Emergent Dark Energy in Classical Channel Gravity with Matter
  Motivated by the recent increased interest in energy non-conserving models in
cosmology, we extend the analysis of the cosmological consequences of the
Classical Channel Model of Gravity (CCG). This model is based on the
classical-quantum interaction between a test particle and a metric (classical)
and results in a theory with a modified Wheeler-deWitt equation that in turn
leads to non conservation of energy. We show that CCG applied to a cosmological
scenario with primordial matter leads to an emergent dark fluid that at late
times behaves as a curvature term in the Friedmann equations, showing that the
late time behaviour is always dominated by the vacuum solutions. We discuss
possible observational constraints for this model and that, in its current
formulation, CCG eludes any meaningful constraints from current observations.
