Holographic duality for 3d spin-3 gravity coupled to scalar field

From MaRDI portal
Revision as of 06:43, 1 February 2024 by Import240129110113 (talk | contribs) (Created automatically from import240129110113)
(diff) ← Older revision | Latest revision (diff) | Newer revision → (diff)

Publication:1731691

DOI10.1016/J.NUCLPHYSB.2019.02.005zbMATH Open1409.81089arXiv1902.02541OpenAlexW2911757634WikidataQ125574089 ScholiaQ125574089MaRDI QIDQ1731691

Author name not available (Why is that?)

Publication date: 13 March 2019

Published in: (Search for Journal in Brave)

Abstract: The 3d spin-3 gravity theory is holographically dual to a 2d calW3-extended CFT. In a large-c limit the symmetry algebra of the CFT reduces to SU(1,2)imesSU(1,2). On the ground of symmetry the dual bulk space-time will be given by an 8d group manifold SU(1,2). Hence we need to introduce five extra coordinates in addition to three ordinary ones. The 3d space-time is a 3d hyper-surface Sigma embedded at constant values of the extra variables. Operators in the CFT at the boundary of Sigma are expressed in terms of calW descendants of the operators at the boundary of Sigma0, where the extra variables vanish. In this paper it is shown that AdS/CFT correspondence for a scalar field coupled to 3d spin-3 gravity is realized in this auxiliary 8d space. A bulk-to-boundary propagator of a scalar field is found and a generating functional of boundary two-point functions of scalar calW-descendant operators is obtained by using the classical action for the scalar field. Classically, the scalar field must satisfy both Klein-Gordon equation and a third-order differential equation, which are related to the quadratic and cubic Casimir operators of su(1,2). It is found that the coefficient function of the derivatives of the scalar field in the latter equation is the spin-3 gauge field, when restricted to the hypersurface. An action integral in the 8d auxiliary space for the 3d spin-3 gravity coupled to a scalar field is presented. An 8d local frame is introduced and the equations of motion for the 8d connections Amu, overlineAmu are solved. By restricting those solutions onto Sigma, flat connections in 3d SL(3,mathbbR)imesSL(3,mathbbR) Chern-Simons theory are obtained and new 3d black hole solutions with and without spin-3 charge are found by this method.


Full work available at URL: https://arxiv.org/abs/1902.02541




No records found.








This page was built for publication: Holographic duality for 3d spin-3 gravity coupled to scalar field

Report a bug (only for logged in users!)Click here to report a bug for this page (MaRDI item Q1731691)