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Gravitational Lensing Predictions from Wave Simulations of Fuzzy Dark Matter

  • Authors: Jiajun Zhou, Zhengxiang Li, Amruth Alfred, Ran Gao, Jeremy Lim, Zong-Hong Zhu

Jiajun Zhou et al 2026 The Astrophysical Journal Letters 1008 .

  • Provider: AAS Journals

Caption: Figure 3.

Probability distributions of the image-position anomaly A. (a) S–P FDM simulations with mψ = 10−22 eV. (b) GRF-based FDM density realizations constructed on top of the best-fitting NFW model. (c) S–P FDM simulations with mψ = 10−23 eV. The blue and red histograms show the normalized distributions for the two radio sources, radio1 and radio2, respectively, while the solid curves denote the corresponding kernel-density-estimation (KDE) fits. The blue and red vertical dashed lines indicate the position anomalies predicted by the best-fitting smooth NFW model for radio1 and radio2, respectively.

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