Physical Society Colloquium
Holography, Black Holes and Quantum Gravity
Department of Physics McGill University
The holographic correspondence is a powerful tool to study basic questions in
quantum gravity. It tells us that quantum gravity in a region of space-time
is completely equivalent to a simple quantum mechanical theory in one less
dimension. In many cases this correspondence can be made explicit. For example,
the two dimensional Ising model appears to be dual to three dimensional
general relativity with a certain value of the cosmological constant. This
allows us to address basic questions involving the quantum mechanics of
black holes and provides a calculable framework for the computation of the
“wave function of the universe” in quantum cosmology.
Friday, September 11th 2015, 15:30
Ernest Rutherford Physics Building, Keys Auditorium (room 112)
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