论文标题
使用Ashtekar变量的重力诱导的破坏模型
A gravitationally induced decoherence model using Ashtekar variables
论文作者
论文摘要
我们考虑标量场与线性重力的耦合,并使用Ashtekar变量得出相对论重力诱导的反应模型。该模型是在关系形式主义中使用合适的几何时钟在规格不变水平上制定的,从而扩大了脱碳模型的现有规格不变制剂。为了构建Dirac可观察物,我们通过一种偶数互换的双重映射扩展了可观察到的可观察地图。我们还讨论了ADM文献中存在的第二种几何时钟选择。然后,我们将减少的相空间定量应用于Fock空间,并得出最终的主方程,为重力环境和使用投影操作员技术选择Gibbs状态。由此产生的主方程不是自动的lindblad类型,这是现象学模型有时会假定的起点,但由于我们以热Wightman函数表达的相关函数的形式,在主方程中有效运算符的水平仍然涉及剩余时间依赖性。此外,我们讨论了为什么在这里分析的模型中,第二个马尔可夫近似的应用,以便获得一组时间独立的有效系统操作员的直接不那么直接,而不是在某些量子机械模型中。
We consider the coupling of a scalar field to linearised gravity and derive a relativistic gravitationally induced decoherence model using Ashtekar variables. The model is formulated at the gauge invariant level using suitable geometrical clocks in the relational formalism, broadening existing gauge invariant formulations of decoherence models. For the construction of the Dirac observables we extend the known observable map by a kind of dual map where the role of clocks and constraints is interchanged. We also discuss a second choice of geometrical clocks existing in the ADM literature. Then we apply a reduced phase space quantisation on Fock space and derive the final master equation choosing a Gibbs state for the gravitational environment and using the projection operator technique. The resulting master equation is not automatically of Lindblad type, a starting point sometimes assumed for phenomenological models, but still involves a residual time dependence at the level of the effective operators in the master equation due to the form of the correlation functions that we express in terms of thermal Wightman functions. Furthermore, we discuss why in the model analysed here the application of a second Markov approximation in order to obtain a set of time independent effective system operators is less straightforward than in some of the quantum mechanical models.