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An inhomogeneous toy model of the quantum gravity with the explicitly evolvable observables

机译:具有明显演化的可观测物的量子引力的不均匀玩具模型

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An inhomogeneous (1 $+$ 1)-dimensional model of the quantum gravity is considered. It is found, that this model corresponds to a string propagating in some curved background space. The quantization scheme including the Wheeler–DeWitt equation and the “particle on a sphere” type of the gauge condition is suggested. In the quantization scheme considered, the “problem of time” is resolved by building of the quasi-Heisenberg operators acting in a space of solutions of the Wheeler–DeWitt equation, and the normalization of the wave function corresponds to the Klein–Gordon type. To analyze the physical consequences of the scheme, a (1 $+$ 1)-dimensional background space is considered for which a classical solution is found and quantized. The obtained estimations show the way to solution of the cosmological constant problem for this model. Such a solution consists in compensation of the zero-point oscillations of the matter fields by the quantum oscillations of the scale factor. Along with such a compensation, a slow global evolution of a background exists that corresponds to an universe expansion.
机译:考虑了量子引力的不均匀(1 + 1)维模型。发现,该模型对应于在某些弯曲背景空间中传播的弦。建议使用量化方案,包括Wheeler-DeWitt方程和标尺条件的“球形粒子”类型。在考虑的量化方案中,“时间问题”通过建立在惠勒-德维特方程解的空间中起作用的准海森堡算子来解决,并且波函数的归一化对应于克莱因-戈登类型。为了分析该方案的物理结果,考虑了一个(1 $ + 1)尺寸的背景空间,为此找到了经典的解决方案并对其进行了量化。获得的估计值显示了该模型解决宇宙常数问题的方法。这种解决方案在于通过比例因子的量子振荡来补偿物质场的零点振荡。伴随着这样的补偿,存在着与宇宙膨胀相对应的背景的缓慢全球演变。

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