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The Ryu-Takayanagi(RT) conjecture proposes that the entanglement entropy of a CFT in the large $c$ limit is equivalent to an area of an appropriate minimal surface in the dual bulk. However, there are some cases that RT conjecture predicts the entanglement entropy, which contradict to that of the corresponding CFT. In this paper, we present a refined gravity dual of the entanglement entropy of the large $c$ limit CFT as the sum of all the signed areas of cosmic branes satisfying a refined homologous condition.
Recent work has shown that entanglement and the structure of spacetime are intimately related. One way to investigate this is to begin with an entanglement entropy in a conformal field theory (CFT) and use the AdS/CFT correspondence to calculate the
We study holographic entanglement entropy in Gauss-Bonnet gravity following a global quench. It is known that in dynamical scenarios the entanglement entropy probe penetrates the apparent horizon. The goal of this work is to study how far behind the
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Previously we have studied the Generalized Minimal Massive Gravity (GMMG) in asymptotically $AdS_3$ background, and have shown that the theory is free of negative-energy bulk modes. Also we have shown GMMG avoids the aforementioned bulk-boundary unit
In this work, a canonical method to compute entanglement entropy is proposed. We show that for two-dimensional conformal theories defined in a torus, a choice of moduli space allows the typical entropy operator of the TFD to provide the entanglement