Holographic chiral induced W-gravities
arXiv:1412.2510
Abstract
We study boundary conditions for 3-dimensional higher spin gravity that admit asymptotic symmetry algebras expected of 2-dimensional induced higher spin theories in the light cone gauge. For the higher spin theory based on sl(3, R) plus sl(3,R) algebra, our boundary conditions give rise to one copy of classical W3 and a copy of sl(3,R) or su(1,2) Kac-Moody symmetry algebra. We propose that the higher spin theories with these boundary conditions describe appropriate chiral induced W-gravity theories on the boundary. We also consider boundary conditions of spin-3 higher spin gravity that admit u(1) plus u(1) current algebra.
arXiv comment19 pages
References in corpus (13)
- The Black Hole in Three Dimensional Space Time
- Nonlinear W(infinity) Algebra as Asymptotic Symmetry of Three-Dimensional Higher Spin Anti-de Sitter Gravity
- Quantum effective action from the AdS/CFT correspondence
- Black holes in three dimensional higher spin gravity: A review
- New Boundary Conditions for AdS3
- Towards metric-like higher-spin gauge theories in three dimensions
- An sl(2, R) current algebra from AdS_3 gravity
- W Symmetry and Integrability of Higher spin black holes
- Chiral Liouville Gravity
- Boundary Conditions and Partition Functions in Higher Spin AdS/CFT
- The Holographic Ward identity: Examples from 2+1 gravity
- Free boundary conditions and the AdS/CFT correspondence
- Holography and the Polyakov action