Four-momenta trend as a function of proper time

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I don't know if you see my last question in the previous post.

$$p^2(\tau)=\gamma(0) (qE_y(1-v_x(0))\tau+mv_y(0))$$

If now I integrate this:
$$\frac{dp^0}{d\tau}=\gamma(0) \frac qm E_yp^2$$
$$p^0(\tau)=\gamma(0) \bigg(\frac qm E_yp^2\tau + m\bigg)$$

##p^2## in this case is ##p^2(0)## or ##p^2(\tau)##? If is ##p^2(\tau)##, why for ##p^0-p^1## we used ##p^0(0)-p^1(0)=\gamma m (1-v_x(0))##?
 
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Frostman said:
One question: ##p^0-p^1## are ##p^0(0)-p^1(0)## or ##p^0(\tau)-p^1(\tau)##?
##p^0(\tau)-p^1(\tau)##, of course.
Frostman said:
If now I integrate this:
$$\frac{dp^0}{d\tau}=\gamma(0) \frac qm E_yp^2$$
$$p^0(\tau)=\gamma(0) \bigg(\frac qm E_yp^2\tau + m\bigg)$$
Where does the ##\gamma## come from? And also how do you do that integral?
Frostman said:
##p^2## in this case is ##p^2(0)## or ##p^2(\tau)##? If is ##p^2(\tau)##, why for ##p^0-p^1## we used ##p^0(0)-p^1(0)=\gamma m (1-v_x(0))##?
Again, ##p^2 = p^2(\tau)##. The second question can be answered in different ways, but you should be able to answer it by looking at
$$\frac{d p^0}{d \tau} = \frac{d p^1}{d \tau}$$
 
Hi Frostman

have a look at this, mainly chapter 6 from page 89 on:

http://www.dfm.uninsubria.it/fh/FHpages/Teaching_files/appSR2.pdf

Furthermore, I’ like to carry your attention to the fact that the velocity ##\vec v ## has three components , so what is ##\gamma## ? To which component does it refer ? No, you can’t do that way, the motion of the charged particle isn’t in the ##x## axis direction only.
Just use the law that you have written for ## \frac { dp^{\mu}}{d\tau}## using the Faraday tensor, the last one that takes into account that ##\vec E ## is parallel to ##y## axis and ## \vec B## is parallel to the ##z## axis , and they have the same magnitude.
 
Gaussian97 said:
Where does the ##\gamma## come from? And also how do you do that integral?
##\frac{dp^0}{d\tau}=\gamma \frac qm E_yp^2##

##p^0(\tau)-p^0(0)=\int_{0}^{\tau}d\tau\gamma \frac qm E_yp^2(\tau)##

##p^0(\tau)-p^0(0)=\int_{0}^{\tau}d\tau\gamma \frac qm E_y\gamma(0) (qE_y(1-v_x(0))\tau+mv_y(0))##

I need to solve this right?

Gaussian97 said:
Again, ##p^2 = p^2(\tau)##. The second question can be answered in different ways, but you should be able to answer it by looking at
$$\frac{d p^0}{d \tau} = \frac{d p^1}{d \tau}$$

Yes. I understand this step.
 
Frostman said:
##\frac{dp^0}{d\tau}=\gamma \frac qm E_yp^2##

##p^0(\tau)-p^0(0)=\int_{0}^{\tau}d\tau\gamma \frac qm E_yp^2(\tau)##

##p^0(\tau)-p^0(0)=\int_{0}^{\tau}d\tau\gamma \frac qm E_y\gamma(0) (qE_y(1-v_x(0))\tau+mv_y(0))##

I need to solve this right?
Yes, that's the idea, but you have an extra ##\gamma## factor in ##\frac{dp^0}{d\tau}=\gamma \frac qm E_yp^2## which will complicate the integral. Try to compute ##\frac{dp^0}{d\tau}## again. Once you've done that, the integral becomes quite trivial and the problem is almost done.
 
italicus said:
Hi Frostman

have a look at this, mainly chapter 6 from page 89 on:

http://www.dfm.uninsubria.it/fh/FHpages/Teaching_files/appSR2.pdf

Furthermore, I’ like to carry your attention to the fact that the velocity ##\vec v ## has three components , so what is ##\gamma## ? To which component does it refer ? No, you can’t do that way, the motion of the charged particle isn’t in the ##x## axis direction only.
Just use the law that you have written for ## \frac { dp^{\mu}}{d\tau}## using the Faraday tensor, the last one that takes into account that ##\vec E ## is parallel to ##y## axis and ## \vec B## is parallel to the ##z## axis , and they have the same magnitude.

