Speaker
Alexandru Dima
(Sapienza University of Rome)
Description
We present results on the linear response of four dimensional magnetic black holes and regular topological stars arising from dimensional compactification of Einstein-Maxwell theory in five dimensions.
We discuss the stability of these solutions under both radial and nonradial perturbations, both in the frequency and in the time domain.
Primary author
Alexandru Dima
(Sapienza University of Rome)
Co-authors
Marco Melis
(Sapienza University of Rome)
Paolo Pani
(Sapienza University of Rome)
