Acceleration in special relativity

In summary, the conversation discusses a problem in which the reference frame ##S'## has a constant acceleration and is connected to the rest frame of the rocket ##S## through a Lorentz transformation ##\Lambda##. The problem can be approached by considering an acceleration ##a## and seeing how it transforms under a Lorentz transformation. The solution involves finding the velocity of the rocket ##v(t)## and using it to calculate the proper time ##\tau (t)## through
  • #1
Markus Kahn
112
14
Homework Statement
Consider a spaceship that is accelerating with a constant acceleration ##a' ## (in its rest frame) along the ##x##-direction. Assume that it launches at ##t = \tau = 0## and determine the proper time of the spaceship as a function of coordinate time ##\tau (t)## and vice versa.
Relevant Equations
We weren't given any in particular...
I'm struggling in the details of this exercise. Let ##S'## be the reference frame where the acceleration of the spaceship is constant, in which case we have ##u'(t')= a' t'## (since we assume no acceleration at the beginning). The rest frame of the rocket ##S## is connected to ##S'## via a Lorentz transformation ##\Lambda##.

  1. My first naive attempt to solve this exercise was to use the definition of proper time and just integrate it $$ \tau (t') = \int_0^{t'} \sqrt{1- \left(\frac{u'(\lambda)}{c}\right)^2} d\lambda.$$Turns out I have no clue how to do this and even if, I would still need to substitute ##t'(t,x)## and hope to obtain a reasonable result only depending on ##t## and ##x##, which seems rather unlikely.
  2. The only other possibility I could think of to approach this exercise was to start looking at an acceleration ##a## and see how it transforms under a Lorentz-transfomration. Let ##v## be a constant velocity between two reference frames ##S## and ##S'##, with velocities ##u## and ##u'## respectively. We then have $$a' = \frac{du'}{dt'} = \frac{d}{dt'} \frac{u-v}{1- \frac{uv}{c^2}} = \frac{dt}{dt'}\frac{d}{dt}\frac{u-v}{1- \frac{uv}{c^2}} = \frac{1}{\gamma}\frac{d}{dt}\frac{u-v}{1- \frac{uv}{c^2}}=\frac{1}{\gamma}\left(\frac{c^2 \left(c^2-v^2\right) }{\left(c^2-v u(t)\right)^2}\right)a,$$ where I just wrote ##a\equiv d u /dt##. The problem from here on is that I don't now what values I need to chose to reproduce the situation in the exercise...
I obviously tried googling the solution and found some texts addressing it (see bottom of text), but none of them explained it in a way that I could understand. Section 1.1 of this text uses an approach that seems to resemble my first one, but there signs are different and in general all expression seem to have a slightly different form... (eq. 4 onwards )

Can someone maybe help me on how to approach this exercise?

Some text addressing this exercise:
  • https://www.dpmms.cam.ac.uk/~stcs/courses/dynamics/lecturenotes/section6.pdf
  • Section 1.1
 
Physics news on Phys.org
  • #2
Markus Kahn said:
  1. The only other possibility I could think of to approach this exercise was to start looking at an acceleration ##a## and see how it transforms under a Lorentz-transfomration. Let ##v## be a constant velocity between two reference frames ##S## and ##S'##, with velocities ##u## and ##u'## respectively. We then have $$a' = \frac{du'}{dt'} = \frac{d}{dt'} \frac{u-v}{1- \frac{uv}{c^2}} = \frac{dt}{dt'}\frac{d}{dt}\frac{u-v}{1- \frac{uv}{c^2}} = \frac{1}{\gamma}\frac{d}{dt}\frac{u-v}{1- \frac{uv}{c^2}}=\frac{1}{\gamma}\left(\frac{c^2 \left(c^2-v^2\right) }{\left(c^2-v u(t)\right)^2}\right)a,$$ where I just wrote ##a\equiv d u /dt##.

This is a good start. In this case, we have a constant ##a'## in a continuous sequence of frames where the ship is instantaneously at rest. As the speed of the ship is changing, we have a coordinate acceleration that depends on ##t##.

Note that ##u' =0## in this case and ##u = v##, which should help simplify things.

I.e. we have:

##a(t) = ## some function of ##a'## and ##v(t)## (the instantaneous speed of the ship)

Where ##a(t) = \frac{dv}{dt}##
 
  • #3
If we assume ##u=v## we end up with
$$a' = \frac{1}{\gamma} \frac{c^2}{(c^2-v^2)} a(t) \Longleftrightarrow a(t)=\frac{d v}{dt}=\frac{c^2-v^2}{c^2}\gamma a' .$$

I'm sorry, but I have absolutely no idea what I'm supposed to do now... For me it looks like we are just manipulating some equations that have vaguely something to do with what I would like to figure out... What are the logical steps here and what am I trying to find in order to obtain ##\tau(t)## and vice versa?

