Can the ΛCDM model reproduce MOND-like behavior?

@article{Dai2017CanT,
  title={Can the $\Lambda$CDM model reproduce MOND-like behavior?},
  author={De-Chang Dai and Chun-Yan Lu},
  journal={Physical Review D},
  year={2017},
  volume={96},
  pages={124016}
}
It is usually believed that MOND can describe the galactic rotational curves with only baryonic matter and without any dark matter very well, while the $\Lambda$CDM model is expected to have difficulty in reproducing MOND-like behavior. Here, we use EAGLE's data to learn whether the $\Lambda$CDM model can reproduce MOND-like behavior. EAGLE's simulation result clearly reproduces the MOND-like behavior for $a_b\gtrapprox 10^{-12}\text{m/s}^2$ at $z=0$, although the acceleration constant, $a_0… 

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