Gravity/CFT correspondence for three dimensional Einstein gravity with a conformal scalar field

  title={Gravity/CFT correspondence for three dimensional Einstein gravity with a conformal scalar field},
  author={Mehrdad Hasanpour and Farhang Loran and Hamid Razaghian},
  journal={Nuclear Physics},

Charged black hole with a scalar hair in (2 + 1) dimensions

We obtain and analyze an exact solution to Einstein-Maxwell-scalar theory in (2+1) dimensions, in which the scalar field couples to gravity in a nonminimal way, and it also couples to itself with the

Einstein-Born-Infeld black holes with a scalar hair in three-dimensions

We present black hole solutions in (2+1)-dimensional Einstein’s theory of gravity coupled with Born–Infeld (BI) nonlinear electrodynamic and a massless self-interacting scalar field. The model has

Three dimensional rotating hairy black holes, asymptotics and thermodynamics

A rotating hairy black hole solution is found in gravity minimally coupled to a self-interacting real scalar field in three spacetime dimensions. Then we discuss analytically the horizon structure

Particle motion in a space-time of a 3D Einstein gravity with torsion

We analyze the motion of both massive and massless particles in a model with space-time of 3D Einstein gravity with torsion. We consider the spinor field and the massless scalar field as the source

Novel Rotating Hairy Black Hole in (2 + 1) Dimensions

We present some novel rotating hairy black hole metric in (2 + 1) dimensions, which is an exact solution to the field equations of the Einstein-scalar-AdS theory with a non-minimal coupling. The

Thermodynamics of a Charged Hairy Black Holein (2+1) Dimensions

In this paper we study thermodynamics, statistics and spectroscopic aspects of a charged black hole with a scalar hair coupled to the gravity in (2+1) dimensions. We obtained effects of the black

Hydrodynamics of a rotating charged black hole in (2+1) dimensions with a scalar charge

In this paper, we consider a rotating charged black hole in three dimensions with a scalar charge and study some hydrodynamical quantities, such as diffusion constant, shear viscosity, and



Central charges in the canonical realization of asymptotic symmetries: An example from three dimensional gravity

It is shown that the global charges of a gauge theory may yield a nontrivial central extension of the asymptotic symmetry algebra already at the classical level. This is done by studying three

Conformally dressed black hole in 2 + 1 dimensions.

  • MartínezZanelli
  • Physics, Mathematics
    Physical review. D, Particles and fields
  • 1996
The Hamiltonian formulation including boundary terms of the Euclidean action, the entropy is found to be $\frac{2}{3}$ of the standard value ($\frac{1}{4} A$), and in agreement with the first law of thermodynamics.

A Stress Tensor for Anti-de Sitter Gravity

Abstract:We propose a procedure for computing the boundary stress tensor associated with a gravitating system in asymptotically anti-de Sitter space. Our definition is free of ambiguities encountered

Applied Conformal Field Theory

These lectures consisted of an elementary introduction to conformal field theory, with some applications to statistical mechanical systems, and fewer to string theory. Contents: 1. Conformal

Surface charge algebra in gauge theories and thermodynamic integrability

Surface charges and their algebra in interacting Lagrangian gauge field theories are constructed out of the underlying linearized theory using techniques from the variational calculus. In the case of

Flat limit of three dimensional asymptotically anti–de Sitter spacetimes

In order to get a better understanding of holographic properties of gravitational theories with a vanishing cosmological constant, we analyze in detail the relation between asymptotically anti-de

Operator Content of Two-Dimensional Conformally Invariant Theories

Three-dimensional N=8 superconformal gravity and its coupling to BLG M2-branes

This paper is concerned with the problem of coupling the N=8 superconformal Bagger-Lambert-Gustavsson (BLG) theory to N=8 conformal supergravity in three dimensions. We start by constructing the

Microscopic formulation of black holes in string theory

Selfdual solutions of (2+1) Einstein gravity with a negative cosmological constant

All the causally regular geometries obtained from (2+1)-anti-de Sitter space by identifications by isometries of the form $P \rightarrow (\exp \pi\xi) P$, where $\xi$ is a self-dual Killing vector of