We study static massive scalar field condensations in the regular
asymptotically flat reflecting star background. We impose Neumann reflecting
surface boundary conditions for the scalar field. We show that the no hair
theorem holds in the neutral reflecting star background. For charged reflecting
stars, we provide bounds for radii of hairy reflecting stars. Below the lower
bound, there is no regular compact reflecting star and a black hole will form.
Above the upper bound, the scalar field cannot condense around the reflecting
star or no hair theorems exist. And in between the bounds, we obtain scalar
configurations supported by Neumann reflecting stars.Comment: 9 pages, 1 figur