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First Law of Entanglement Entropy vs Black Hole Entropy in an Anomalous Theory

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arxiv 1511.03844 v1 pith:JJWEQQMD submitted 2015-11-12 hep-th cond-mat.str-el

classification hep-thcond-mat.str-el
keywords entropyentanglementfirstblackbulkholeholographicaffect
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abstract

In this note we explore the validity of the first law of entanglement entropy in the context of the topologically massive gravity (TMG). We found that the variation of the holographic entanglement entropy under perturbation from the pure AdS background satisfies the first law upon imposing the bulk equations of motion in a given time slice, despite the appearance of instabilities in the bulk for generic gravitationl Chern-Simons coupling $\mu$. The black hole entropy is different from the holographic entanglement entropy in a general boosted frame. This discrepancy however do not affect the entanglement first law.

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  1. Timelike and gravitational anomalous entanglement from the inner horizon

    hep-th 2024-12 conditional novelty 7.0 of 10

    The inner horizon of Rindler AdS3 maps to the inner RT surface, which encodes timelike entanglement entropy and gravitational anomaly corrections to holographic entanglement.

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