How does this equation imply that time slows down?

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In summary, the concept of time dilation in Special Relativity states that time appears to move slower for a person in motion relative to someone at rest. This is represented by the equation T = T0γ, where T0 is the time measured by a person at rest and T is the time measured by someone in motion. However, this equation does not take into account the relativity of simultaneity, which means that both time and space should be considered together. It is important to use the Lorentz transformation to accurately understand the effects of time dilation. Some textbooks may simplify the concept by only focusing on time dilation, but it is important to also consider relativity of simultaneity for a complete understanding.
  • #1
Heatherfield
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I've studied SR previously and, after a lot of work, grew to understand it. Now I have to re-work through it using a different textbook and can't figure out the deal with time dillation.

I derived the equation

T = T0γ

With relative ease. In this equation, T0 is measured by a person at rest (in his own frame) while T is measured by a person moving (in the rest frame of the first observer. Due to the nature of γ, T will always be larger than T0.

At this point, my textbook states that this means that the observer at rest observes time slowing down for the moving person. I don't understand this.

Say a spaceship was passing by Earth. I'm laying in the grass, looking up. In my frame, I'm at rest. The spaceship passes over, quickly. I measure the time I can see it. Since I'm at rest in my own frame, this time is T0.

The same chain of events could be measured from the spaceship. Staying in my frame, my equation tells me that the spaceship measures a higher time. Perhaps I measured 4 seconds, while the spaceship measured 8!

In other words, more time passed for the ship. Doesn't that mean that I observe a spaceship where time is moving much faster! After all, I "saw" twice as much as time passing on their clocks than on mine!
 
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  • #2
The most important thing to remember about time dilation is that you can't just look at time dilation. You have to also take into account relativity of simultaneity--or, to put it another way, you have to look at both space and time together, not just time. The equation ##T = T_0 \gamma## does not do that, so if you just use that equation by itself, you will be misled.

My advice would be to first assign coordinates in your rest frame to the two events of interest (the ones separated by a time interval ##T_0## in your rest frame). Then use the Lorentz transformation to transform those coordinates into the ship's rest frame. Looking at both the time and space coordinates, not just the time coordinate, should help to resolve your confusion.

(Similar remarks apply to length contraction.)
 
  • #3
Thanks. This bothers me though, because the textbook completely ignores relativity of simultaneity at this point. Not even a single mention. It merely creates the lorenz transformation for time dillation from the postulates of SR, then uses that to deduce time slowing down for moving observers. Any clue as to why the book wants me to make this logical step, even though I cannot (according to your answer).
 
  • #5
Heatherfield said:
In this equation, T0 is measured by a person at rest (in his own frame) while T is measured by a person moving (in the rest frame of the first observer.
It is a little more subtle than that. T and T0 are measured between two given events. T is in a reference frame for which the two events are co-located. T0 is in a frame which is moving at velocity v wrt the first. In this frame the two events are not co-located.

That said, I agree that the Lorentz transformation is the way to go. It will automatically simplify when appropriate.
 
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  • #6
Heatherfield said:
Thanks. This bothers me though, because the textbook completely ignores relativity of simultaneity at this point. Not even a single mention. It merely creates the lorenz transformation for time dillation from the postulates of SR, then uses that to deduce time slowing down for moving observers. Any clue as to why the book wants me to make this logical step, even though I cannot (according to your answer).
As someone who also has only a thin knowledge of Relativity, I can guess:

When being introduced to a subject, it is often better to keep things simple and tackle only one issue at a time. Bringing together both time dilation and relativity of simultenaity adds unnecessary complexity (IMO) and potential to mistake one issue for the other or think they are interdependent when in reality they are completely separate issues.

For that reason I prefer starting with simpler scenarios where only time dilation is needed, such as a simple version of the twins paradox.
 
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  • #7
Everything is easier to keep track of if you specify reference events in spacetime.

Event A: the nose of the spaceship crosses a "starting line" to your left

Event B: the nose of the spaceship crosses a "finishing line" to your right

A single wristwatch worn by a passenger at the nose of the spaceship logs the spaceship's proper time. (Let's not worry about YOUR proper time right now.) Between Events A and B, that wristwatch measures a proper time interval ##\Delta t_0##.

For you on the ground, the coordinate time interval between Events A and B is measured by two different synchronized clocks: one at the starting line, which takes a reading when the nose of the spaceship arrives (marking your coordinate time for Event A); and the other at the finishing line, which records your coordinate time for Event B. After the readings are taken, you compare the clocks and find that Event B happened a time ##\Delta t## after Event A.

The time dilation formula tells you that ##\Delta t = \gamma \Delta t_0##, guaranteeing that ##\Delta t > \Delta t_0##. So you would say that the passenger ages less than you do during the spaceship's journey from starting line to finishing line.
Now, if you wanted to bring YOUR proper time into this, then you'd need to specify events that both happen at YOUR location. For example:

Event C: someone at the NOSE of the spaceship gives you a high-five while passing by

Event D: someone at the TAIL of the spaceship gives you a high-five while passing by

Because you're physically present at both events, YOUR wristwatch logs the inertial proper time interval between Events C and D. From the spaceship's perspective, it is YOU who is "moving" while the spaceship is "stationary." Two different synchronized clocks on the spaceship measure the coordinate time interval between Events C and D: one at the nose of the ship, which takes a reading when you high-five the nose-passenger; and the other at the tail of the ship, which takes a reading when you high-five the tail-passenger.