##\gamma## in this case is ##\frac{1}{\sqrt{1-(v_x(0)^2+v_y(0)^2+v_z(0)^2)}}##
 
Gaussian97 said:
Yes, that's the idea, but you have an extra ##\gamma## factor in ##\frac{dp^0}{d\tau}=\gamma \frac qm E_yp^2## which will complicate the integral. Try to compute ##\frac{dp^0}{d\tau}## again. Once you've done that, the integral becomes quite trivial and the problem is almost done.
Okay, tomorrow I'll try to put it all together.

What I got for ##p^3(\tau)## is it right?
##p^3(\tau) - p^3(0) = 0 \rightarrow p^3(\tau)= \text{cost} = m\gamma v_z(0)##
 
Yes, but again, you should specify ##\gamma(0)##
Frostman said:
##\gamma## in this case is ##\frac{1}{\sqrt{1-(v_x(0)^2+v_y(0)^2+v_z(0)^2)}}##
If this is your definition of ##\gamma##, then it's okay to write ##\gamma## instead of ##\gamma(0)##, but notice that after some time the "relativistic factor" (the one you need to use to compute time dilation, etc...) will no longer be ##\gamma##.
 
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@Frostman

please check the dimensions, because the mass ##m## is already contained in ##\vec p##, so I think there is a dimensional mistake.
Make reference to ##\frac{d\vec p}{dt} =q(\vec E +\vec v\times\vec B)##, then introduce the relativistic ##\vec p## and the Faraday tensor. If you take ##m## out of the derivative in the LHS and divide both members by it , the LHS becomes an acceleration, and the RHS contains q/m.
IMO.
 
Last edited:
italicus said:
@Frostman

please check the dimensions, because the mass ##m## is already contained in ##\vec p##, so I think there is a dimensional mistake.
Make reference to ##\frac{d\vec p}{dt} =q(\vec E +\vec v\times\vec B)##, then introduce the relativistic ##\vec p## and the Faraday tensor. If you take ##m## out of the derivative in the LHS and divide both members by it , the LHS becomes an acceleration, and the RHS contains q/m.
IMO.
Which equation are you referring to?
 
Good morning to both of you, I try to do a little order since between one answer and the other we had to correct some of my misunderstandings.

Let's start with the relation that describes the motion of a particle in an electromagnetic field:
$$\frac{dp^\mu}{d\tau}=qF^{\mu\nu}p_{\nu}=\frac qm F^{\mu\nu}p_\nu$$
Component by component:

##\frac{dp^0}{d\tau}=\frac qm E_yp_2(\tau)##
##\frac{dp^1}{d\tau}=\frac qm B_zp_2(\tau) \equiv \frac{dp^0}{d\tau}##
##\frac{dp^2}{d\tau}=\frac qm (E_yp_0(\tau)-B_zp_1(\tau))=\frac qmE_y (p_0(\tau)-p_1(\tau))##
##\frac{dp^3}{d\tau}=0##

Now, let's look at the first and second equations, due to the fact that ##|E|=|B|## we have:
$$\frac{dp^1}{d\tau}=\frac{dp^0}{d\tau}$$
Integrating:
$$p^0(\tau)-p^0(0)=p^1(\tau)-p^1(0)$$ $$p^0(\tau)-p^1(\tau)=p^0(0)-p^1(0)$$
This allows us first of all to integrate the following component:

