Find Relativistic Momentum Equation for a Moving Reference Frame?

In summary, the relativistic momentum equation for a moving reference frame can be derived by considering the relationship between momentum, velocity, and the Lorentz factor. The relativistic momentum \( p \) is expressed as \( p = \gamma m v \), where \( \gamma = \frac{1}{\sqrt{1 - \frac{v^2}{c^2}}} \) is the Lorentz factor, \( m \) is the rest mass, and \( v \) is the velocity of the object. This equation accounts for the effects of relativity as the object's speed approaches the speed of light \( c \), demonstrating that momentum increases significantly at high velocities compared to classical mechanics.
  • #1
Ascendant0
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Homework Statement
Suppose that a mass ##m## has momentum ##p## and energy ##E##, as measured in a frame ##S##. Use the relations ## p = m(dr)/(dt_0) ## and ##E = mc^2(dt)/(dt_0)## and the known transformation of dr and dt to find the values of ##p'## and ##E'## as measured in a second frame ##S'## traveling with speed ##v## along ##O_x##
Relevant Equations
Lorentz Transformation for velocity: ##u_x' = (u_x-v)/(1-(u_xv/c^2) ##
Possibly time? ##t = \gamma t_0##
I figured since ## dr/dt ## is simply the velocity of the target mass, the velocity ##u_x## would simply have to be changed by the Lorentz transformation. Since the rest mass doesn't change, I think this should be as simple as taking the Lorentz transformation for velocity, and substituting the equation for ##u_x'## listed in the "relevant equations" section above, and multiply that by ##m## to get ##mu' = p' ##, so:

##p' = \gamma mu_x' = \gamma m(u_x-v)/(1-(u_xv/c^2) ##

But, I can't find anything online about a conversion like this for some reason, and I'm not all that confident it would be that simple, but I'm not sure how else to look at this other than the velocity should be converted via the Lorentz transformation.

As far as ##E'##, I'm not sure how to do that one. I don't see how I would add in some sort of Lorentz transformation into it in order to take into consideration the new velocity, unless I were to include it in the ##\gamma##
 
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  • #2
I suspect the problem is to find ##E', p'## in terms of ##E, p##. I assume that ##t_0## is the proper time of the particle.
 
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  • #3
PeroK said:
I suspect the problem is to find ##E', p'## in terms of ##E, p##. I assume that ##t_0## is the proper time of the particle.
Yes, that's all correct. The problem tells us to use the two relations there, $$p = m(dr)/(dt_0) $$
and $$ E = mc^2 (dt)/(dt_0) $$to find them. So going by that, that is what led me to the equation above for ##p'##, but again, I'm not all that confident in that answer.

And I don't know how to go about solving for ##E'##, so I'm lost on this one. I know the ##mc^2## won't change, since mass is not changing, and of course the constant ##c## isn't going to change. But, if I were to change the equation to ## t## instead of ##t_0## in that equation to convert to ##E'##, I'd just end up changing it to ## E =\gamma mc^2 ##, but then I don't know what ##v ## would be to take into consideration both the ##v## of ##S'##, as well as the ##v_0## in the momentum of the mass relative to the original frame. I feel like I'm not fully wrapping my brain around all the relations here in various frames
 
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  • #4
Why not differentiate the Lorentz Transformations for the time and position of the particle with respect to its proper time?
 
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  • #5
PeroK said:
Why not differentiate the Lorentz Transformations for the time and position of the particle with respect to its proper time?
Thank you. I did this earlier today after class, but I wanted to post on here, because I'm not confident I simplified it enough, but not sure how else to simplify it

So, I took ## p_x' = m(dr_x') = m \gamma (dx - vdt)/(dt_0) = \gamma p_x - \gamma mv(dt)/(dt_0) ##

To finish with: ##p_x' = \gamma [p_x - mv (dt)/(dt_0) ]##

I don't see any way to simplify it further, as the ##mv## is relativistic, so I can't break that down to ##p##. I don't like leaving it with the ##(dt)/(dt_0) ## though, but is there anything else I can do to make this simpler?