In this scenario, the passengers on the ship would say that you age less than they do during "your journey" from nose to tail.
 
  • #8
Heatherfield said:
I've studied SR previously and, after a lot of work, grew to understand it. Now I have to re-work through it using a different textbook and can't figure out the deal with time dillation.

I derived the equation

T = T0γ

With relative ease. In this equation, T0 is measured by a person at rest (in his own frame) while T is measured by a person moving (in the rest frame of the first observer. Due to the nature of γ, T will always be larger than T0.

##T_o## is the time that elapses between two events that occur at the same place. This is called the proper time. Note that this can be the time that elapses between two events in only one of your two frames.

So, in the example of you watching a ship pass across the sky, we can choose two events such as "ship is located on the western horizon" and "ship is located on the eastern horizon". For you those two events occur at different places so the time that elapses between them, as measured by say your wristwatch, is not a proper time. For a person aboard the ship they do occur at the same place, say his chair, so the time that elapses between them as measured on his watch is a proper time.
 
  • #10
Heatherfield said:
I've studied SR previously and, after a lot of work, grew to understand it. Now I have to re-work through it using a different textbook and can't figure out the deal with time dillation.

I derived the equation

T = T0γ

With relative ease. In this equation, T0 is measured by a person at rest (in his own frame) while T is measured by a person moving (in the rest frame of the first observer. Due to the nature of γ, T will always be larger than T0.

At this point, my textbook states that this means that the observer at rest observes time slowing down for the moving person. I don't understand this.

Say a spaceship was passing by Earth. I'm laying in the grass, looking up. In my frame, I'm at rest. The spaceship passes over, quickly. I measure the time I can see it. Since I'm at rest in my own frame, this time is T0.

The same chain of events could be measured from the spaceship. Staying in my frame, my equation tells me that the spaceship measures a higher time. Perhaps I measured 4 seconds, while the spaceship measured 8!

In other words, more time passed for the ship. Doesn't that mean that I observe a spaceship where time is moving much faster! After all, I "saw" twice as much as time passing on their clocks than on mine!

Moving clock runs slowly. Mathematically:

Tnot_moving = Tmovingγ

if we change that to your notation we get this:

T0 = Tγ

Not this: T = T0γ
 
  • #11
jartsa said:
Moving clock runs slowly. Mathematically:

Tnot_moving = Tmovingγ

That's a simplification that's often presented in introductory discussions of relativity, but it leads to the very type of learner confusion that caused the OP to start this thread. Here's why. If an observer is moving in such a way that he co-moves with a clock, and that motion is relative to a stationary (that is, not-moving) clock, then he will observe that the stationary clock is running slow.

Now I realize that you can get around this pedagogical difficulty by emphasizing that by "moving clock" you mean moving relative to the observer. And if that works for the learners you're trying to educate, then that's what you can do.

For me, though, I find that he following scheme works better because it forces the learner to think about a pair of events, and the time that elapses between them. So rather than using "not moving" and "moving" to distinguish between the clocks, one can use "proper time" and "dilated time" to distinguish between the things that the clocks are measuring. The dilated time is always larger than the proper time, whether it's the moving clock or the not-moving clock that's measuring it. And for a time to be a proper time it must be the time that elapses between two events that occur in the same place, whether that's the same place for the moving frame or the same place for the stationary frame.
 

1. How does this equation imply that time slows down?

According to Einstein's theory of relativity, time slows down for an object in motion relative to an observer. This is represented by the equation t' = t/√(1-v²/c²), where t' is the time observed by the moving object, t is the time observed by the stationary observer, v is the velocity of the moving object, and c is the speed of light.

2. What is the significance of the speed of light in this equation?

The speed of light, denoted by c, is a fundamental constant in Einstein's theory of relativity. It represents the maximum speed at which any object can travel in the universe, and is used to calculate the time dilation effect in the equation t' = t/√(1-v²/c²).

3. How does this equation relate to the concept of time dilation?

Time dilation is the phenomenon in which time appears to run slower for an object in motion relative to an observer. The equation t' = t/√(1-v²/c²) is used to calculate the time dilation effect, as it shows how the observed time (t') is affected by the velocity (v) of the moving object relative to the speed of light (c).

4. Can you provide an example of how this equation can be applied?

One example of how this equation can be applied is in the famous "twin paradox" thought experiment. In this scenario, one twin stays on Earth while the other twin travels through space at a high velocity. When the traveling twin returns to Earth, they would have aged less than their twin who stayed on Earth due to the time dilation effect calculated by the equation t' = t/√(1-v²/c²).

5. Is this equation always applicable, or are there certain conditions that must be met?

This equation is applicable in situations where the relative velocity between two objects is close to the speed of light. It is most commonly observed in scenarios involving high-speed travel, such as space travel or particle accelerators. Additionally, the effects of time dilation become more pronounced as the velocity approaches the speed of light, but are negligible at lower speeds.

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