摘要
Considerations of a particular limit of the magnetohydrodynamic equations, appropriate for the generation of magnetic field in planetary interiors, lead to a set of constraints involving a certain class of homogeneous polynomials. This set is significantly degenerate owing to an identity satisfied by the polynomial coefficients, which involves linear combinations of simple (2)F(1) Gauss hypergeometric functions. A generalised version of this new identity is proved by appealing to Wilf-Zeilberger theory.
- 出版日期2009-10