English

Kinematic space and the orbit method

High Energy Physics - Theory 2019-07-24 v1 General Relativity and Quantum Cosmology

Abstract

Kinematic space has been defined as the space of codimension-22 spacelike extremal surfaces in anti de Sitter (AdSd+1_{d+1}) spacetime which, by the Ryu-Takayanagi proposal, compute the entanglement entropy of spheres in the boundary CFTd_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 dd-dimensional conformal group SO(d,2)SO(d,2). In addition, we show that the Crofton form on kinematic space associated to AdS3_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.

Keywords

Cite

@article{arxiv.1812.02176,
  title  = {Kinematic space and the orbit method},
  author = {Robert F. Penna and Claire Zukowski},
  journal= {arXiv preprint arXiv:1812.02176},
  year   = {2019}
}

Comments

25 pages, 5 figures

R2 v1 2026-06-23T06:33:08.185Z