Por Richard Brito (CENTRA, Instituto Superior Técnico).
Ultralight bosonic fields are compelling dark-matter candidates and arise in a variety of beyond-Standard-Model scenarios. These fields can tap energy and angular momentum from spinning black holes (BHs) through superradiant instabilities, forming macroscopic bosonic condensates around astrophysical BHs. The formation of such condensates can lead to several striking signatures, such as the emission of continuous gravitational-wave (GW) signals, lack of highly spinning BH in particular BH mass ranges, modifications to the dynamics of binary BH systems, among others. In this talk I will give an overview of this research program, focusing on the work I have been involved in over the past few years and on recent developments.
Short Bio: Richard Brito is a FCT junior researcher and an invited assistant Professor at CENTRA, Instituto Superior Técnico. His research focuses on black-hole and gravitational-wave physics and he is currently a co-chair of the Fundamental Physics Working Group of the LISA consortium. Previously he was a postdoctoral researcher at the Max Planck Institute for Gravitational Physics and a Marie Curie fellow at the Sapienza University of Rome.
