Physics:Exact solutions of classical central-force problems

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In the classical central-force problem of classical mechanics, some potential energy functions [math]\displaystyle{ V(r) }[/math] produce motions or orbits that can be expressed in terms of well-known functions, such as the trigonometric functions and elliptic functions. This article describes these functions and the corresponding solutions for the orbits.

General problem

Let [math]\displaystyle{ r = 1/u }[/math]. Then the Binet equation for [math]\displaystyle{ u(\varphi) }[/math] can be solved numerically for nearly any central force [math]\displaystyle{ F(1/u) }[/math]. However, only a handful of forces result in formulae for [math]\displaystyle{ u }[/math] in terms of known functions. The solution for [math]\displaystyle{ \varphi }[/math] can be expressed as an integral over [math]\displaystyle{ u }[/math]

[math]\displaystyle{ \varphi = \varphi_{0} + \frac{L}{\sqrt{2m}} \int ^{u} \frac{du}{\sqrt{E_{\mathrm{tot}} - V(1/u) - \frac{L^{2}u^{2}}{2m}}} }[/math]

A central-force problem is said to be "integrable" if this integration can be solved in terms of known functions.

If the force is a power law, i.e., if [math]\displaystyle{ F(r) = ar^{n} }[/math], then [math]\displaystyle{ u }[/math] can be expressed in terms of circular functions and/or elliptic functions if [math]\displaystyle{ n }[/math] equals 1, -2, -3 (circular functions) and -7, -5, -4, 0, 3, 5, -3/2, -5/2, -1/3, -5/3 and -7/3 (elliptic functions).[1]

If the force is the sum of an inverse quadratic law and a linear term, i.e., if [math]\displaystyle{ F(r) = \frac{a}{r^2} + cr }[/math], the problem also is solved explicitly in terms of Weierstrass elliptic functions.[2]

References

  1. Whittaker, pp. 80–95.
  2. Izzo and Biscani

Bibliography