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In a galactic halo like the Milky Way, bosonic dark matter particles lighter than about $30$ eV have a de Broglie wavelength larger than the average inter-particle separation and are therefore well described as a set of classical waves.
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J. Lesgourgues, A. Arbey, and P. Salati, “A light scalar field at the origin of galaxy rotation curves,” New Astron. Rev. 46
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S. Alexander and S. Cormack, “Gravitationally bound BCS state as dark matter,” JCAP 1704
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K. Mukaida, M. Takimoto, and M. Yamada, “On Longevity of I-ball/Oscillon,” JHEP 03
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K. Van Tilburg, A.-M. Taki, and N. Weiner, “Halometry from Astrometry,” JCAP 1807
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T. C. Bachlechner, K. Eckerle, O. Janssen, and M. Kleban, “Axion Landscape Cosmology,” JCAP 1909
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