Period of a particle in a given potential (ex. from Mechanics Landau Lifshitz))

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SUMMARY

The discussion focuses on determining the period of oscillation for a particle of mass m in a potential field defined by the equation U = U0 tan²(αx). The relevant formula for the period T(E) is T(E) = √(2m) ∫(x1(E) to x2(E)) (dx/√(E - U(x))). The solution involves finding the roots x1(E) and x2(E) of the equation U(x) = E and simplifying the integral through substitutions. The final integral can be computed using the residue theorem, leading to a solvable form.

PREREQUISITES
  • Understanding of classical mechanics, specifically oscillatory motion.
  • Familiarity with integral calculus and techniques for solving definite integrals.
  • Knowledge of potential energy functions and their graphical interpretations.
  • Experience with complex analysis, particularly the residue theorem.
NEXT STEPS
  • Study the derivation of the period of oscillation in various potential fields.
  • Learn advanced integration techniques, including trigonometric substitutions and the residue theorem.
  • Explore the implications of potential energy shapes on particle motion.
  • Review classical mechanics texts, such as "Mechanics" by Landau and Lifshitz, for deeper insights into oscillatory systems.
USEFUL FOR

This discussion is beneficial for physics students, particularly those studying classical mechanics, as well as educators and researchers interested in oscillatory motion and potential energy analysis.

alex.dranoel
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Homework Statement


Determine the period of oscillation, as a function of the energy, when a particle of mass ##m## moves in a field for which the potential energy is
$$ U = U_0 \tan^2\alpha x.$$


Homework Equations


The relevant equation is given by the general formula for the period ##T## of the oscillations:
$$ T(E) = \sqrt{2m} \int_{x_1(E)}^{x_2(E)} \frac{dx}{\sqrt{E-U(x)}}$$
where ##x_1(E)## and ##x_2(E)## are roots of ##U(x)=E##, giving the limit of the motion.


The Attempt at a Solution


This problem is found in Mechanics by Landau and Lifshtiz at $11 in the 3rd edition. It is basically a problem of integration. The first thing I did is to find ##x_2(E)##, which is not complicated:
$$E = U_0 tan^2\alpha x \rightarrow x = \frac{1}{\alpha}\arctan \sqrt{\frac{E}{U_0}}$$
Then given the symmetry of the problem, it is clear that
$$ T(E) = 2\sqrt{2m} \int_{0}^{x_2(E)} \frac{dx}{\sqrt{E-U_0\tan^2\alpha x}}$$
Now I am left with an integral that I didn't manage to compute while the result in the book looks very simple.

Thanks for help
 
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I found the way to compute the integral. Firstly, subsitute ##y=\alpha x## to get ride of the ##\alpha## term and then factorize ##E## under the square root. Then substitute ##\sin z = \frac{U_0}{E}\tan y##. If you do everything correctly you will end up with the definite integral:
$$ \int_0^{\pi/2} \frac{dz}{\frac{U_0}{E} + \sin^2 z}$$
that you can compute by using the residue theorem.

If any of want to try, feel free :)
 

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