Holography without strings?
arXiv:1308.1977 · doi:10.1088/0264-9381/31/1/015008
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 (ρ) sources what we call a pseudo-Newtonian potential (Φ) 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.
13 pages
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- Gauge-invariant observables, gravitational dressings, and holography in AdS
- Universal horizons in maximally symmetric spaces
- Gauge-invariant observables in gravity and electromagnetism: black hole backgrounds and null dressings
- On the questions of asymptotic recoverability of information and subsystems in quantum gravity
- Holography and unitarity
- A "black hole theorem," and its implications
- Perturbative quantum evolution of the gravitational state and dressing in general backgrounds
- Quantum Channels in Quantum Gravity