Entanglement and Generalized Berry Geometrical Phases in Quantum Gravity

Symmetry Pub Date : 2024-08-12 DOI:10.3390/sym16081026
Diego J. Cirilo-Lombardo, Norma G. Sanchez
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Abstract

A new formalism is introduced that makes it possible to elucidate the physical and geometric content of quantum space–time. It is based on the Minimum Group Representation Principle (MGRP). Within this framework, new results for entanglement and geometrical/topological phases are found and implemented in cosmological and black hole space–times. Our main results here are as follows: (i) We find the Berry phases for inflation and for the cosmological perturbations and express them in terms of the observables, such as the spectral scalar and tensor indices, nS and nT, and the tensor-to-scalar ratio r. The Berry phase for de Sitter inflation is imaginary with the sign describing the exponential acceleration. (ii) The pure entangled states in the minimum group (metaplectic) Mp(n) representation for quantum de Sitter space–time and black holes are found. (iii) For entanglement, the relation between the Schmidt type representation and the physical states of the Mp(n) group is found: This is a new non-diagonal coherent state representation complementary to the known Sudarshan diagonal one. (iv) Mean value generators of Mp(2) are related to the adiabatic invariant and topological charge of the space–time, (matrix element of the transition −∞
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量子引力中的纠缠和广义贝里几何相位
本文引入了一种新的形式主义,使阐明量子时空的物理和几何内容成为可能。它以最小群表示原理(MGRP)为基础。在这一框架内,我们发现了纠缠和几何/拓扑相位的新结果,并在宇宙学和黑洞时空中加以实现。我们的主要成果如下(i) 我们找到了暴胀和宇宙学扰动的贝里相位,并用光谱标量和张量指数 nS 和 nT 以及张量与标量之比 r 等观测指标来表示。(ii) 发现了量子德西特时空和黑洞在最小群(元映射)Mp(n) 表示中的纯纠缠态。(iii) 就纠缠而言,找到了施密特型表示与 Mp(n) 群物理状态之间的关系:这是一种新的非对角相干态表示,是对已知须弥对角表示的补充。(iv) Mp(2) 的均值发生器与绝热不变量和时空拓扑电荷有关(转换的矩阵元素-∞
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