|COOKIES: By using this website you agree that we can place Google Analytics Cookies on your device for performance monitoring.|
Superradiant instabilities in astrophysical systems
If you have a question about this talk, please contact Dr Joan Camps.
Black holes are key players in a wide range of fundamental physics including astrophysics as well as high energy physics. Crucial questions concern their stability properties with potentially important implications for the phase-space of solutions or the understanding of condensates in the vicinity of black holes. Of particular interest is the superradiant or “BH-bomb” like instability of Kerr BHs which arises naturally in aymptotically anti-de Sitter spacetimes or in the presence of massive fields surrounding the BH.
Here, we focus on the latter scenario and present our investigations of massive scalar and vector fields in BH backgrounds. Specifically, we have explored the time evolution of these fields with generic initial configurations in highly spinning BH environments. We have found interesting, non-trivial evolution patterns and have been able to deduce the growth rate of the superradiant instability.
This talk is part of the DAMTP Friday GR Seminar series.
This talk is included in these lists:
Note that ex-directory lists are not shown.
Other listsInteresting talks- 1st try Cancer Metabolism Interest Group Seminars Cambridge Review of International Affairs
Other talksThe Metallicity of Damped Lyα Systems A case of Rasamsonia Argillacea pyelonephritis in a German Shepherd dog Self-organisation of pluripotent cells in the mouse embryo Lessons in innate immunity taught by a virus Statistical Methods for Ambulance Fleet Management The Filtering Distribution For Partially Observed Chaotic Dynamical Systems