  Temperature dependent relativistic mean-field (RMF) plus BCS approach has
been used for the first time to investigate the anti-bubble effect of the
temperature and deformation in the light, medium-heavy and superheavy nuclei.
Influence of temperature is studied on density distribution, charge
form-factor, single particle (s.p.) energies, occupancy, deformation and the
depletion fraction (DF). At T $=$ 0, the quenching effect of deformation is
predominant. DF is found usually less in oblate deformation than in prolate. DF
decreases with increasing prolate deformation even though the 2s-orbit is empty
which shows the role of deformation in central depletion apart from the
unoccupancy in s-orbit as is usually believed. As T increases, the occupancy of
s-orbit increases, shell structure melts, the deformation vanishes and the
weakening of central depletion is solely due to the temperature. The bubble
effect is eliminated at T $\approx$ 3$-$5 MeV as indicated by DF and the charge
form factor. The temperature effect is found less prominent in superheavy
bubble nuclei where the role of shell effects is indicated.
