Constructing holographic spacetimes using entanglement renormalization

By Brian Swingle. 2012

238 citations recorded by the source corpus.

We elaborate on our earlier proposal connecting entanglement renormalization and holographic duality in which we argued that a tensor network can be reinterpreted as a kind of skeleton for an emergent holographic space. Here we address the question of the large N limit where on the holographic side the gravity theory becomes classical and a non-fluctuating smooth spacetime description emerges. We show how a number of features of holographic duality in the large N limit emerge naturally from entanglement renormalization, including a classical spacetime generated by entanglement, a sparse spectrum of operator dimensions, and phase transitions in mutual information. We also address questions related to bulk locality below the AdS radius, holographic duals of weakly coupled large N theories, Fermi surfaces in holography, and the holographic interpretation of branching MERA. Some of our considerations are inspired by the idea of quantum expanders which are generalized quantum transformations that add a definite amount of entropy to most states. Since we identify entanglement with geometry, we thus argue that classical spacetime may be built from quantum expanders (or something like them).

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics

View Paper: https://www.semanticscholar.org/paper/bf084262081418ec7e0209b05d8bedb798c29926

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In Astronomy and Astrophysics

  1. R. Myers
  2. T. Takayanagi
  3. Shira Chapman
  4. H. Marrochio
  5. L. Susskind
  6. D. Stanford
  7. V. Hubeny
  8. B. Yoshida

In Nuclear and High Energy Physics

  1. R. Myers
  2. T. Takayanagi
  3. Shira Chapman
  4. H. Marrochio
  5. D. Stanford
  6. L. Susskind
  7. V. Hubeny
  8. J. Maldacena

In Statistical and Nonlinear Physics

  1. R. Myers
  2. T. Takayanagi
  3. Shira Chapman
  4. H. Marrochio
  5. L. Susskind
  6. B. Yoshida
  7. D. Stanford
  8. D. Harlow

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