This research paper presents a new numerical method for solving Milne's phase-amplitude equations, which are used to represent continuum radial wavefunctions in atomic physics. The authors argue that existing methods for solving these equations are often unstable and highly sensitive to numerical errors, particularly when dealing with fine grids.
The paper begins by discussing the limitations of existing methods, such as the Hamming predictor-corrector and the Kaps-Rentrop method. These methods often suffer from error amplification and require significant grid refinement to maintain accuracy, leading to increased computational cost.
The core of the paper is the presentation of a new explicit numerical method based on a linear third-order equation derived from Milne's equations. This linearization eliminates the coupling to spurious, rapidly varying solutions that plague previous methods, resulting in improved stability and reduced sensitivity to errors.
The proposed method employs a combination of numerical schemes: a standard Numerov scheme for the innermost region, a novel explicit scheme based on the linear third-order equation for the intermediate region, and an adapted version of Bar Shalom et al.'s modified predictor-corrector scheme for the outermost region.
The authors demonstrate the effectiveness of their method through numerical tests comparing it to the method proposed by Bar Shalom et al. The results show that the new method exhibits improved stability and accuracy, particularly for finer grids, without requiring excessive grid refinement.
The paper concludes by highlighting the advantages of the proposed method, emphasizing its potential for efficient and accurate computation of continuum radial wavefunctions in atomic physics applications. The authors suggest that their method could be particularly beneficial in scenarios where a large number of wavefunctions need to be calculated, such as in the description of continuum states in atomic physics.
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by R. Piron, M.... at arxiv.org 11-06-2024
https://arxiv.org/pdf/2411.02621.pdfDeeper Inquiries