A slowly rotating BEC dark matter halo model, with baryonic components from 3.6 micron and R-band photometry, fits 11 of 12 dwarf galaxy rotation curves and yields an ultralight particle mass range of about 10^-17 eV/c^2.
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Slowly rotating Bose-Einstein Condensate confronted with the rotation curves of 12 dwarf galaxies
A slowly rotating BEC dark matter halo model, with baryonic components from 3.6 micron and R-band photometry, fits 11 of 12 dwarf galaxy rotation curves and yields an ultralight particle mass range of about 10^-17 eV/c^2.