Electron in a magnetic field problem

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SUMMARY

The discussion focuses on solving the problem of an electron moving in a magnetic field, specifically analyzing the forces acting on it and comparing its trajectory to that of a proton. The participants clarify that while the accelerations of both particles may be equal, their motions can differ significantly due to initial velocity conditions. Key insights include the necessity of converting time-dependent equations of motion into time-independent trajectory equations using natural parametrization and the chain rule. The final derived equation is a differential equation that describes the motion of both particles under the influence of the magnetic field.

PREREQUISITES
  • Understanding of classical mechanics, specifically Newton's laws of motion.
  • Familiarity with vector calculus, including cross products and derivatives.
  • Knowledge of magnetic forces and Lorentz force law.
  • Ability to apply the chain rule in calculus for parameterization of curves.
NEXT STEPS
  • Study the Lorentz force law and its implications for charged particles in magnetic fields.
  • Learn about natural parametrization of curves in vector calculus.
  • Explore differential equations related to motion in magnetic fields.
  • Investigate the concept of unit tangent vectors and their role in motion analysis.
USEFUL FOR

Students and educators in physics, particularly those focusing on electromagnetism and classical mechanics, as well as anyone interested in the dynamics of charged particles in magnetic fields.

  • #31
voko said:
So what do you get all in all?

$$\frac{d^2\vec r}{ds^2}=\frac{e}{mv}\left(\frac{d\vec r}{ds}\times \vec B\right)$$

I don't see how to interpret the equation I have written above. :(
 
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  • #32
The equation is correct. It is a differential equation of a naturally parametrized curve. You need to find out the condition that the curves corresponding to an electron and a proton are equal.
 
  • #33
voko said:
The equation is correct. It is a differential equation of a naturally parametrized curve. You need to find out the condition that the curves corresponding to an electron and a proton are equal.

Looking at the equation I have obtained, I would say the mv part should be same for both electron and proton, correct?

voko, sorry to ask foolish question but what does "naturally parametrized curve" mean? Can you please pass a link? Many thanks!
 
  • #34
Pranav-Arora said:
Looking at the equation I have obtained, I would say the mv part should be same for both electron and proton, correct?

Yes.

voko, sorry to ask foolish question but what does "naturally parametrized curve" mean? Can you please pass a link? Many thanks!

##s## is a parameter of the curve. If you take any function ##s' = f(s)##, ##s'## is also a parameter of the curve. But there is unique (up to an additive constant) way to parametrize the curve so that ##s## is equal to the length of the curve. This is natural parametrization. The condition on ##s## you have in #1 ensures that. Can you see why?

Also, do you see that ## \frac {d\vec r} {ds} ## is the unit velocity vector, a. k. a. the unit tangent vector?

Do you see that ## \frac {d^2\vec r} {ds^2} ## is the normal acceleration vector?
 
  • #35
voko said:
Yes.

So that gives ##U_p=-5.44 \times 10^{-7}##. Thanks voko! :)

##s## is a parameter of the curve. If you take any function ##s' = f(s)##, ##s'## is also a parameter of the curve. But there is unique (up to an additive constant) way to parametrize the curve so that ##s## is equal to the length of the curve. This is natural parametrization. The condition on ##s## you have in #1 ensures that. Can you see why?

Which condition? :confused:

Also, do you see that ## \frac {d\vec r} {ds} ## is the unit velocity vector, a. k. a. the unit tangent vector?

Do you see that ## \frac {d^2\vec r} {ds^2} ## is the normal acceleration vector?

I don't see any of this. :(

Can you please suggest a book or a link where this is discussed?
 
  • #36
Pranav-Arora said:
Which condition? :confused:

The one in the end: ## s = \int v(t)dt ##.

I don't see any of this. :(

Hmm. You had ##\hat v## for the velocity unit vector. Then you found that it was equal to ##\frac {d\vec r} {ds} ##.

Now, because it is unit vector, its derivative must be orthogonal to it, so it is normal to the curve.

The total velocity vector is $$ \frac {d\vec r} {dt} = v \frac {d \vec r} {ds} $$ so the total acceleration vector is $$ \frac {d^2\vec r} {dt^2} = \frac {dv} {dt} \frac {d \vec r} {ds} + v^2 \frac {d^2 \vec r} {ds^2} $$ The first term here is the tangential acceleration, and the second term is the normal acceleration.

The magnitude of ## \frac {d^2 \vec r} {ds^2} ## is the curvature, and its inverse is the radius of curvature.

Can you please suggest a book or a link where this is discussed?

http://en.wikipedia.org/wiki/Frenet–Serret_formulas
 
  • #37
voko said:
Hmm. You had ##\hat v## for the velocity unit vector. Then you found that it was equal to ##\frac {d\vec r} {ds} ##.

Now, because it is unit vector, its derivative must be orthogonal to it, so it is normal to the curve.

The total velocity vector is $$ \frac {d\vec r} {dt} = v \frac {d \vec r} {ds} $$ so the total acceleration vector is $$ \frac {d^2\vec r} {dt^2} = \frac {dv} {dt} \frac {d \vec r} {ds} + v^2 \frac {d^2 \vec r} {ds^2} $$ The first term here is the tangential acceleration, and the second term is the normal acceleration.

The magnitude of ## \frac {d^2 \vec r} {ds^2} ## is the curvature, and its inverse is the radius of curvature.

Thank you very much voko for the explanations! :)

I am not sure if I fully understand this discussion so I will be looking at the link you have posted and try to learn more about this. Thanks again. :smile:
 
  • #38
Hi Pranav-Arora,

The beginning of the book by Kleppner and Kolenkow has some treatment on this topic.
 

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