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Wheeler DeWitt States of a Charged AdS4 Black Hole

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If you have a question about this talk, please contact Xi Tong .

In AdS/CFT radial evolution of bulk fields will give a holographic renormalization flow of coupling contants. The renormalization flow usually starts at the asymptotical boundary as the UV point and ends at horzion as the IR point. However, in 2004.01192, Hartnoll found that the radial evolution does not stop at the horizon and can continue to flow into black hole interior with the same equation of motion. In exterior the equation of motion defines a partition function and at interior it defines a WdW wave function. In 2208.04348 Hartnoll gave a unified description in the language of Hamiltonian Jacobi equation of both the exterior partion function and the interior WdW wave function for 4d AdS Schwarzchild black hole. In this talk, I will extend Hartnoll’s formalism to 4d charged Reissner-Nordstrom AdS black hole.

This talk is part of the DAMTP Friday GR Seminar series.

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