Large N field theories, string theory and gravity

O Aharony, SS Gubser, J Maldacena, H Ooguri, Y Oz - Physics Reports, 2000 - Elsevier
We review the holographic correspondence between field theories and string/M theory,
focusing on the relation between compactifications of string/M theory on Anti-de Sitter …

Microscopic formulation of black holes in string theory

JR David, G Mandal, SR Wadia - Physics Reports, 2002 - Elsevier
In this report we review the microscopic formulation of the five-dimensional black hole of
type IIB string theory in terms of the D1–D5 brane system. The emphasis here is more on the …

Top down approach to topological duality defects

JJ Heckman, M Hübner, E Torres, X Yu, HY Zhang - Physical Review D, 2023 - APS
Topological duality defects arise as codimension one generalized symmetry operators in
quantum field theories (QFTs) with a duality symmetry. Recent investigations have shown …

The path integral of 3D gravity near extremality; or, JT gravity with defects as a matrix integral

H Maxfield, GJ Turiaci - Journal of High Energy Physics, 2021 - Springer
A bstract We propose that a class of new topologies, for which there is no classical solution,
should be included in the path integral of three-dimensional pure gravity, and that their …

Semiclassical 3D gravity as an average of large-c CFTs

J Chandra, S Collier, T Hartman, A Maloney - Journal of High Energy …, 2022 - Springer
A bstract A two-dimensional CFT dual to a semiclassical theory of gravity in three
dimensions must have a large central charge c and a sparse low energy spectrum. This …

Cool horizons for entangled black holes

J Maldacena, L Susskind - Fortschritte der Physik, 2013 - Wiley Online Library
General relativity contains solutions in which two distant black holes are connected through
the interior via a wormhole, or Einstein‐Rosen bridge. These solutions can be interpreted as …

Generalized gravitational entropy

A Lewkowycz, J Maldacena - Journal of High Energy Physics, 2013 - Springer
A bstract We consider classical Euclidean gravity solutions with a boundary. The boundary
contains a non-contractible circle. These solutions can be interpreted as computing the trace …

Time evolution of entanglement entropy from black hole interiors

T Hartman, J Maldacena - Journal of High Energy Physics, 2013 - Springer
A bstract We compute the time-dependent entanglement entropy of a CFT which starts in
relatively simple initial states. The initial states are the thermofield double for thermal states …

Holographic Derivation of Entanglement Entropy from the anti–de Sitter<? format?> Space/Conformal Field Theory Correspondence

S Ryu, T Takayanagi - Physical review letters, 2006 - APS
A holographic derivation of the entanglement entropy in quantum (conformal) field theories
is proposed from anti–de Sitter/conformal field theory (AdS/CFT) correspondence. We argue …

Black hole entropy and soft hair

S Haco, SW Hawking, MJ Perry… - Journal of High Energy …, 2018 - Springer
A bstract A set of infinitesimal Virasoro L⊗ Virasoro R diffeomorphisms are presented which
act non-trivially on the horizon of a generic Kerr black hole with spin J. The covariant phase …