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Friday, March 25, 2016
2:00 PM - 3:00 PM
Cahill, Hameetman Auditorium

TAPIR Seminar

Physics near Rapidly Spinning Black Holes
Samuel Gralla, Asst Professor, Dept of Physics, University of Arizona,

When a black hole spins near the maximum rate, its near-horizon region gains additional emergent symmetries and can be thought of as a spacetime in its own right.  I will discuss the dynamics of particles and fields in this region, the constraints imposed by symmetry, and observational consequences.  In particular I will discuss a "smoking gun" gravitational-wave signal of a black hole with near-maximal spin.




For more information, please contact JoAnn Boyd by phone at 4280 or by email at