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arXiv 2302.02840gr-qchep-thmath-phmath.MP
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黎曼量子几何的出现

Emergence of Riemannian Quantum Geometry

Hal M. Haggard, Jerzy Lewandowski, Hanno Sahlmann

摘要:

在这一章中,我们讨论时空的空间切片的量子黎曼几何。虽然研究人员仍然面临着观测量子引力的挑战,但循环量子引力有一个几何核心,它在很大程度上定义了这种方法。这个核心是它的几何可观测量的量子特性:空间和时空是由普朗克尺度的量子颗粒构成的。这些颗粒之间的相互关系由自旋网络来描述,自旋网络的边缘捕获了互连节点的边界区域,这些节点编码了每个颗粒的范围。我们解释了量子黎曼几何如何从两种不同的方法中产生:在本章的前半部分,我们从连续统几何的角度出发,解释了量子几何如何从一些原理中产生,例如场论正则量子化的一般规则,广义相对论的经典公式,它似乎嵌入在杨-米尔斯理论的相空间中,以及广义协方差。在本章的后半部分,我们证明了量子几何也是从离散几何中编码的引力场的有限自由度的直接量子化中产生的。这两种方法是互补的,并提供帮助读者与不同的背景进入量子黎曼几何引人注目的舞台。

英文摘要:

In this chapter we take up the quantum Riemannian geometry of a spatial slice of spacetime. While researchers are still facing the challenge of observing quantum gravity, there is a geometrical core to loop quantum gravity that does much to define the approach. This core is the quantum character of its geometrical observables: space and spacetime are built up out of Planck-scale quantum grains. The interrelations between these grains are described by spin networks, graphs whose edges capture the bounding areas of the interconnected nodes, which encode the extent of each grain. We explain how quantum Riemannian geometry emerges from two different approaches: in the first half of the chapter we take the perspective of continuum geometry and explain how quantum geometry emerges from a few principles, such as the general rules of canonical quantization of field theories, a classical formulation of general relativity in which it appears embedded in the phase space of Yang-Mills theory, and general covariance. In the second half of the chapter we show that quantum geometry also emerges from the direct quantization of the finite number of degrees of freedom of the gravitational field encoded in discrete geometries. These two approaches are complimentary and are offered to assist readers with different backgrounds enter the compelling arena of quantum Riemannian geometry.

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