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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 2.

Spherically averaged radial-density profiles of the evolved FDM halos. The blue and orange curves correspond to particle masses of mψ = 10−22 eV and mψ = 10−23 eV, respectively. The blue and orange dotted curves show the corresponding best-fitting soliton profiles in the inner halo regions (H.-Y. Schive et al. 2014b). The black dashed and solid curves show the best-fitting NFW profiles for the mψ = 10−22 eV and mψ = 10−23 eV halos, respectively, obtained using only the radial data beyond the effective Einstein radius.

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