Additionally, I get where the ## \gamma p_x ## comes from in the first part, that makes complete sense to me. But, I'm not sure where the second part of the equation comes from? I would think it would have to do with the energy ##E##, but I don't see any way to change what I see there into ##E##?
 
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  • #6
Ascendant0 said:
I don't see any way to change what I see there into ##E##?
Ascendant0 said:
Homework Statement: … Use the relations ## p = m(dr)/(dt_0) ## and ##E = mc^2(dt)/(dt_0)##
 
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  • #7
Omg, I can't believe I missed that. Thank you.

I finished the rest of my homework problems, and I'm trying to finish up the second part, finding the equation for ##E'##. I believe it might be simpler than I originally thought...

Since ##(dt)/(dt_0) = \gamma##, I can just take the ## E = \gamma mc^2 ## and take the derivative of that with respect to v (from ##\gamma##), right?

With that, I'm getting:

##E' = -mc^2/((1-v^2/{c^2})^{3/2}) ##

The only thing that's throwing me off there is the negative sign I get from the derivative, but I'm thinking I would just make it positive since it will of course be a positive energy ##E##?
 
  • #8
Ascendant0 said:
Omg, I can't believe I missed that. Thank you.

I finished the rest of my homework problems, and I'm trying to finish up the second part, finding the equation for ##E'##. I believe it might be simpler than I originally thought...

Since ##(dt)/(dt_0) = \gamma##, I can just take the ## E = \gamma mc^2 ## and take the derivative of that with respect to v (from ##\gamma##), right?
No. Why do you think differentiating ##E## with respect to ##v## would give you the energy measured in ##S'##? You want to use the same approach you did for ##p'##.

Ascendant0 said:
The only thing that's throwing me off there is the negative sign I get from the derivative, but I'm thinking I would just make it positive since it will of course be a positive energy ##E##?
You can't erase a sign just because it's inconvenient. A wrong sign is typically an indication you made a mistake which you should find and correct.
 
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  • #9
vela said:
No. Why do you think differentiating ##E## with respect to ##v## would give you the energy measured in ##S'##? You want to use the same approach you did for ##p'##.


You can't erase a sign just because it's inconvenient. A wrong sign is typically an indication you made a mistake which you should find and correct.
I figured it was wrong, but I'm struggling, and people complain on here if they feel you aren't making an effort, which I am, I'm just stuck on this one.

With ##p##, I saw how the ##m(dr'/dt_0)## could be used, but with energy, I'm not seeing any derivative I could use for energy. Any derivative I have on my formulas sheet relating to energy is also the derivative of E, like ##dE = (dp)/(dt) udt##, which obviously wouldn't do me any good and isn't even one of the equations included here.

If I took ##E = mc^2(dt)/(dt_0) ## and changed ##dt## to ##dt'##, then it's basically going to be ##t' = t/\gamma##, along with ## 1/t_0 = \gamma/t##, and they'd just cancel out, which of course doesn't do me any good (unless they don't cancel out and there's a difference between the two that I'm not seeing). But anything I manipulate with the equations they gave, I can't see a way to take a derivative that would give me ##E'##

Based off the other equations, I know it's going to look something like:

##E' = \gamma(E - [something])##, just no clue what the [something] is, nor how to derive the equation
 
  • #10
What are the Lorentz transformation equations you have?
 
  • #11
vela said:
What are the Lorentz transformation equations you have?
The ones for position:

##x' = \gamma (x - vt)## and the inverse

Velocity:

##u'= (u_x-v)/(1-(u_xv/c^2) ## and the inverse

... and I actually think I found it just now. I kept looking at ## t = \gamma t'##, which I had grouped with the aforementioned, and I forgot on the back of my reference sheet, I have:

## t' = \gamma (t-vx/c^2) ##

Ok, I know what to do now. I have to redo my formula sheet so I can include that near the other ones. Our professor didn't cover it until the day after the other ones (only gave us the ##t = \gamma t'## with the other transformations the first day), so I didn't have it grouped with them.

