点阵引力和宇宙学

J. Bilski
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引用次数: 0

摘要

与背景无关的量子引力是构建广义相对论量子场论的必要框架。通过假设时空的ADM分解,可以为该公式定义与度量无关的Fock空间。这个空间称为自旋网络,在SU(2)对称和空间微分同态变换下是不变的。它是环量子引力模型的Fock空间,其中正则算符是Ashtekar连接的量子化完整组和致密化dreibein的通量。我将提出一种改进的晶格引力构造及其基于相同晶格变量的量规固定宇宙学约简。该方法基于正则化参数中二次项的幂级数几何展开。结果得到了一个更精确的过程,其中连接的对称性直接反映在连接的相关分布上。将这一过程应用于哈密顿约束正则化,提供了它的晶格类比,其域具有初等元胞和的自然结构。因此,可以定义相关的标量约束算子,其谱与缠绕无关。晶格引力的宇宙学相空间约简需要严格地应用规范固定条件来降低SU(2)对称性和空间微分同态不变性。将内部对称性固定在阿贝尔情况下,同时将微分同胚不变性简化为空间平移。所得到的哈密顿约束是有限的(没有任何截断引入)和精确的(没有围绕短链的完整展开)。此外,它具有对初等立方单元求和的期望形式。最后,它的均匀性和各向异性的简单结构应该允许用跃迁幅度来描述宇宙的量子宇宙学演化,而不是使用摄动近似。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Lattice gravity and cosmology
The background-independent quantum gravity is the necessary framework to construct generally relativistic quantum field theory. By assuming the ADM decomposition of spacetime, it is possible to define the metric-independent Fock space for this formulation. This space, known as spin network, is invariant under the SU(2) symmetry and the spatial diffeomorphisms transformations. It is the Fock space for the model called loop quantum gravity in which the canonical operators are the quantized holonomies of the Ashtekar connection and the fluxes of densitized dreibein. I will present an improved construction of the lattice gravity and its gauge-fixed cosmological reduction based on the same lattice variables. The approach is based on the geometric expansion of holonomies into power series up to the quadratic order terms in the regularization parameter. As a result, a more accurate procedure is obtained in which the symmetry of holonomies assigned to links is directly reflected in the related distribution of connections. The application of the procedure to the Hamiltonian constraint regularization provides its lattice analog, the domain of which has a natural structure of elementary cells sum. In consequence, the related scalar constraint operator, which spectrum is independent of intertwiners, can be defined. The cosmological phase space reduction of lattice gravity requires rigorous application of gauge-fixing conditions that reduce the SU(2) symmetry and the spatial diffeomorphisms invariance. The internal symmetry is fixed to the Abelian case and the diffeomorphisms invariance is simultaneously reduced to spatial translations. The obtained Hamiltonian constraint is finite (without any cut-off introduction) and exact (without the holonomy expansion around short links). Furthermore, it has the expected form of the sum over elementary cuboidal cells. Finally, the simple structure of its homogeneities and anisotropies should allow to describe the quantum cosmological evolution of the Universe in terms of transition amplitudes, instead of using perturbative approximations.
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