Calculating Proper Time for an Object Under Constant Acceleration

In summary, the conversation discusses the correct way to calculate the proper time for an object under constant acceleration. It is noted that using the formula v = at would result in v > c after a certain amount of time, which is not possible. The correct formula involves hyperbolic trigonometric functions and assumes constant proper acceleration. The conversation also touches on the differences between constant proper acceleration and constant coordinate acceleration, and the implications for both the accelerating object and the inertial observer. The use of Latex in the discussion is also mentioned.
  • #1
jacksonwalter
42
0
Is this the correct way to calculate the proper time that has passed for an object under constant acceleration over the time interval [0,t1]? I just downloaded and started teaching myself how to use LaTex today so bear with me here. I can get the output PDF file but I don't know how to insert everything into the thread here, so I just attached it, and https://docs.google.com/fileview?id=0BxjDgugfV3GMYTdhNjI5OWYtNjUyZi00MzcwLTlkNjUtOWQ1NDU0NjNkYzFj&hl=en" a link to it in Google Docs.
 

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  • #2
Careful; it is not true that [itex]v = at[/itex], as this would give [itex]v > c[/itex] after sufficient time.
 
  • #3
No, I don't think so because it's going to take more and more energy to maintain that constant acceleration, and it would take an infinite amount of energy to go past c. I'm assuming that the thing accelerating is increasing it's power in order to maintain constant acceleration.
 
  • #4
I didn't check, but this site is usually very good:
http://math.ucr.edu/home/baez/physics/Relativity/SR/rocket.html
"The proper time as measured by the crew of the rocket (i.e. how much they age) will be denoted by T, and the time as measured in the non-accelerating frame of reference in which they started (e.g. Earth) will be denoted by t."
 
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  • #5
George Jones said:
Careful; it is not true that [itex]v = at[/itex], as this would give [itex]v > c[/itex] after sufficient time.
jacksonwalter said:
No, I don't think so because it's going to take more and more energy to maintain that constant acceleration, and it would take an infinite amount of energy to go past c. I'm assuming that the thing accelerating is increasing it's power in order to maintain constant acceleration.
George is correct. In your formula for t>c/a you get FTL travel. Your expression is wrong at that point, but up until then it should be fine. It would be constant coordinate acceleration, not constant proper acceleration. Also, at t>c/a you get imaginary results for your proper time which would clue you in that there is a problem.
 
  • #6
DaleSpam said:
It would be constant coordinate acceleration, not constant proper acceleration.

And consequently, the acceleration as measured by an accelerometer (e.g., bathroom scales) carried by the object would not be constant.
 
  • #7
Yea, that website covers pretty much everything. I'm curious where the hyperbolic trig functions came from, though.

So, if someone could check my calculation and also tell me how to insert things from LaTex that would be awesome.
 
  • #8
jacksonwalter said:
I'm curious where the hyperbolic trig functions came from, though.
They come from the assumption of constant proper acceleration instead of your assumption of constant coordinate acceleration.
 
  • #9
atyy said:
I didn't check, but this site is usually very good:
http://math.ucr.edu/home/baez/physics/Relativity/SR/rocket.html
"The proper time as measured by the crew of the rocket (i.e. how much they age) will be denoted by T, and the time as measured in the non-accelerating frame of reference in which they started (e.g. Earth) will be denoted by t."

I just did a quick scan of that reference and it looks pretty awkward. The deriviation starts with the rocket having a constant acceleration wrt the inertial observer. That would mean an ever increasing acceleration wrt the people in the rocket. Not realistic.

The derivation I am familiar with starts with a constant acceleration wrt the people in the rocket. That gives an ever diminishing acceleration wrt the inertial observer.
 
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  • #10
Hi MikeLizzi, I think you misread the Baez page. The linked derivation uses constant proper acceleration. Jacksonwalter's derivation uses constant coordinate acceleration.
 
  • #11
MikeLizzi :
The derivation I am familiar with starts with a constant acceleration wrt the people in the rocket. That gives an ever diminishing acceleration wrt the inertial observer.
That being the case can we deduce that the interial observer will always be able to see the accelerating rocket, forever approaching c but not getting there. While the rocket will eventually lose the inertial observer behind an horizon ?
 
  • #12
jacksonwalter said:
Yea, that website covers pretty much everything. I'm curious where the hyperbolic trig functions came from, though.

Look at section 2.10, which starts on page 35, of Gron and Hervik,

http://books.google.com/books?id=Iy...rontcover&dq=hervik&cd=2#v=onepage&q=&f=false
jacksonwalter said:
So, if someone could check my calculation and also tell me how to insert things from LaTex that would be awesome.

If you want to insert Latex in a line of prose, surround your LateX code by the the tags itex and \itex, where the tags are inside square brackets. For example,

Code:
The energy of an individual photon, itex E = \hbar \omega /itex is used to derive

produces:

The energy of an individual photon, [itex]E = \hbar \omega[/itex], is used to derive

If you want to insert Latex in a stand-alone line, surround your LateX code by the the tags tex and \tex, where the tags are inside square brackets. For example,

Code:
The energy of an individual photon, 

tex E = \hbar \omega, /tex

is used to derive

produces:

The energy of an individual photon,

[tex]E = \hbar \omega,[/tex]

is used to derive

tex, \tex, itex, \itex all should be surrounded by square bracket, but if I did this in my examples, the actual Latex would not appear.
 
  • #13
Mentz114 said:
MikeLizzi :

That being the case can we deduce that the interial observer will always be able to see the accelerating rocket, forever approaching c but not getting there. While the rocket will eventually lose the inertial observer behind an horizon ?

