PIRSA:13090060

Video URL

https://pirsa.org/13090060

Holography without Strings - Joint Quantum Gravity and String Theory Seminar

Marolf, D. (2013). Holography without Strings - Joint Quantum Gravity and String Theory Seminar. Perimeter Institute for Theoretical Physics. https://pirsa.org/13090060

Marolf, Donald. Holography without Strings - Joint Quantum Gravity and String Theory Seminar. Perimeter Institute for Theoretical Physics, Sep. 12, 2013, https://pirsa.org/13090060 

          @misc{ scivideos_PIRSA:13090060,
            doi = {10.48660/13090060},
            url = {https://pirsa.org/13090060},
            author = {Marolf, Donald},
            keywords = {Quantum Gravity},
            language = {en},
            title = {Holography without Strings - Joint Quantum Gravity and String Theory Seminar},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2013},
            month = {sep},
            note = {PIRSA:13090060 see, \url{https://scivideos.org/pirsa/13090060}}
          }

Donald Marolf University of California, Santa Barbara

Talk numberPIRSA:13090060
DOI10.48660/13090060
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

A defining feature of holographic dualities is that, along with the bulk equations of motion, boundary correlators at any given time t determine those of observables deep in the bulk. We argue that this property emerges from the bulk gravitational Gauss law together with bulk quantum entanglement as embodied in the Reeh-Schlieder theorem. Stringy bulk degrees of freedom are not required and play little role even when they exist. As an example we study a toy model whose matter sector is a free scalar field. The energy density (\rho) sources what we call a pseudo-Newtonian potential (\Phi) through Poisson's equation on each constant time surface, but there is no back-reaction on the matter. We show the Hamiltonian to be essentially self-adjoint on the domain generated from the vacuum by acting with boundary observables localized in an arbitrarily small neighborhood of the chosen time t. Since the Gauss law represents the Hamiltonian as a boundary term, the model is holographic in the sense stated above.