If I had to guess I'd probably try the following: we solve the last equation for ##dt## and integrate then.
$$ \int \frac{c^2}{a'} \sqrt{1-\frac{v^2}{c^2}} dv = \int dt = t.$$
This seems kind of weird, especially since I don't really think there is an analytical solution for the lhs, or at the very least I don't know how to calculate it...

Sorry that I can't contribute here... Could you maybe help me a little bit more?
 
  • #4
I'm not sure what the problem is as this is all standard mathematical physics.

If you find ##v(t)## you have ##\gamma(t)## which relates ##dt## and ##d\tau##.
 
  • #5
Ps check your working. You should have a factor of ##\gamma^3## relating ##a## and ##a'##.
 
  • Like
Likes Markus Kahn
  • #6
Alright, I'll go trough everything again tomorrow. Thanks for the help!
 
  • #7
@PeroK
Alright, so another try. Let ##u(t)## and ##u'(t')## be the velocities of the rocket in the observers and the rest frame of the rocket respectively and let ##v## be the constant velocity between the the two frames. We then have
$$\begin{align*}a'
&= \frac{du'}{dt'} = \frac{dt}{dt'} \frac{du'}{dt} = \frac{dt}{dt'} \frac{d}{dt} \frac{u-v}{1-\frac{uv}{c^2}}.
\end{align*}$$
  • Since ##t' = \gamma(t-\frac{v}{c^2}x)## we have $$\frac{dt}{dt'}=\frac{d}{dt'} \left(\frac{t'}{\gamma} + \frac{v}{c^2}x\right) = \frac{1}{\gamma}$$
  • and here we have with the product rule $$\begin{align*} \frac{d}{dt} \frac{u-v}{1-\frac{uv}{c^2}} &= \frac{u' (1-\frac{vu}{c^2}) - (u-v) (-\frac{u'v}{c^2}) }{(1-\frac{uv}{c^2})^2} =\frac{(1-\frac{vu}{c^2}) + (\frac{uv}{c^2}-\frac{v^2}{c^2}) }{(1-\frac{uv}{c^2})^2}u' \\&= \frac{1-\frac{v^2}{c^2} }{(1-\frac{uv}{c^2})^2}u' =\frac{1}{(1-\frac{uv}{c^2})^2} \frac{u'}{\gamma^2}.\end{align*}$$
So everything together gives
$$a' =\frac{1}{(1-\frac{uv}{c^2})^2} \frac{a}{\gamma^3} $$

The thing that confuses me now is that if we set ##u=v## we will find
$$a' = \frac{a}{\gamma^3} \frac{1}{(1-\frac{v^2}{c^2})^2} = \frac{a}{\gamma^3} \gamma^4 = a\gamma \quad\Longleftrightarrow\quad a =\frac{a'}{ \gamma}.$$
Is this correct? It almost seems to simple to be true...

Assuming this to be correct, we have
$$ a=\frac{dv}{dt} = a'/\gamma \quad \Longleftrightarrow \quad \int_{v_0}^v \sqrt{1-\frac{v^2}{c^2}}dv = a'(t-t_0).$$
The result of this integral is not really nice and doesn't seem to have anything to do with the solution that I'm expecting (the solution presented in my opening post in the links).. So once again, I'm doing something wrong... Can you maybe point me to my mistake?
 
  • #8
Here's the mistake:

Markus Kahn said:
  • Since ##t' = \gamma(t-\frac{v}{c^2}x)## we have $$\frac{dt}{dt'}=\frac{d}{dt'} \left(\frac{t'}{\gamma} + \frac{v}{c^2}x\right) = \frac{1}{\gamma}$$

The fundamental problem there is that you took ##\frac{dx}{dt'} = 0##.

It was simpler just to do:
  • Since ##t' = \gamma(t-\frac{v}{c^2}x)## we have $$\frac{dt'}{dt}=\gamma(1 - \frac{vu}{c^2})$$

Also, it seems better to me to aim for an expression for ##a## in terms of ##a'##. It all comes out the same, of course, but it seemed more logical to me to start with:

##a = \frac{du}{dt} = \dots ##
 
Last edited:
  • #9
Markus Kahn said:
  • and here we have with the product rule $$\begin{align*} \frac{d}{dt} \frac{u-v}{1-\frac{uv}{c^2}} &= \frac{u' (1-\frac{vu}{c^2}) - (u-v) (-\frac{u'v}{c^2}) }{(1-\frac{uv}{c^2})^2} =\frac{(1-\frac{vu}{c^2}) + (\frac{uv}{c^2}-\frac{v^2}{c^2}) }{(1-\frac{uv}{c^2})^2}u' \\&= \frac{1-\frac{v^2}{c^2} }{(1-\frac{uv}{c^2})^2}u' =\frac{1}{(1-\frac{uv}{c^2})^2} \frac{u'}{\gamma^2}.\end{align*}$$
So everything together gives
$$a' =\frac{1}{(1-\frac{uv}{c^2})^2} \frac{a}{\gamma^3} $$

PS all those ##u'## should be ##a'##.
 
