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Von Neumann's quantization of general relativity

机译:von neumann的量化一般相对论

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摘要

Von Neumann's procedure is applied to quantizing general relativity. Initial data for dynamical variables in the Planck epoch, where the Hubble parameter value coincided with the Planck mass are quantized. These initial data are defined in terms of the Fock orthogonal simplex in the tangent Minkowski spacetime and the Dirac conformal interval. The Einstein cosmological principle is used to average the logarithm of the determinant of the spatial metric over the spatial volume of the visible Universe. The splitting of general coordinate transformations into diffeomorphisms and transformations of the initial data is introduced. In accordance with von Neumann's procedure, the vacuum state is treated is a quantum ensemble that is degenerate in quantum numbers of nonvacuum states. The distribution of the vacuum state leads to the Casimir effect in gravidynamics in just the same way as in electrodynamics. The generating functional for perturbation theory in gravidynamics is found by solving the quantum energy constraint. The applicability range of gravidynamics is discussed along with the possibility of employing this theory to interpret modern observational data.
机译:von neumann的程序适用于量化一般相对性。普兰克epoch中动态变量的初始数据,其中量化了与绘制质量一致的哈勃参数值。这些初始数据是根据切线Minkowski Spacetime和Dirac保形间隔中的套筒正交单纯x而定义的。爱因斯坦宇宙学原理用于平均可见宇宙空间量的空间度量的决定因子。介绍了一般坐标转换的分裂成差异和初始数据的变换。根据von Neumann的程序,处理真空状态是一种量子集合,其在非撤分状态的量子数中是退化的。真空状态的分布在以与电动动力学中的方式相同的方式导致令人瞩目的基础效应。通过求解量子能量约束,发现了引人注目的扰动​​理论的产生功能。讨论了引人注目的适用性范围以及采用这种理论来解释现代观测数据的可能性。

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