Loop Quantization and Symmetry: Configuration Spaces

Christian Fleischhack

Published 2010-10-03, updated 2014-09-23Version 2

Given two sets $S_1, S_2$ and unital C*-algebras $A_1$, $A_2$ of functions thereon, we show that a map $\sigma : S_1 \nach S_2$ can be lifted to a continuous map $\bar\sigma : \spec A_1 \to \spec A_2$ iff $\sigma^\ast A_2 := \{\sigma^\ast f | f \in A_2\} \subset A_1$. Moreover, $\overline\sigma$ is unique if existing, and injective iff $\sigma^\ast A_2$ is dense. Then, we apply these results to loop quantum gravity and loop quantum cosmology. Here, the quantum configuration spaces are indeed spectra of certain C*-algebras $A_\cosm$ and $A_\grav$, respectively, whereas the choices for the algebras diverge in the literature. We decide now for all usual choices whether the respective cosmological quantum configuration space is embedded into the gravitational one. Typically, there is no embedding, but one can always get an embedding by defining $A_\cosm := C^\ast(\sigma^\ast A_\grav)$, where $\sigma$ denotes the embedding between the classical configuration spaces. Finally, we explicitly determine $C^\ast(\sigma^\ast A_\grav)$ in the homogeneous isotropic case for $A_\grav$ generated by the matrix functions of parallel transports along analytic paths. The cosmological quantum configuration space obtained this way, equals the disjoint union of $\R$ and the Bohr compactification of $\R$, appropriately glued together.