Phenomenology of Quantum Reduced Loop Gravity in the isotropic
  cosmological sector
  Quantum reduced loop gravity is designed to consistently study symmetry
reduced systems within the loop quantum gravity framework. In particular, it
bridges the gap between the effective cosmological models of loop quantum
cosmology and the full theory, addressing the dynamics before the
minisuperspace reduction. This mostly preserves the graph structure and SU(2)
quantum numbers. In this article, we study the phenomenological consequences of
the isotropic sector of the theory, the so-called emergent bouncing universe
model. In particular, the parameter space is scanned and we show that the
number of inflationary e-folds is almost always higher than the observational
lower-bound. We also compute the primordial tensor power spectrum and study its
sensitivity upon the fundamental parameters used in the model.
