  We study a self-interacting scalar field theory coupled to gravity and are
interested in spherically symmetric solutions with a regular origin surrounded
by a horizon. Using the most general spherically symmetric ansatz, we show that
in addition to the known static, oscillating solutions discussed earlier in the
literature there exist new classes of solutions which appear in the strong
field case. For these solutions the spatial sphere shrinks either beyond the
horizon, implying a collapsing universe outside of the cosmological horizon, or
it shrinks already inside of the horizon, implying the existence of a black
hole surrounding the scalar lump in all directions. Crucial for the existence
of all such solutions is the presence of a scalar field potential with a
barrier that satisfies the swampland conjectures.
