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Semi-Classical Limit of Quantum Gravity on Corners

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arxiv 2510.25843 v5 pith:LOOJOE5Y submitted 2025-10-29 hep-th math-phmath.MP

Semi-Classical Limit of Quantum Gravity on Corners

classification hep-th math-phmath.MP
keywords quantumclassicalmathrmgravityobservablesrepresentation-theoreticabstractadmitting
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We study quantum and classical systems associated with the quantum corner symmetry group $\mathrm{QCS}=\widetilde{\mathrm{SL}}(2,\mathbb{R})\ltimes \mathrm{H}_3,$ which arises in the context of quantum gravity. We relate quantum observables -- specified by representation-theoretic data -- to their classical counterparts using generalized Perelomov coherent states and the framework of Berezin quantization. This procedure links abstract representation-theoretic input to geometric classical observables, such as area. We conclude by applying the formalism to static, spherically symmetric spacetimes admitting a horizon.

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  1. Quantum Geometry from Area Fluctuations

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    Derives a thermal fluctuation formula for causal-diamond boundary area with a linear term of Verlinde-Zurek scaling interpreted as statistical evidence for discrete quanta of geometry.