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Kinematic space and the orbit method

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arxiv 1812.02176 v1 pith:XL3Z7XXK submitted 2018-12-05 hep-th gr-qc

classification hep-thgr-qc
keywords spacekinematicorbitcoadjointgroupsymplecticadditioncompute
verification ladder T0 review T1 audit T2 compute T3 formal

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abstract

Kinematic space has been defined as the space of codimension-$2$ spacelike extremal surfaces in anti de Sitter (AdS$_{d+1}$) spacetime which, by the Ryu-Takayanagi proposal, compute the entanglement entropy of spheres in the boundary CFT$_d$. It has recently found many applications in holography. Coadjoint orbits are symplectic manifolds that are the classical analogues of a Lie group's unitary irreducible representations. We prove that kinematic space is a particular coadjoint orbit of the $d$-dimensional conformal group $SO(d,2)$. In addition, we show that the Crofton form on kinematic space associated to AdS$_3$, that was shown to compute the lengths of bulk curves, is equal to the standard Kirillov-Kostant symplectic form on the coadjoint orbit. Since kinematic space is K\"{a}hler in addition to symplectic, it can be quantized. The orbit method extends the kinematic space dictionary, which was originally motivated through connections to integral geometry, by directly translating geometrical properties of holographic auxiliary spaces into statements about the representation theory of the conformal group.

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Cited by 2 Pith papers

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    A solvable low-energy effective theory based on the warped Virasoro group with three cocycles is constructed, and its one-loop-exact partition function and thermodynamics are derived.

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    Cross-boundary entanglement thread flux in a planar BTZ wormhole is computed explicitly (Eq. 53) and shown to integrate to the standard thermal entropy density.

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