I'm not 100% on it, but I think I know the right direction now. I'm going to try to work this out real quick now before I head to bed.
 
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  • #12
vela said:
What are the Lorentz transformation equations you have?
So I believe it's:

## E' = \gamma^2mc^2(dt-dv(x)/(c^2)) ##, and then just simplify this as I'm able, right?
 
  • #13
Ascendant0 said:
So I believe it's:

## E' = \gamma^2mc^2(dt-dv(x)/(c^2)) ##, and then just simplify this as I'm able, right?
If you check the units, you should notice the righthand side has the wrong units, so it can't be correct. It's better if you show your work instead of just posting a result and asking if it's right.
 
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  • #14
vela said:
If you check the units, you should notice the righthand side has the wrong units, so it can't be correct. It's better if you show your work instead of just posting a result and asking if it's right.
Thank you for pointing that out. I finally came back to finish this since it's due tomorrow. I think I have it now

So, I took ## E = mc^2 (dt)/(dt_0) ## and ## t' = \gamma (t' - vx'/(c^2) ##, then:

##E' = mc^2 (dt')/(dt_0) = mc^2 \gamma ((dt)/(dt_0) - (v/c^2) (dx/dt_0) = \gamma (E - vp) ##

So ## E' = \gamma (E - vp) ##

That seems right looking at the other equations, and it is also consistent units-wise. I had expected it to be " ## \gamma (E - [something]) ##", and it being ## vp ## make sense

Thank you for pointing out the units (and all your previous help of course). That's something that I have to remember to check on things like this
 
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FAQ: Find Relativistic Momentum Equation for a Moving Reference Frame?

What is relativistic momentum?

Relativistic momentum is the momentum of an object moving at a significant fraction of the speed of light. It accounts for the effects of special relativity, which states that as an object's velocity approaches the speed of light, its momentum increases without bound. The formula for relativistic momentum is given by p = γmv, where p is momentum, m is the rest mass, v is the velocity of the object, and γ (gamma) is the Lorentz factor, defined as γ = 1 / √(1 - v²/c²), with c being the speed of light.

How do you derive the relativistic momentum equation?

To derive the relativistic momentum equation, start with the classical momentum formula, p = mv. In special relativity, as an object's speed approaches the speed of light, time dilation and length contraction occur. The Lorentz factor γ modifies the mass term, leading to the equation p = γmv. This derivation involves considering the conservation of momentum in collisions and applying the principles of special relativity.

What is the significance of the Lorentz factor in the momentum equation?

The Lorentz factor (γ) is crucial in the relativistic momentum equation because it accounts for the relativistic effects that occur at high velocities. As an object's speed increases, γ increases, which means that the momentum p increases more rapidly than it would in classical physics. This adjustment ensures that momentum remains conserved in relativistic collisions and interactions, and it reflects the increased energy required to accelerate an object as it approaches the speed of light.

How does relativistic momentum differ from classical momentum?

Relativistic momentum differs from classical momentum in that it incorporates the effects of special relativity. In classical mechanics, momentum is simply p = mv, which does not account for changes in mass with speed. In contrast, relativistic momentum uses the equation p = γmv, which includes the Lorentz factor γ that increases as velocity approaches the speed of light. This means that relativistic momentum can become significantly larger than classical momentum for high-speed objects, ensuring that conservation laws hold true in relativistic contexts.

Can you give an example of using the relativistic momentum equation?

Certainly! Let's consider an object with a rest mass of 1 kg moving at a speed of 0.8c (where c is the speed of light). First, calculate the Lorentz factor γ: γ = 1 / √(1 - (0.8c)²/c²) = 1 / √(1 - 0.64) = 1 / √0.36 = 1 / 0.6 = 5/3. Now, using the relativistic momentum equation p = γmv, we have p = (

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