Baryon-driven growth of solitonic cores in fuzzy dark matter halos
  We present zoom-in simulations of fuzzy dark matter (FDM) halos including
baryons and star-formation with sufficient resolution to follow the formation
and evolution of central solitons. We find that their properties are determined
by the local dark matter velocity dispersion in the combined dark matter-baryon
gravitational potential. This motivates a simple prescription to estimate the
radial density profiles of FDM cores in the presence of baryons. As cores
become more massive and compact if baryons are included, galactic rotation
curve measurements are likely harder to reconcile with FDM.
