Axion-like dark matter search with space-based gravitational wave detectors

Abstract We propose a novel modification to the optical benches of space-based gravitational wave detectors (SGWDs) to enable the detection of axion-like dark matter (ALDM)-induced birefringence without altering the polarization of inter-spacecraft laser links. Our design introduces an auxiliary interferometer to convert polarization modulation into measurable phase shifts. Analytical expressions for sensitivity to the ALDM-photon coupling are derived for various time-delay interferometry (TDI) combinations. Projected sensitivity curves demonstrate complementary coverage across the ALDM mass range 10 -19 ∼ 10 -14 eV. This approach preserves the original interferometric stability while enabling new physics capabilities for SGWDs.

Authors

Publication Details

Journal
Journal of Cosmology and Astroparticle Physics
Published
2026-04-01
DOI
https://doi.org/10.1088/1475-7516/2026/04/082
Citations
1
Primary Topic
Dark Matter and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
18.47

Funders

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article

Axion-like dark matter search with space-based gravitational wave detectors

Run-Min Yao, Xiao-Jun Bi, Qing-Guo Huang, Peng‐Fei Yin
1 citations
Journal of Cosmology and Astroparticle Physics
Dark Matter and Cosmic Phenomena
18.47
article

Axion-like dark matter search with space-based gravitational wave detectors

Run-Min Yao, Xiao-Jun Bi, Qing-Guo Huang, Peng‐Fei Yin
article en
1 citations

Abstract

Abstract We propose a novel modification to the optical benches of space-based gravitational wave detectors (SGWDs) to enable the detection of axion-like dark matter (ALDM)-induced birefringence without altering the polarization of inter-spacecraft laser links. Our design introduces an auxiliary interferometer to convert polarization modulation into measurable phase shifts. Analytical expressions for sensitivity to the ALDM-photon coupling are derived for various time-delay interferometry (TDI) combinations. Projected sensitivity curves demonstrate complementary coverage across the ALDM mass range 10 -19 ∼ 10 -14 eV. This approach preserves the original interferometric stability while enabling new physics capabilities for SGWDs.

Journal of Cosmology and Astroparticle PhysicsVol. 2026(04)
National Natural Science Foundation of China, National Key Research and Development Program of China
Openalex Percentile: Top 4%
Dark Matter and Cosmic Phenomena
18.47
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