  Within the functional renormalization group approach to Background
Independent quantum gravity, we explore the scale dependent effective geometry
of the de Sitter solution dS${}_4$. The investigation employs a novel approach
whose essential ingredient is a modified spectral flow of the metric dependent
d'Alembertian, or of similar hyperbolic kinetic operators. The corresponding
one-parameter family of spectra and eigenfunctions encodes information about
the nonperturbative backreaction of the dynamically gravitating vacuum
fluctuations on the mean field geometry of the quantum spacetime. Used as a
diagnostic tool, the power of the spectral flow method resides in its ability
to identify the scale dependent subsets of field modes that supply the degrees
of freedom which participate in the effective field theory description of the
respective scale. A central result is that the ultraviolet of Quantum Einstein
Gravity comprises far less effective degrees of freedom than predicted
(incorrectly) by background dependent reasoning. Exploring the quantum
spacetime's spatial geometry carried by physical fields, we find that
3-dimensional space disintegrates into a collection of coherent patches which
individually can, but in their entirety cannot be described by one of the
effective average actions occurring along the renormalization group trajectory.
A natural concept of an entropy is introduced in order to quantify this
fragmentation effect. Tentatively applied to the real Universe, surprising
analogies to properties of the observed cosmic microwave background are
uncovered. Furthermore, a set of distinguished field modes is found which, in
principle, has the ability to transport information about the asymptotic fixed
point regime from the ultraviolet, across almost the entire "scale history", to
cosmological distances in the observed Universe.
