A Fast Concentric-disk Contour Integration Method For Microlensing Limb-darkening Effect

arXiv:2607.12483 · astro-ph.EP, astro-ph.GA, astro-ph.IM · Submitted 2026-07-14 · Read on arXiv

Suwei Wang

astro-ph.EP, astro-ph.GA, astro-ph.IM

Submitted: 2026-07-14

Comments: Accepted for publication in The Astronomical Journal. 16 pages, 4 figures

License: http://creativecommons.org/licenses/by/4.0/

The gist: Incorporating limb darkening is a computationally demanding step in contour-integration-based microlensing modeling.

Terminology

Abstract

Incorporating limb darkening is a computationally demanding step in contour-integration-based microlensing modeling. Conventional concentric-ring integration is incompatible with high-order quadrature schemes, limiting efficiency. We develop a new concentric-disk method, which reformulates the limb-darkening integral and enables the application of high-order adaptive quadrature, significantly accelerating the computation. While mainly demonstrated using a linear limb-darkening profile, the method readily extends to more general limb-darkening profiles. As a source effect, it applies to lens systems of any complexity. The method achieves a convergence rate scaling faster than N-4 with the number of uniform-source magnification evaluations N, a significant improvement over the concentric-ring N-2 scaling. For a relative accuracy of 10-6, the concentric-disk approach typically requires only 30% or less of the computational cost of traditional algorithms. This method has been implemented in the binary-lens contour integration code Twinkle, providing an efficient and precise tool for analyzing current and future high-precision microlensing observations.

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