The “Little Dark Dot”: Evidence for Self-interacting Dark Matter in the Strong Lens SDSS J0946+1006?

Abstract Previous studies, based on precise modeling of a gravitationally lensing image, have identified what may be an extremely compact, dark perturber in the well-known lensing system SDSS J0946+1006 (the “Jackpot”). Its remarkable compactness challenges the standard cold dark matter paradigm. In this paper, we explore whether such a compact perturber could be explained as a core-collapse halo described by the self-interacting dark matter (SIDM) model. Using the isothermal Jeans method, we compute the density profiles of core-collapse halos across a range of masses. Our comparison with observations indicates that a core-collapse halo has an inner density profile and mass enclosed within 1 kpc that fit the data well, but only if the halo has a total mass of ∼10 11 M ⊙ . While a halo of this mass should host a detectable galaxy, the current observational upper limit on the perturber’s luminosity remains uncertain. Resolving whether or not the data support the presence of a core-collapse SIDM halo therefore requires future deep observations to measure its luminosity.

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Publication Details

Journal
The Astrophysical Journal
Published
2025-11-26
DOI
https://doi.org/10.3847/1538-4357/ae1462
Citations
3
Primary Topic
Galaxies: Formation, Evolution, Phenomena
Type
article
Field-Weighted Citation Impact
3.46

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article

The “Little Dark Dot”: Evidence for Self-interacting Dark Matter in the Strong Lens SDSS J0946+1006?

Qiuhan He, Samuel C. Lange, Andrew Robertson, R. Massey et al.
3 citations
The Astrophysical Journal
Galaxies: Formation, Evolution, Phenomena
3.46
article

The “Little Dark Dot”: Evidence for Self-interacting Dark Matter in the Strong Lens SDSS J0946+1006?

Qiuhan He, Samuel C. Lange, Andrew Robertson, R. Massey, Carlos S. Frenk, J.W Nightingale, Maximilian von Wietersheim-Kramsta, Fangzhou Jiang, Shaun Cole, Xiaoyue Cao, Kaihao Wang, Aristeidis Amvrosiadis, Ran Li, S. Z. Li, Zhonghua Jia, Xianghao Ma
article en
3 citations

Abstract

Abstract Previous studies, based on precise modeling of a gravitationally lensing image, have identified what may be an extremely compact, dark perturber in the well-known lensing system SDSS J0946+1006 (the “Jackpot”). Its remarkable compactness challenges the standard cold dark matter paradigm. In this paper, we explore whether such a compact perturber could be explained as a core-collapse halo described by the self-interacting dark matter (SIDM) model. Using the isothermal Jeans method, we compute the density profiles of core-collapse halos across a range of masses. Our comparison with observations indicates that a core-collapse halo has an inner density profile and mass enclosed within 1 kpc that fit the data well, but only if the halo has a total mass of ∼10 11 M ⊙ . While a halo of this mass should host a detectable galaxy, the current observational upper limit on the perturber’s luminosity remains uncertain. Resolving whether or not the data support the presence of a core-collapse SIDM halo therefore requires future deep observations to measure its luminosity.

The Astrophysical JournalVol. 994(2)
Durham University (GB), Chinese Academy of Sciences (CN), Peking University (CN), Beijing Normal University (CN), Kavli Institute for Theoretical Sciences (CN), Carnegie Observatories (US), National Astronomical Observatories (CN), University of Chinese Academy of Sciences (CN), Newcastle University (GB)
National Natural Science Foundation of China
Openalex Percentile: Top 7%
Galaxies: Formation, Evolution, Phenomena
3.46
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