compute_coeffs_discrete

gala.potential.scf.compute_coeffs_discrete(xyz, mass, nmax, lmax, r_s, skip_odd=False, skip_even=False, skip_m=False, compute_var=False)[source]

Compute the expansion coefficients for representing the density distribution of input points as a basis function expansion. The points, xyz, are assumed to be samples from the density distribution.

Computing the coefficients involves computing triple integrals which are computationally expensive. For an example of how to parallelize the computation of the coefficients, see examples/parallel_compute_Anlm.py.

Parameters
xyzarray_like

Samples from the density distribution. Should have shape (n_samples, 3).

massarray_like

Mass of each sample. Should have shape (n_samples,).

nmaxint

Maximum value of n for the radial expansion.

lmaxint

Maximum value of l for the spherical harmonics.

r_snumeric

Scale radius.

skip_oddbool (optional)

Skip the odd terms in the angular portion of the expansion. For example, only take \(l=0, 2, 4, ...\)

skip_evenbool (optional)

Skip the even terms in the angular portion of the expansion. For example, only take \(l=1, 3, 5, ...\)

skip_mbool (optional)

Ignore terms with \(m > 0\).

compute_varbool (optional)

Also compute the variances (and covariances) of the coefficients.

Returns
Snlmndarray

The value of the cosine expansion coefficient.

Tnlmndarray

The value of the sine expansion coefficient.

STcovarndarray, optional

If compute_var==True, this also computes and returns the covariance matrix of the coefficients.