Trajectory of a particle in a field (special relativity)

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Homework Help Overview

The discussion revolves around finding the trajectory of a particle in a force field described by the equation F = -α/x², within the context of special relativity. Participants are exploring the implications of relativistic effects on the motion of the particle.

Discussion Character

  • Mixed

Approaches and Questions Raised

  • The original poster attempts to derive the trajectory using force equations and relativistic momentum, leading to a complex differential equation. Some participants question the feasibility of solving for x(t) directly using this method.
  • Alternative approaches are suggested, including the work-energy theorem and conservation of energy, with participants discussing the implications of these methods on the problem.
  • There are discussions about substitutions and transformations to simplify the equations, with varying levels of success reported by participants.

Discussion Status

The conversation is ongoing, with participants offering different perspectives on how to approach the problem. Some guidance has been provided regarding the use of energy conservation and potential energy, but no consensus has been reached on a definitive method to solve for the trajectory.

Contextual Notes

Participants note the complexity introduced by the relativistic gamma factor and the challenges posed by the nature of the differential equations involved. There is also mention of constraints related to homework expectations and the difficulty of obtaining explicit solutions.

Kynio
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Hi, I'm new on this forum and I would like to say hello to everybody!
I have a problem with homework from my "Basics of theoretical phisics" class.

Homework Statement


I have to find a trajectory of a particle in field of force:

F = - \frac{\alpha}{x^2}

Homework Equations



I was said to use:

F = \dot{p} = \frac{dp}{dt} and p=mv\gamma

where \gamma is: \gamma = \frac{1}{\sqrt{1-\frac{v^2}{c^2}}} and m is rest mass.


The Attempt at a Solution



\dot{p} = \frac{dp}{dt}=m \frac{d (v\gamma)}{dt} = m (\dot{v}\gamma + v \dot{\gamma})

\dot{\gamma} = -\frac{1}{2} (1-\frac{v^2}{c^2})^{-3/2} \frac{2v}{c} \dot{v} = \dot{v} \frac{v}{c^2} \gamma^3

\dot{p} = m(\dot{v} \gamma + v \dot{v} \frac{v}{c^2} \gamma^3) = m \dot{v} \gamma (1+ \frac{v^2}{c^2} \gamma^2)= m \dot{v} \gamma^3

v=\dot{x} , m \dot{v} \gamma^3 = m \ddot{x} \gamma^3 = -\frac{\alpha}{x^2}

\ddot{x} x^2 \gamma^3 = -\frac{\alpha}{m}

Now I have a problem with that equation. Any ideas how to solve it and get x(t)?
 
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This is similar to a classical particle in a gravitational field which cannot be solved for x(t). Adding the gamma factor to it doesn't make things prettier. I don't see how you can solve this for x(t). Are you sure you have to use this method?
 
I think you'll want to use the work-energy theorem and conservation of energy instead...

Edit: I suppose since you've come this far with the force method, you may as well continue...just multiply both sides of your equation by \frac{\dot{x}}{c^2x^2} and integrate w.r.t. t. You won't be able to get an solution in the form x(t)=\ldots, but you should be able to get an implicit solution
 
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Since the equation doesn't depend on t explicitly, I used a substitution:
\dot{x}=u(x)
\ddot{x}=\frac{du}{dt}=\frac{du}{dx}\frac{dx}{dt}=u'\dot{x}=u'u

After separating variables and integrating, I've got:

\dot{x}=c\sqrt{1-\frac{c^4m^2x^2}{(\alpha+Dmx)^2} where D is a constant.
I think I cannon do much more, tried to solve this in Mathematica, but got a nightmarish outcome.

I think you'll want to use the work-energy theorem and conservation of energy instead...
I don't really have an idea how to use it. Can you at least tell me how to start?
 
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Kynio said:
After separating variables and integrating, I've got:

\dot{x}=c\sqrt{1-\frac{c^4m^4x^2}{(\alpha+Dmx)^2} where D is a constant.
I think I cannon do much more, tried to solve this in Mathematica, but got a nightmarish outcome.

You've now got a separable 1st order ODE...surely you know how to solve that:wink:EDIT: Shouldn't you have m^2 in the numerator, and not m^4?

I don't really have an idea how to use it. Can you at least tell me how to start?

You'll end up with the same DE as above, but a little quicker. Energy is conserved here, so you have E=\gamma mc^2+U(x) where the total energy E is just some constant, and U(x) is the potential energy of the particle due to the conservative force field

U(x)=-\int \textbf{F}\cdot d\textbf{r}=\alpha\int \frac{dx}{x^2}=-\frac{\alpha}{x}

So,

\gamma=\left(1-\frac{\dot{x}^2}{c^2}\right)^{-2}=\frac{E}{mc^2}-\frac{\alpha}{mc^2 x}

Solve for \dot{x} and you should end up with the same DE you have above.
 
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