Tessarotto Massimo, Cremaschini Claudio
Department of Mathematics and Geosciences, University of Trieste, Via Valerio 12, 34127 Trieste, Italy.
Institute of Physics, Faculty of Philosophy and Science, Silesian University in Opava, Bezručovo nám.13, CZ-74601 Opava, Czech Republic.
Entropy (Basel). 2018 Mar 19;20(3):205. doi: 10.3390/e20030205.
A trajectory-based representation for the quantum theory of the gravitational field is formulated. This is achieved in terms of a covariant Generalized Lagrangian-Path (GLP) approach which relies on a suitable statistical representation of Bohmian Lagrangian trajectories, referred to here as . The result is established in the framework of the manifestly-covariant quantum gravity theory (CQG-theory) proposed recently and the related CQG-wave equation advancing in proper-time the quantum state associated with massive gravitons. Generally non-stationary analytical solutions for the CQG-wave equation with non-vanishing cosmological constant are determined in such a framework, which exhibit Gaussian-like probability densities that are non-dispersive in proper-time. As a remarkable outcome of the theory achieved by implementing these analytical solutions, the existence of an emergent gravity phenomenon is proven to hold. Accordingly, it is shown that a mean-field background space-time metric tensor can be expressed in terms of a suitable statistical average of stochastic fluctuations of the quantum gravitational field whose quantum-wave dynamics is described by GLP trajectories.
本文构建了一种基于轨迹的引力场量子理论表示形式。这是通过协变广义拉格朗日路径(GLP)方法实现的,该方法依赖于对玻姆拉格朗日轨迹的适当统计表示,在此称为[具体名称未给出]。结果是在最近提出的明显协变量子引力理论(CQG理论)框架以及相关的CQG波动方程中建立的,该波动方程使与有质量引力子相关的量子态在固有时中演化。在这样的框架中确定了具有非零宇宙学常数的CQG波动方程的一般非平稳解析解,这些解表现出在固有时中不弥散的类高斯概率密度。作为通过实施这些解析解所实现理论的一个显著成果,证明了涌现引力现象的存在。因此,表明平均场背景时空度规张量可以用由GLP轨迹描述其量子波动力学的量子引力场随机涨落的适当统计平均值来表示。