Vacuum polarization effects on quasinormal modes in electrically charged black hole spacetimes

Understand

We investigate the influence of vacuum polarization of quantum massive fields on the scalar sector of quasinormal modes in spherically symmetric black holes.

• We consider the evolution of a massless scalar field on the spacetime corresponding to a charged semiclassical black hole, consisting of the quantum corrected geometry of a Reissner-Nordstr\"om black hole dressed by a quantum massive scalar field in the large mass limit.
• Using a sixth order WKB approach we find the shift in the quasinormal mode frequencies due to vacuum polarization .