Horizons, holography and condensed matter

By S. Hartnoll. 2011

176 citations recorded by the source corpus.

The holographic correspondence creates an interface between classical gravitational physics and the dynamics of strongly interacting quantum field theories. This chapter will relate the physics of charged, asymptotically Anti-de Sitter spacetimes to the phenomenology of low temperature critical phases of condensed matter. Common essential features will characterise both the gravitational and field theoretic systems. Firstly, an emergent scaling symmetry at the lowest energy scales appears as an emergent isometry in the interior, `near horizon' regime of the spacetime. Secondly, the field theoretic distinction between fractionalized and mesonic phases appears as the presence or absence of a charge-carrying horizon in the spacetime. A perspective grounded in these two characteristics allows a unified presentation of `holographic superconductors', `electron stars' and `charged dilatonic spacetimes'.

Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/edcd1ffdcce8b10df4aab0177a8c0d2b6cbe8fcf

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In Astronomy and Astrophysics

  1. Blaise Goutéraux
  2. S. Sachdev
  3. Aristomenis Donos
  4. Paolo Pani
  5. Jorge E Santos
  6. R. Brito
  7. V. Cardoso
  8. E. Kiritsis

In Atomic and Molecular Physics, and Optics

  1. Blaise Goutéraux
  2. Aristomenis Donos
  3. S. Sachdev
  4. Jorge E Santos
  5. E. Kiritsis
  6. S. Hartnoll
  7. Paolo Pani
  8. R. Brito

In Nuclear and High Energy Physics

  1. Blaise Goutéraux
  2. Aristomenis Donos
  3. S. Sachdev
  4. S. Hartnoll
  5. E. Kiritsis
  6. Jorge E Santos
  7. Paolo Pani
  8. R. Brito

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