Speaker
Nizar Ezroura
Description
Motivated by recent studies of supersymmetric black holes, we revisit the phase diagram of AdS5 black holes, whether BPS or not, with particular emphasis on the role of rotation. We develop BPS thermodynamics systematically and note the differences and similarities with the thermodynamics of more familiar AdS black holes. We also explore the role of rotation in the attractor flow formalism for AdS5 supersymmetric black holes.
Primary author
Co-authors
Dr
Marina David
(University of Michigan)
Prof.
Finn Larsen
(University of Michigan)
Zhihan Liu
(Cambridge University)
Dr
Yangwenxiao Zeng
(University of Michigan)
