Speakers
Alba Grassi
(CERN and Université de Genève)
Daniele Mauri
Massimo Bianchi
Massimo Bianchi
(Universita degli Studi di Roma Tor Vergata)
Description
Although linear perturbations of black hole solutions have been studied in great detail, much less is known about quadratic fluctuations. In this work, we take a step forward in this direction by first analyzing simple toy models — the Inverted Hydrogen Atom in four-dimensional Minkowski spacetime and pure AdS — where we construct closed-form solutions for quadratic perturbations. We then turn to the gravity–scalar sector of an N=2,D=4 supergravity Lagrangian, deriving linear and quadratic quasi-normal mode solutions perturbatively in the black hole mass.
Author
Co-authors
Alba Grassi
(CERN and Université de Genève)
Massimo Bianchi
Massimo Bianchi
(Universita degli Studi di Roma Tor Vergata)