Don't know, never extrapolatedd the transformation out that far. Good question for somebody to answer.
 
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  • #14
DaleSpam said:
Hi MikeLizzi, I think you misread the Baez page. The linked derivation uses constant proper acceleration. Jacksonwalter's derivation uses constant coordinate acceleration.

You are right. I scanned it to fast. So the derivation must be the same as the one I'm famliar with. It's just that I can't read the format of the equations. I guess the author didn't know Latex either.

added a few minutes later: Ok, I can now see that the equations are the same. My bad.
 
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  • #15
Mentz114 said:
MikeLizzi :

That being the case can we deduce that the interial observer will always be able to see the accelerating rocket, forever approaching c but not getting there. While the rocket will eventually lose the inertial observer behind an horizon ?

This depends on how things are set up, but, in the usual set-up, this is close to what happens. In this set-up, the inertial observer does cross the horizon, but, similarly to what happens with a black hole event horizon, the the rocket observer never quite sees the inertial observer cross the horizon. The rocket observer see the inertial observer more and more redshifted. See

https://www.physicsforums.com/showthread.php?p=2215073#post2215073

MikeLizzi said:
I guess the author didn't know Latex either.

Originally, this was written for an internet discussion group in 1996, and LateX was not implemented by this discussion group.
 
  • #16
DaleSpam said:
George is correct. In your formula for t>c/a you get FTL travel. Your expression is wrong at that point, but up until then it should be fine. It would be constant coordinate acceleration, not constant proper acceleration. Also, at t>c/a you get imaginary results for your proper time which would clue you in that there is a problem.

Yea, it only works for t<c/a, but I only wanted it to work on the interval (0,t), as that's the interval where it wouldn't require an infinite amount of energy. I think the other guy's derivation is better though.

Thanks for the responses, and thanks for the LaTex help George.

Last question: So the difference between proper acceleration and proper time is similar to the difference between between proper time and 'coordinate' time? Could I say proper acceleration [tex] = \frac{d^{2}x}{dT} [/tex] if T = proper time? i.e proper acceleration is the acceleration in the ship's reference frame and and coordinate acceleration is the acceleration as seen from earth?
 
  • #17
jacksonwalter said:
Last question: So the difference between proper acceleration and proper time is similar to the difference between between proper time and 'coordinate' time? Could I say proper acceleration [tex] = \frac{d^{2}x}{dT} [/tex] if T = proper time? i.e proper acceleration is the acceleration in the ship's reference frame and and coordinate acceleration is the acceleration as seen from earth?
Actually it's a bit more complicated than that.

You might find my derivation within the thread Questions about acceleration in SR helpful, in posts #13, #14, #15 of that thread and a correction in post #28 to equation (5).

In fact, the proper acceleration is given by

[tex]\frac{d^2x}{dt^2} \left( \frac{dt}{d\tau} \right) ^3 [/tex]​

which follows from equations (2) and (12) in my derivation. [itex]dt/d\tau[/itex] is the Lorentz factor [itex]\gamma = 1 / \sqrt{(1 - v^2 / c^2)}[/itex].
 
  • #18
George Jones said:
tex, \tex, itex, \itex all should be surrounded by square bracket, but if I did this in my examples, the actual Latex would not appear.
By the way, I recently found out there's a little-publicised way of getting the characters "[noparse][tex][/noparse]" to appear in a post.

[noparse][noparse][tex][/noparse][/noparse]
 
  • #19
DrGreg said:
Actually it's a bit more complicated than that.

You might find my derivation within the thread Questions about acceleration in SR helpful, in posts #13, #14, #15 of that thread and a correction in post #28 to equation (5).

In fact, the proper acceleration is given by

[tex]\frac{d^2x}{dt^2} \left( \frac{dt}{d\tau} \right) ^3 [/tex]​

which follows from equations (2) and (12) in my derivation. [itex]dt/d\tau[/itex] is the Lorentz factor [itex]\gamma = 1 / \sqrt{(1 - v^2 / c^2)}[/itex].

Yea, it sucks having not quite taken a formal course in SR + GR yet, just a lot of reading and hand waving. Thanks though, lot of good insight.
 

Related to Calculating Proper Time for an Object Under Constant Acceleration

1. What is proper time?

Proper time is a concept in relativity that refers to the time measured by a clock that is at rest relative to the observer. It is the time experienced by an object or person in its own frame of reference, and it is the most fundamental measure of time in the theory of relativity.

2. How do you calculate proper time?

To calculate proper time, you need to know the speed of the object or observer in question and the length of time that has passed for that object or observer. The equation for proper time is t = t0√(1- v2/c2) where t is the proper time, t0 is the time in the rest frame, v is the speed, and c is the speed of light.

3. Why is proper time important in relativity?

Proper time is important in relativity because it is the only quantity that is independent of the frame of reference. It is a fundamental concept that allows us to make accurate predictions about the behavior of objects and observers moving at different speeds. It also helps us understand the effects of time dilation and how time is experienced differently by different observers.

4. Can proper time be negative?

No, proper time cannot be negative. Proper time is always a positive quantity, as it represents the time experienced by an object in its own frame of reference. Negative values would imply that an object has experienced time traveling backwards, which is not possible according to the laws of physics.

5. How is proper time different from coordinate time?

Proper time and coordinate time are different ways of measuring time in relativity. Proper time is the time experienced by an object in its own frame of reference, while coordinate time is the time measured by an observer in a different frame of reference. Proper time is absolute, while coordinate time is relative to the observer's frame of reference. Additionally, proper time takes into account the effects of time dilation, while coordinate time does not.

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