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Gravity Edges Modes and Hayward Term

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arxiv 1912.01636 v2 pith:4EGYUDAE submitted 2019-12-03 hep-th gr-qc

classification hep-thgr-qc
keywords gravitymodesedgeentropyhaywardtermactionarea
verification ladder T0 review T1 audit T2 compute T3 formal
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We argue that corner contributions in gravity action (Hayward term) capture the essence of gravity edge modes, which lead to gravitational area entropies, such as the black hole entropy and holographic entanglement entropy. We explain how the Hayward term and the corresponding edge modes in gravity are explained by holography from two different viewpoints. One is an extension of AdS/CFT to general spacetimes and the other is the AdS/BCFT formulation. In the final part, we explore how gravity edge modes and its entropy show up in string theory by considering open strings stuck to a Rindler horizon.

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Cited by 3 Pith papers

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  3. Emergent Holographic Spacetime from Quantum Information

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    Takayanagi's essay outlines a research program in which holographic spacetime, including the time direction, may emerge from entanglement, complexity, and complex-valued pseudo-entropy, without presenting a new derivation.

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