  • #10
Here's my working:

##a = \frac{du}{dt} = \frac{du/dt'}{dt/dt'}##

##t = \gamma(t' + vx'/c^2) \ \Rightarrow \ \frac{dt}{dt'} = \gamma(1 + vu'/c^2)##

##\frac{du}{dt'} = \frac{d}{dt'}(\frac{v + u'}{1 + vu'/c^2}) = \frac{a'}{1 + vu'/c^2} - \frac{(v + u')}{(1 + vu'/c^2)^2}(\frac{va'}{c^2}) = \frac{1}{(1 + vu'/c^2)^2}(1 - v^2/c^2)a' = \frac{a'}{\gamma^2(1 + vu'/c^2)^2} ##

Putting this together gives:

##a = \frac{a'}{\gamma^3(1 + vu'/c^2)^3} ##

In this case we set ##u' = 0## to get ##a = \frac{a'}{\gamma^3} ##
 
  • #11
Alright, this took me way longer than it should have, but I think I've got it now... Again, I did a slightly different way ##\frac{du}{dt} = \frac{dt'}{dt}\frac{du}{dt'}## instead of ##\frac{du}{dt} = \frac{du/dt'}{dt/dt'}##, but I arrive at the same result. Thank you for your patience!

But just to make sure that I understand what we are doing here: What we have found now is the acceleration ##a## that an external observer in a reference frame ##S## would measure if the rocket was accelerating in a reference frame ##S'## with constant acceleration ##a'##. Is this correct?

Our goal is now to obtain ##v(t)## right? For this I would need to solve the Differential equation from above.

I don't really know how to solve
$$\frac{dv}{dt} = \frac{a'}{(1-\frac{v^2}{c^2})^3}$$
but by fixing ##v(0)=0## as boundry condition, wolfram alpha gives
$$a c^2 t = \frac{3}{8} c^3 \sin^{-1}(v(t)/c) + \frac{1}{8} v(t) (5 c^2 - 2 v(t)^2) \sqrt{1 - v(t)^2/c^2},$$
which indicates that there is no closed form for ##v(t)##. So how does one proceed to find the solution for this DE?
 
  • #12
Markus Kahn said:
Alright, this took me way longer than it should have, but I think I've got it now... Again, I did a slightly different way ##\frac{du}{dt} = \frac{dt'}{dt}\frac{du}{dt'}## instead of ##\frac{du}{dt} = \frac{du/dt'}{dt/dt'}##, but I arrive at the same result. Thank you for your patience!

That's just the same thing, using ##dt'/dt = \frac{1}{dt/dt'}##

Markus Kahn said:
But just to make sure that I understand what we are doing here: What we have found now is the acceleration ##a## that an external observer in a reference frame ##S## would measure if the rocket was accelerating in a reference frame ##S'## with constant acceleration ##a'##. Is this correct?

It's more general than that. ##a'## does not have to be constant. The formula relates the acceleration (for 1D motion) between reference frames. Note that you can do the same thing for the other components of velocity and acceleration to get a more general acceleration transformation for 3D motion (under a Lorentz boost).

If the particle is instantaneously at rest in S', then we have the simplification using ##u' =0##. Note that these formulas relate instantaneous, time-dependent quantities in general.

The special case we have here is that ##a'## is constant and S' is the instantaneous rest frame of the ship.

Markus Kahn said:
I don't really know how to solve
$$\frac{dv}{dt} = \frac{a'}{(1-\frac{v^2}{c^2})^3}$$
but by fixing ##v(0)=0## as boundry condition, wolfram alpha gives
$$a c^2 t = \frac{3}{8} c^3 \sin^{-1}(v(t)/c) + \frac{1}{8} v(t) (5 c^2 - 2 v(t)^2) \sqrt{1 - v(t)^2/c^2},$$
which indicates that there is no closed form for ##v(t)##. So how does one proceed to find the solution for this DE?

Okay, so there might be a trick! What about looking at ##\frac{d}{dt}({\gamma v})##?

