Ultra-faint dwarf galaxies serve as powerful testing grounds for wave dark matter models through dynamical stellar heating. Previous simulation-based work derived a lower bound on …
Strong lensing constraints on FDM
Star formation in FDM model.
A wave Schwarzschild method.
Soliton oscillatino as mode interference.
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Numerical and perturbative computations of the fuzzy dark matter model
We study the gravitational effect of non-self-annihilating dark matter on compact stellar objects. The self-interaction of condensate dark matter can give high accretion rate of …