Acquiring the Lefschetz thimbles: efficient evaluation of the diffraction integral for lensing in wave optics

ABSTRACT Evaluating the Kirchhoff–Fresnel diffraction integral is essential in studying wave effects in astrophysical lensing, but is often intractable because of the highly oscillatory integrand. A recent breakthrough was made by exploiting the Picard–Lefschetz theory: the integral can be performed along the ‘Lefschetz thimbles’ in the complex domain where the integrand is not oscillatory but rapidly converging. The application of this method, however, has been limited by both the unfamiliar concepts involved and the low numerical efficiency of the method used to find the Lefschetz thimbles. In this paper, we give simple examples of the Lefschetz thimbles and define the ‘flow lines’ that facilitate the understanding of the concepts. Based on this, we propose new ways to obtain the Lefschetz thimbles with high numerical efficiency, which provide an effective tool for studying wave effects in astrophysical lensing.

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Publication Details

Journal
Monthly Notices of the Royal Astronomical Society
Published
2024-09-12
DOI
https://doi.org/10.1093/mnras/stae2127
Citations
4
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
1.33

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article

Acquiring the Lefschetz thimbles: efficient evaluation of the diffraction integral for lensing in wave optics

Xun Shi
4 citations
Monthly Notices of the Royal Astronomical Society
Pulsars and Gravitational Waves Research
1.33
article

Acquiring the Lefschetz thimbles: efficient evaluation of the diffraction integral for lensing in wave optics

Xun Shi
article en
4 citations

Abstract

ABSTRACT Evaluating the Kirchhoff–Fresnel diffraction integral is essential in studying wave effects in astrophysical lensing, but is often intractable because of the highly oscillatory integrand. A recent breakthrough was made by exploiting the Picard–Lefschetz theory: the integral can be performed along the ‘Lefschetz thimbles’ in the complex domain where the integrand is not oscillatory but rapidly converging. The application of this method, however, has been limited by both the unfamiliar concepts involved and the low numerical efficiency of the method used to find the Lefschetz thimbles. In this paper, we give simple examples of the Lefschetz thimbles and define the ‘flow lines’ that facilitate the understanding of the concepts. Based on this, we propose new ways to obtain the Lefschetz thimbles with high numerical efficiency, which provide an effective tool for studying wave effects in astrophysical lensing.

Monthly Notices of the Royal Astronomical SocietyVol. 534(2)
Yunnan University (CN)
National Natural Science Foundation of China
Openalex Percentile: Top 20%
Pulsars and Gravitational Waves Research
1.33
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