Proper Time Interval: Explaining Δs Relationship

In summary, Δs is related to the proper time interval through the equation Δs = c*ΔTau, where ΔTau represents the proper time between two events. In Minkowski space, a positive Δs2 indicates a real proper time interval, while a negative Δs2 represents a spacelike interval.
  • #1
xma123
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Could anyone explain how Δs is related to the proper time interval?
 
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  • #2
There's no real difference between proper time and [itex]ds[/itex] except for (maybe) a factor of [itex]\pm c[/itex] to make sure that a real trajectory has a positive proper time and that the units are right. Either way, proper time is the analogue of arc length in Euclidean spaces, and for a curved trajectory, one integrates to get the right result (the same way you would in 3D).
 
  • #3
xma123 said:
Could anyone explain how Δs is related to the proper time interval?

Δs is really c*ΔTau where ΔTau is the proper time interval. In Minkowski space and using the (+---) sign convention, when Δs2 is positive, then the proper time interval is real and represent the proper time of a clock that moves inertially between the two events. If Δs2 is zero then it represents a light like interval. (i.e. ΔTau is zero). If Δs2 is negative, the proper time interval is imaginary and in that case, no real particle or physical clock can physically travel between those two events and the interval is said to be spacelike and after reversing the signature to (-+++) represents the proper distance (ruler) measurement between the two events.
 

Related to Proper Time Interval: Explaining Δs Relationship

1. What is the proper time interval (Δs)?

The proper time interval, denoted as Δs, is a concept in special relativity that measures the time separation between two events in a reference frame. It takes into account both the time and spatial components of an event, and is invariant across different reference frames.

2. How is proper time interval related to space-time?

The concept of proper time interval is closely related to the idea of space-time, which combines the three dimensions of space and one dimension of time into a four-dimensional continuum. In space-time, the proper time interval between two events is the shortest time that could possibly elapse between them, as measured by a clock moving along the same path as the events.

3. What is the formula for calculating proper time interval?

The formula for calculating proper time interval is Δs = √(Δt² - Δx²), where Δt is the time separation between the two events and Δx is the spatial separation between them. This formula takes into account the different time and space components of an event and gives the proper time interval, which is invariant across reference frames.

4. How does proper time interval differ from coordinate time?

Proper time interval and coordinate time are two different ways of measuring time in special relativity. Proper time interval is the time measured between two events by an observer who is in the same reference frame as the events, and is invariant across all reference frames. On the other hand, coordinate time is the time measured by an observer who is at rest in a specific reference frame, and can vary depending on the relative motion of different observers.

5. What are some real-life applications of proper time interval?

Proper time interval has several real-life applications, especially in the fields of astrophysics and particle physics. For example, it is used to calculate the time dilation effects experienced by objects moving at high speeds, such as satellites. It is also used in the measurement of atomic clocks and in the study of subatomic particles, where precise measurements of time are crucial.

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