Basis sets and Coulomb resolutions in rotational coordinates
arXiv:2606.13324 · doi:10.1088/1751-8121/ae6e04
Abstract
Using generalised Laplacian symmetry operators, we construct basis sets or Coulomb resolutions in several separable coordinate systems, including two R-separable systems. This expands the possible geometries in which basis set construction is feasible, a problem which is relevant to both galactic dynamics and computational chemistry. In particular we derive three basis sets (two in prolate spheroidal and one in cylindrical coordinates) which are expressible in closed-form using a single Jacobi polynomial. We also show how any spherical polar or prolate spheroidal basis set may be transformed into a bispherical or toroidal basis set.
arXiv commentAuthor-accepted manuscript; see J. Phys. A for final published version
References in corpus (14)
- A Universal Density Profile from Hierarchical Clustering
- Analytical Models For Galactic Nuclei
- An adaptive algorithm for n-body field expansions
- A Halo Expansion (HEX) Technique for Approximating Simulated Dark Matter Haloes
- Models of Distorted and Evolving Dark Matter Halos
- Galaxy halo expansions: a new biorthogonal family of potential-density pairs
- Potential-Density Basis Sets for Galactic Disks
- New biorthogonal potential--density basis functions
- Resolutions of the Coulomb operator: VI. Computation of auxiliary integrals
- A two-parameter family of double-power-law biorthonormal potential-density expansions
- Efficient Algorithm for Two-Center Coulomb and Exchange Integrals of Electronic Prolate Spheroidal Orbitals
- A general basis set algorithm for galactic haloes and discs
- Two-integral distribution functions for axisymmetric stellar systems with separable densities
- Linear response of rotating and flattened stellar clusters: the oblate Kuzmin-Kutuzov Stäckel family