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SUMMARY:Wheeler DeWitt States of a Charged AdS4 Black Hole - Sirui Ning\, 
 University of Oxford
DTSTART:20231020T120000Z
DTEND:20231020T130000Z
UID:TALK207553@talks.cam.ac.uk
CONTACT:Xi Tong
DESCRIPTION:In  AdS/CFT  radial evolution of bulk fields will give a holog
 raphic renormalization flow of coupling contants. The renormalization flow
  usually starts at the asymptotical boundary as the UV point and ends at h
 orzion 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 in
 to black hole interior with the same equation of motion. In exterior the e
 quation 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 f
 unction and the interior WdW wave function for 4d AdS Schwarzchild black h
 ole. In this talk\, I will extend Hartnoll's formalism to  4d charged Reis
 sner-Nordstrom AdS  black hole. 
LOCATION:Potter room/Zoom
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