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29 Lamé FunctionsLamé Functions

§29.8 Integral Equations

Let w(z) be any solution of (29.2.1) of period 4\!\mathop{K\/}\nolimits\!, w_{2}(z) be a linearly independent solution, and \mathop{\mathscr{W}\/}\nolimits\left\{w,w_{2}\right\} denote their Wronskian. Also let x be defined by

where z,z_{1},z_{2},z_{3} are real, and \mathop{\mathrm{sn}\/}\nolimits, \mathop{\mathrm{cn}\/}\nolimits, \mathop{\mathrm{dn}\/}\nolimits are the Jacobian elliptic functions (§22.2). Then

where \mathop{\mathsf{P}_{{\nu}}\/}\nolimits\!\left(x\right) is the Ferrers function of the first kind (§14.3(i)),

29.8.3\mu=\frac{2\sigma\tau}{\mathop{\mathscr{W}\/}\nolimits\left\{w,w_{2}\right\}},

and \sigma (= \pm 1) and \tau are determined by

For further integral equations see Arscott (1964a), Erdélyi et al. (1955, §15.5.3), Shail (1980), Sleeman (1968a), and Volkmer (1982, 1983, 1984).