S E M I N A R IDepartament d'Astronomia i Astrofísica
Universitat de València
Rapidly Rotating Black Holes through Gravitational Collapse
Department of Physics, Rikkyo University, Japó
Seminari del departament d'Astronomia i Astrofísica
Dijous 24 febrer 2011
We all believe that there exist various mass range of black hole in Nature. Some of them are produced through the binary merger of compact objects, while some others through gravitational collapse. Here I will focus on the collapse of a massive object to a massive black hole in order to investigate the properties of the rapidly rotating dynamic black holes. In this talk, I will focus on the new feature we found; the existence of quasi-periodic waves after the black hole ringdown in gravitational waveform. The radiation may be detected in the future space-based detector LISA, which may tell us the environment of the massive object.