An analytic relation between tidal radius, gravitational Bohr radius, and axion de Broglie wavelength yields a mass estimator for intermediate ultralight axions of order 10^{-19} eV from observed stellar stream widths.
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Wave-Tide Locking in Thin Stellar Streams: A Phenomenological Mass Spectrometer for an Intermediate Ultralight Axion
An analytic relation between tidal radius, gravitational Bohr radius, and axion de Broglie wavelength yields a mass estimator for intermediate ultralight axions of order 10^{-19} eV from observed stellar stream widths.