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.
Small-scale structure of fuzzy and axion-like dark matter,
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hep-ph 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Current interplanetary range measurements could probe ultralight dark matter at masses around 10^{-15} eV if its solar system density were 10^5 times the local value.
citing papers explorer
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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.
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Precision Solar System Dynamics for Ultralight Dark Matter Search
Current interplanetary range measurements could probe ultralight dark matter at masses around 10^{-15} eV if its solar system density were 10^5 times the local value.