Dimension-adaptive sparse-grid refinement for binary-black-hole initial-data models
Develop a dimension-adaptive, downward-closed Smolyak sparse-grid index set for the differentiable parametric solver of conformally flat Bowen–York binary-black-hole initial data, growing the index set greedily along parameter axes whose hierarchical interpolation surpluses remain large, in order to account for unequal parameter difficulty more efficiently than the isotropic sparse grid.
References
Several directions remain open. First, the cheap computation of the nodal representation currently requires nested point sets. Extending it to non-nested sequences would broaden the method's applicability. Second, the weight strategies of \Cref{subsec:SelectionOfOptimalWeights} rely on knowledge of the smoothness parameters $\sigma_j$. A data-driven or adaptive selection of $$ is desirable in practice. A dimension-adaptive variant, in which the index set is built greedily from error indicators rather than prescribed a priori, could handle functions with unknown anisotropy. Finally, combining the offline phase with $\mathcal{H}$-matrix compression or Samplets would extend the method to non-local kernels at nearly linear cost.
When the parameters differ in difficulty, as the slowly converging spin axes of Sec.~\ref{sec:model:peraxis} do, the isotropic simplex can be replaced by a dimension-adaptive downward-closed index set grown greedily along the axes whose surpluses remain large, a refinement we leave to future work.