Symmetries of holographic minimal models
By M. Gaberdiel, Thomas Hartman. 2011
321 citations recorded by the source corpus.
It was recently proposed that a large N limit of a family of minimal model CFTs is dual to a certain higher spin gravity theory in AdS3, where the ’t Hooft coupling constant of the CFT is related to a deformation parameter of the higher spin algebra. We identify the asymptotic symmetry algebra of the higher spin theory for generic ’t Hooft parameter, and show that it coincides with a family of $ \mathcal{W} $-algebras previously discovered in the context of the KP hierarchy. We furthermore demonstrate that this family of $ \mathcal{W} $-algebras controls the representation theory of the minimal model CFTs in the ’t Hooft limit. This provides a non-trivial consistency check of the proposal and explains part of the underlying mechanism.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics
View Paper: https://www.semanticscholar.org/paper/f2c1d976b2ed15ede4681d1bd374e28da12b1b73
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Astronomy and Astrophysics
In Nuclear and High Energy Physics
- M. Gaberdiel
- Rajesh Gopakumar
- Eric Perlmutter
- Per Kraus
- S. Giombi
- Thomas Hartman
- M. Gutperle
- M. Ammon
In Statistical and Nonlinear Physics
- M. Gaberdiel
- Rajesh Gopakumar
- Eric Perlmutter
- Per Kraus
- M. Ammon
- M. Gutperle
- Thomas Hartman
- Ashoke Sen
Citations in the corpus
- Towards integrability for AdS 3 / CFT 2 ?> (2014, background): “This provided a new approach to holograpic dualities, and lead to rapid developments [269–272]—see also ref.”
- Towards metric-like higher spin gauge theories in three dimensions (2012, methodology): “It thus preserves the same amount of gauge symmetry as the sum of the linearized Einstein–Hilbert and Fronsdal actions.”
- Thermodynamics of higher spin black holes in 3D (2012, background): “Spurred on by these developments another concrete proposal by Gaberdiel and Gopakumar [28] posits a duality between three dimensional higher spin theories and a WN minimal model CFT in a ’t Hooft-like large-N limit [29, 30, 31, 32].”
- Higher spin AdS3 supergravity and its dual CFT (2011, methodology): “The theory is described by the 3d Chern-Simons theory based on two copies of sl(N) [7], and the asymptotic symmetry near the boundary is found to be the WN algebra [8, 9, 10, 11].”
- Higher spin black holes from CFT (2012, background): “In the large N limit, the detailed microscopics of this proposal are supported by symmetries [14], the spectrum of primaries [15], and certain correlation functions [16, 17, 18, 19, 20]; at finite N some new ingredients may be required in the bulk (or perhaps can be found within the Vasiliev theory ”
- Partition functions of higher spin black holes and their CFT duals (2011, methodology): “The spacetime interpretation and asymptotic symmetries of the SL(3,R) × SL(3,R) Chern-Simons theory were treated in detail in [29], following which [17,18] discovered smooth, asymptotically AdS3, black hole solutions with nonzero spin-3 charge and consistent thermodynamics.”
- Partition functions of holographic minimal models (2011, methodology): “The bulk asymptotic symmetries form (two copies of) a larger algebra W∞[λ] that extends hs[λ] much like the Virasoro algebra extends sl(2) [16, 17, 22].”
- Triality in minimal model holography (2012, methodology): “The particular cases studied in [3, 4] actually belong to a one-parameter family of higher spin theories whose symmetry algebras could be identified with W∞[μ] [5] (see also [6]).”
- How higher-spin gravity surpasses the spin-two barrier (2010, unknown): “[142, 143, 144, 145, 146, 147, 148, 149, 150, 151, 152] and references therein.”
- Asymptotically flat spacetimes in three-dimensional higher spin gravity (2013, background): “The asymptotically AdS3 conditions of [14, 15, 23, 24], that extend the ones of Brown and Henneaux to the case of higher spin fields, have been shown to possess an interesting vanishing cosmological constant limit.”
- Black holes and singularity resolution in higher spin gravity (2011, background): “A full discussion of this prescription can be found in [34, 35, 36], and its implementation in higher spin theories in [37, 23, 38, 33].”
- Higher spin black holes (2011, background): “Introduction Theories of gravity coupled to massless higher spin fields [1,2,3,4,5] have received increased attention in recent years due to their appearance within the AdS/CFT correspondence [6,7,8,9,10,11,12,13,14,15,16,17,18,19,20,21].”
- Conical defects in higher spin theories (2011, methodology): “The analysis in [11, 12] showed that in the ’t Hooft limit the spectrum of the WN minimal model instead falls into representations of W∞[λ], and hence the gauge group in the bulk is its wedge algebra, hs[λ].”
- Higher spins & strings (2014, background): “We believe the AdS3/CFT2 case is particularly suited for this endeavour, because, unlike in higher dimensions, the higher spin symmetry group is enlarged here to aW∞ algebra [21, 22, 23] (generalising the enhancement to Virasoro discovered by Brown and Henneaux [24]).”
- Bounding the space of holographic CFTs with chaos (2016, methodology): “This is the asymptotic symmetry algebra of hs[λ] Chern-Simons theory in AdS3, which also forms the gauge sector of 3D Vasiliev theory [39,40].”
- Spacetime geometry in higher spin gravity (2011, background): “This conjecture has been investigated further in [34,35,36,37].”