In §22.19(ii) it is noted that Jacobian elliptic functions provide a natural basis of solutions for problems in Newtonian classical dynamics with quartic potentials in canonical form . The Weierstrass function plays a similar role for cubic potentials in canonical form . See, for example, Lawden (1989, Chapter 7) and Whittaker (1964, Chapters 4–6).
Airault et al. (1977) applies the function to an integrable classical many-body problem, and relates the solutions to nonlinear partial differential equations. For applications to soliton solutions of the Korteweg–de Vries (KdV) equation see McKean and Moll (1999, p. 91), Deconinck and Segur (2000), and Walker (1996, §8.1).
Ellipsoidal coordinates may be defined as the three roots of the equation
23.21.1 | |||
where are the corresponding Cartesian coordinates and , , are constants. The Laplacian operator (§1.5(ii)) is given by
23.21.2 | |||
where
23.21.3 | |||
Another form is obtained by identifying , , as lattice roots (§23.3(i)), and setting
23.21.4 | ||||
Then
23.21.5 | |||
See also §29.18(ii).