need to worry about Newton’s laws. Otherwise the same definition works. Perhaps with the caveat that the coordinate system should have three spacelike and one timelike coordinates.
 
  • #33
Somewhat related question: would a sufficient definition of “inertial reference frame” in special relativity (assuming isotropy and homogeneity) simply be a reference frame in which Newtons law of inertia holds good? If not, what more would be needed?
 
  • #34
I do not read the previous part of the thread but the definition of IFR is as you said.
 
  • #35
jbriggs444 said:
Set up a coordinate system in which Newton's laws hold good. An object is "at rest" if its spatial coordinates are constant in such a system.
So this notion of "at rest" is actually w.r.t. a coordinate system. What about the notion of "being at rest" w.r.t. another body ?
 
  • #36
cianfa72 said:
So this notion of "at rest" is actually w.r.t. a coordinate system.
Yes.
cianfa72 said:
What about the notion of "being at rest" w.r.t. another body ?
In flat space-time, there is relative velocity -- the velocity of the one body in the [momentary, inertial] rest frame of the other. If this is zero then the objects are at rest relative to each other.

In curved space-time, the notion of relative velocity gets slippery. Non-local comparison of velocities becomes ambiguous and one needs to "parallel transport" the velocity of the one into the local frame of the other. The result can depend on the path over which this "parallel transport" is performed.

There is a different notion which might be used. Have you Googled "born rigidity"?
 
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  • #37
Hello to every body. I’ve found the attached image among my old draft papers, which I used in a conference to illustrate the so-called twin paradox:
 effetto gemelli .jpg


Do you have difficulties with Italian ? In short , the test says that , in the flat spacetime of SR (no mass- energy that causes curvature) , one can go from event O to event Q in two (or more...) ways :

1) staying at home, sitting in a very comfortable arm chair, (but let’s ignore for the moment that the Earth is not an inertial RF , from the point of view of relativity) , and just letting proper time (wristwatch time) flow. So, OQ is a piece of geodesics. Spatial coordinate x doesn’t change.
2) moving from O to Q along a curved universe line OSQ , that can be approximated by a succession of short segments , during which the speed maintains constant , and varies from piece to piece. Axes t’ , t” ...are the instantaneous time axes of the MCRFs which are tangent to the curved universe line.

Then, mathematics and physics formulae don’t need to be translated. Fortunately , their language is (or should be) universal and well understood by everybody.
In the end, the result is that the integral of proper time along the curved universe line is shorter than the coordinate time from O to Q : the geodesics OQ , on the time axis of the stationary twin, is the "longest time line” . No paradox, then .

Sorry for my bad English.
 
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  • #38
jbriggs444 said:
There is a different notion which might be used. Have you Googled "born rigidity"?
AFAIK in SR it is related to the hyperbolic motion (basically the spacelike distance as measured from a family or congruence of objects accelerating with constant proper acceleration).
 
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