There's a general rule of thumb in SR. If it doesn't work out with velocity, try energy-momentum. In this case the momentum (per unit mass) is ##\gamma v##. So, it's worth trying the time derivative of momentum.
 
Last edited:
  • Like
Likes Markus Kahn
  • #13
Thanks for the hint, but this time I didn't work because I again didn't pay enough attention to the details... The differential equation, with the same boundary condition, is actually
$$\frac{dv}{dt} = {\left(1-\frac{v^2}{c^2}\right)^{3/2}}a'\quad\Longrightarrow \quad \frac{v}{\sqrt{1-\frac{v^2}{c^2}}}= a't.$$

From this we find
$$v(t)= \frac{a' c t}{\sqrt{{a'}^2 t^2+c^2}}\quad \Longrightarrow \sqrt{1-v^2/c^2} = \frac{1}{\sqrt{1+\frac{{a'}^2t^2}{c^2}}}$$
We therefore find
$$\tau(t) = \int \frac{dt}{\sqrt{1+\frac{{a'}^2t^2}{c^2}}} = \frac{c}{a'}\sinh^{-1}\left(\frac{a't}{c}\right).$$

Thank you so much for the help, I really appreciate it! Just out of curiosity, what exactly was your idea with the ##\gamma v##? I tried taking the derivative of it, but in the end I just got a way more complicated expression..
 
  • Like
Likes PeroK
  • #14
Markus Kahn said:
Thank you so much for the help, I really appreciate it! Just out of curiosity, what exactly was your idea with the ##\gamma v##? I tried taking the derivative of it, but in the end I just got a way more complicated expression..

The derivative of ##\gamma## is quite important in SR kinematics. You should get:

##\frac{d}{dt}\gamma = \frac{d}{dt}(1 - v^2/c^2)^{-1/2} = \gamma^3(v/c^2)\frac{dv}{dt} = \gamma^3(v/c^2)a##

If we now include the mass of the object, we have:

##\frac{dp}{dt} = \frac{d}{dt}(\gamma mv) = \gamma^3(mv^2/c^2)a + \gamma ma = \gamma^3 ma (v^2/c^2 + 1/\gamma^2) = \gamma^3 ma##

And that's quite an important result, because if we use the formula for the accelerations above we get:

##\frac{dp}{dt} = ma'##

If we now define the three-force, ##F##, as the rate of change of momentum, then we have:

##F = \frac{dp}{dt} = ma' = F'##

Where ##F'## is measured in the rest frame of the particle.

Also, as ##E = \gamma mc^2##, we have ##\frac{dE}{dt} = \gamma^3(v/c^2)amc^2 = Fv##

And, in fact, this generalises to ##\frac{dE}{dt} = \vec{F}.\vec{v}##

In any case, it's important to remember how to do these derivatives.
 

1. What is acceleration in special relativity?

Acceleration in special relativity refers to the change in velocity of an object over time, taking into account the principles of special relativity. It describes how the velocity of an object changes as it approaches the speed of light, and is dependent on the object's mass and energy.

2. How is acceleration calculated in special relativity?

Acceleration in special relativity can be calculated using the equation a = γ^3 * (dv/dt), where γ is the Lorentz factor and dv/dt is the rate of change of velocity over time. This equation takes into account the time dilation and length contraction effects of special relativity.

3. What is the difference between acceleration in special relativity and classical acceleration?

The main difference between acceleration in special relativity and classical acceleration is that in special relativity, the effects of time dilation and length contraction must be taken into account. This means that the acceleration of an object approaching the speed of light will not follow the same pattern as predicted by classical mechanics.

4. How does acceleration affect time in special relativity?

In special relativity, acceleration can affect time through the principle of time dilation. This means that as an object accelerates, time will appear to pass slower for that object compared to a stationary observer. This effect becomes more pronounced as the object approaches the speed of light.

5. Can acceleration be greater than the speed of light in special relativity?

No, according to the principles of special relativity, the speed of light is the maximum speed possible and cannot be exceeded. This means that the acceleration of an object cannot exceed the speed of light, as it would violate the fundamental laws of physics.

Similar threads

  • Advanced Physics Homework Help
Replies
1
Views
307
  • Advanced Physics Homework Help
Replies
2
Views
1K
  • Advanced Physics Homework Help
Replies
3
Views
387
  • Advanced Physics Homework Help
Replies
7
Views
2K
  • Advanced Physics Homework Help
Replies
2
Views
823
  • Advanced Physics Homework Help
Replies
4
Views
1K
  • Advanced Physics Homework Help
Replies
1
Views
492
  • Advanced Physics Homework Help
Replies
5
Views
1K
  • Advanced Physics Homework Help
Replies
4
Views
1K
Replies
2
Views
1K
Back
Top