English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

Motivated by the recently proposed Kerr/CFT correspondence, we investigatethe holographic dual of the extremal and non-extremal rotating linear dilatonblack hole in Einstein-Maxwell-Dilaton-Axion Gravity. For the case of extremalblack hole, by imposing the appropriate boundary condition at spatial infinityof the near horizon extremal geometry, the Virasoro algebra of conservedcharges associated with the asymptotic symmetry group is obtained. It is shownthat the microscopic entropy of the dual conformal field given by Cardy formulaexactly agrees with Bekenstein-Hawking entropy of extremal black hole. Then, byrewriting the wave equation of massless scalar field with sufficient low energyas the SL(2, R)$_L$$\times$SL(2, R)$_R$ Casimir operator, we find the hiddenconformal symmetry of the non-extremal linear dilaton black hole, which impliesthat the non-extremal rotating linear dilaton black hole is holographicallydual to a two dimensional conformal field theory with the non-zero left andright temperatures. Furthermore, it is shown that the entropy of non-extremalblack hole can be reproduced by using Cardy formula.

Holographic Dual of Linear Dilaton Black Hole in Einstein-Maxwell-Dilaton-Axion Gravity