Quantum null geometry and gravity

被引:4
作者
Ciambelli, Luca [1 ]
Freidel, Laurent [1 ]
Leigh, Robert G. [1 ,2 ,3 ]
机构
[1] Perimeter Inst Theoret Phys, 31 Caroline St N, Waterloo, ON N2L 2Y5, Canada
[2] Univ Illinois, Illinois Ctr Adv Studies Universe, 1110 West Green St, Urbana, IL 61801 USA
[3] Univ Illinois, Dept Phys, 1110 West Green St, Urbana, IL 61801 USA
关键词
Classical Theories of Gravity; Models of Quantum Gravity; Scale and Conformal Symmetries; Space-Time Symmetries; BLACK-HOLE ENTROPY; CONFORMAL FIELD-THEORY; DEFORMATION QUANTIZATION; SINGULARITY STRUCTURE; 2-POINT FUNCTION; STRING THEORY; TIME; SPACETIME; MODES; LOOP;
D O I
10.1007/JHEP12(2024)028
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
In this work, we demonstrate that quantizing gravity on a null hypersurface leads to the emergence of a CFT associated with each null ray. This result stems from the ultralocal nature of null physics and is derived through a canonical analysis of the Raychaudhuri equation, interpreted as a constraint generating null time reparametrizations. The CFT exhibits a non-zero central charge, providing a mechanism for the quantum emergence of time in gravitational systems and an associated choice of vacuum state. Our analysis reveals that the central charge quantifies the degrees of freedom along each null ray. Throughout our investigation, the area element of a cut plays a crucial role, necessitating its treatment as a quantum operator due to its dynamic nature in phase space or because of quantum backreaction. Furthermore, we show that the total central charge diverges in a perturbative analysis due to the infinite number of null generators. This divergence is resolved if there is a discrete spectrum for the area form operator. We introduce the concept of 'embadons' to denote these localized geometric units of area, the fundamental building blocks of geometry at a mesoscopic quantum gravity scale.
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页数:62
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