LISA can distinguish waveforms from extreme-mass-ratio inspirals affected by dynamical friction in axion-like gravitational atom halos, probing boson masses 10^{-17} to 10^{-15} eV and decay constants 10^{10} to 3.2e12 GeV for total masses 10^4-10^5 solar masses under NFW-consistent densities.
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Impact of the axion-like self-interactions in gravitational atoms for LISA
LISA can distinguish waveforms from extreme-mass-ratio inspirals affected by dynamical friction in axion-like gravitational atom halos, probing boson masses 10^{-17} to 10^{-15} eV and decay constants 10^{10} to 3.2e12 GeV for total masses 10^4-10^5 solar masses under NFW-consistent densities.