  Static oscillating bounces in Schwarzschild de Sitter spacetime are
investigated. The oscillating bounce with many oscillations gives a super-thick
bubble wall, for which the total vacuum energy increases while the mass of the
black hole decreases due to the conservation of Arnowitt-Deser-Misner (ADM)
mass. We show that the transition rate of such an "up-tunneling" consuming the
seed black hole is higher than that of the Hawking-Moss transition. The
correspondence of analyses in the static and global coordinates in the
Euclidean de Sitter space is also investigated.
