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On shape dependence of holographic entanglement entropy in AdS4/CFT3

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arxiv 1510.03664 v1 pith:4WD7BED7 submitted 2015-10-13 hep-th cond-mat.str-elgr-qc

On shape dependence of holographic entanglement entropy in AdS4/CFT3

classification hep-th cond-mat.str-elgr-qc
keywords ads4beenfiniteanalyticareabackgroundsdimensionaldomains
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We study the finite term of the holographic entanglement entropy of finite domains with smooth shapes and for four dimensional gravitational backgrounds. Analytic expressions depending on the unit vectors normal to the minimal area surface are obtained for both stationary and time dependent spacetimes. The special cases of AdS4, asymptotically AdS4 black holes, domain wall geometries and Vaidya-AdS backgrounds have been analysed explicitly. When the bulk spacetime is AdS4, the finite term is the Willmore energy of the minimal area surface viewed as a submanifold of the three dimensional flat Euclidean space. For the static spacetimes, some numerical checks involving spatial regions delimited by ellipses and non convex domains have been performed. In the case of AdS4, the infinite wedge has been also considered, recovering the known analytic formula for the coefficient of the logarithmic divergence.

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Cited by 2 Pith papers

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    The quadratic shape-deformation correction to pseudoentropy in dS/CFT is controlled by the analytically continued stress-tensor coefficient C_T, making the sphere a local extremum across Einstein and quadratic-curvatu...

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    Renormalized holographic pseudoentropy in dS/CFT is constructed from conformal-gravity actions in four and six dimensions, yielding finite sphere values and Mezei-like shape dependence for small deformations.