$$\int_{p^2(0)}^{p^2(\tau)}dp^2=\int_0^\tau d\tau\frac qmE_y (p_0(\tau)-p_1(\tau))$$
Using the result just obtained:
$$\int_{p^2(0)}^{p^2(\tau)}dp^2=\int_0^\tau d\tau\frac qmE_y (p_0(0)-p_1(0))$$$$p^2(\tau)=\frac qmE_y (p_0(0)-p_1(0))\tau+p^2(0)$$$$p^2(\tau)=\gamma(0)\bigg[\frac qmE_y (m-mv_x(0))\tau+mv_y(0)\bigg]$$
Now we can go to evaluate the first two components of ##p_\nu##:
$$\int_{p^0(0)}^{p^0(\tau)}dp^0=\int_0^\tau d\tau\frac qm E_yp_2(\tau)$$$$\int_{p^0(0)}^{p^0(\tau)}dp^0=\int_0^\tau d\tau\frac qm E_y\gamma(0)\bigg[\frac qmE_y (m-mv_x(0))\tau+mv_y(0)\bigg]$$$$p^0(\tau)=\frac qm E_y\gamma(0)\bigg[\frac qmE_y (m-mv_x(0))\frac{\tau^2}2+mv_y(0)\tau\bigg]+p^0(0)$$$$p^0(\tau)=\frac {q^2}{m^2} E_y^2\gamma(0)(m-mv_x(0))\frac{\tau^2}2+\frac qm E_y\gamma(0)mv_y(0)\tau+\gamma(0)m$$$$p^0(\tau)=\gamma(0)\bigg[\frac {q^2}{m} E_y^2(1-v_x(0))\frac{\tau^2}2+q E_yv_y(0)\tau+m\bigg]$$
Now for ##p^1(\tau)## we can use this relation that we find:
$$p^0(\tau)-p^1(\tau)=p^0(0)-p^1(0)$$ $$p^1(\tau)=p^0(\tau)-p^0(0)+p^1(0)$$$$p^1(\tau)=\gamma(0)\bigg[\frac {q^2}{m} E_y^2(1-v_x(0))\frac{\tau^2}2+q E_yv_y(0)\tau+mv_x(0)\bigg]$$
Dulcis in fundo:
$$\frac{dp^3}{d\tau}=0$$$$\int_{p^3(0)}^{p^3(\tau)}dp^3=0$$$$p^3(\tau)-p^3(0)=0$$$$p^3(\tau)=\gamma(0)mv_z(0)$$
So summing up the various components we have:
$$p^0(\tau)=\gamma(0)\bigg[\frac {q^2}{m} E_y^2(1-v_x(0))\frac{\tau^2}2+q E_yv_y(0)\tau+m\bigg]$$$$p^1(\tau)=\gamma(0)\bigg[\frac {q^2}{m} E_y^2(1-v_x(0))\frac{\tau^2}2+q E_yv_y(0)\tau+mv_x(0)\bigg]$$$$p^2(\tau)=\gamma(0)\bigg[qE_y (1-v_x(0))\tau+mv_y(0)\bigg]$$$$p^3(\tau)=\gamma(0)mv_z(0)$$
I hope everything is correct and did not make any miscalculations, let me know!
 
Yes! This is almost perfect.
Fist a little mistake that is not important:
Frostman said:
Let's start with the relation that describes the motion of a particle in an electromagnetic field:
$$\frac{dp^\mu}{d\tau}=qF^{\mu\nu}p_{\nu}=\frac qm F^{\mu\nu}p_\nu$$
It should be
$$\frac{dp^\mu}{d\tau}=qF^{\mu\nu}u_{\nu}=\frac qm F^{\mu\nu}p_\nu$$
But fortunately, this doesn't affect the rest of the computation.
Unfortunately, there is another mistake that does affect the final result
Frostman said:
$$p^2(\tau)=\gamma(0)\bigg[\frac qmE_y (m-mv_x(0))\tau+mv_y(0)\bigg]$$
Now we can go to evaluate the first two components of ##p_\nu##:
$$\int_{p^0(0)}^{p^0(\tau)}dp^0=\int_0^\tau d\tau\frac qm E_yp_2(\tau)$$$$\int_{p^0(0)}^{p^0(\tau)}dp^0=\int_0^\tau d\tau\frac qm E_y\gamma(0)\bigg[\frac qmE_y (m-mv_x(0))\tau+mv_y(0)\bigg]$$
Notice that you have computed ##p^2(\tau)##, but inside the integral you have ##p_2(\tau)##. What's the relation between these two?
 
Gaussian97 said:
Yes! This is almost perfect.
Fist a little mistake that is not important:

It should be
dpμdτ=qFμνuν=qmFμνpν
But fortunately, this doesn't affect the rest of the computation.
Yep, I just forgot to change the name!
Gaussian97 said:
Unfortunately, there is another mistake that does affect the final result
Notice that you have computed p2(τ), but inside the integral you have p2(τ). What's the relation between these two?
A sign! I forgot to keep in mind that ##p^2(\tau)=-p_2(\tau)##, right?
 
Gaussian97 said:
Yes, and I think, after that everything is ok, unless @italicus wants to add something else that I have missed.
Okay, perfect. I await @italicus! In the meantime, I thank you and sorry for the stupid mistakes that I made yesterday, I was practicing all day and I was destroyed.
 
Gaussian97 said:
No worries, we are here to help!
I just wanted to evidence what @Gaussian97 told in #42. The mass m is part of ##p^{\mu}##.