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首页> 外文期刊>International journal of modern physics, D. Gravitation, astrophysics, cosmology >Generating functional for the gravitational field: Implementation of an evolutionary quantum dynamics
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Generating functional for the gravitational field: Implementation of an evolutionary quantum dynamics

机译:产生引力场的函数:进化量子动力学的实现

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We provide a generating functional for the gravitational field that is associated with the relaxation of the primary constraints by extending to the quantum sector. This requirement of the theory relies on the assumption that a suitable time variable exists, when taking the T-products of the dynamical variables. More precisely, we start from the gravitational field equations written in the Hamiltonian formalism and expressed via Misner-like variables; hence we construct the equation to which the T-products of the dynamical variables obey and transform this paradigm in terms of the generating functional, as taken on the theory phase-space. We show how the relaxation of the primary constraints (which corresponds to the breakdown of the invariance of the quantum theory under the four-diffeomorphisms) is summarized by a free functional taken on the Lagrangian multipliers, accounting for such constraints in the classical theory. The issue of our analysis is equivalent to a Gupta-Bleuler approach on the quantum implementation of all the gravitational constraints; in fact, in the limit of small h, the quantum dynamics is described by a Schrodinger equation as soon as the mean values of the momenta, associated to the lapse function and the shift vector, are not vanishing. Finally we show how, in the classical limit, the evolutionary quantum gravity reduces to General Relativity in the presence of an Eckart fluid, which corresponds to the classical Counterpart of the physical clock, introduced in the quantum theory.
机译:我们提供了一个引力场的生成函数,该函数与扩展到量子扇区的基本约束的放松相关。该理论的要求依赖于以下假设:在获取动态变量的T乘积时,存在合适的时间变量。更准确地说,我们从用哈密尔顿形式论编写的引力场方程开始,并通过类似Misner的变量表示。因此,根据理论相空间,我们构造了动力学变量的T积服从的方程,并根据生成函数对这种范式进行了转换。我们展示了如何通过对拉格朗日乘子采取的自由函数来概括主要约束的弛豫(这对应于四微分同态下量子理论不变性的分解),从而解释了经典理论中的此类约束。我们的分析问题等效于所有引力约束的量子实现的Gupta-Bleuler方法。实际上,在小的h范围内,只要与衰减函数和位移矢量相关的矩量平均值不消失,就可以通过Schrodinger方程描述量子动力学。最后,我们展示了在经典极限中,在存在埃克特流体的情况下,进化量子引力如何减小到广义相对论,该流体对应于量子理论中引入的物理时钟的经典对应部分。

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