  We review recent calculations of quasinormal modes and asymptotic tails of
the Bardeen spacetime interpreted as a quantum corrected Schwarzschild-like
black holes. Massless electromagnetic and Dirac fields and massive scalar field
are considered. The first few overtones are much more sensitive to the change
of the quantum correction parameter than the fundamental mode, because such
correction deforms the black hole geometry near the event horizon. While the
asymptotic tails of massless fields are identical to those for the
Schwarzschild case, the tails for a massive field differs from the
Schwarzschild limit at both intermediate and asymptotic times.
