Dark energy and dark matter unification from dynamical space time:
  observational constraints and cosmological implications
  A recently proposed Dynamical Space-time Cosmology (DSC) that unifies dark
energy and dark matter is studied. The general action of this scenario includes
a Lagrange multiplier, which is coupled to the energy momentum tensor and a
scalar field which is different from quintessence. First for various types of
potentials we implement a critical point analysis and we find solutions which
lead to cosmic acceleration and under certain conditions to stable late-time
attractors. Then the DSC cosmology is confronted with the latest cosmological
data from low-redshift probes, namely measurements of the Hubble parameter and
standard candles (Pantheon SnIa, Quasi-stellar objects). Performing an overall
likelihood analysis and using the appropriate information criteria we find that
the explored DSC models are in very good agreement with the data. We also find
that one of the DSC models shows a small but non-zero deviation from $\Lambda$
cosmology, nevertheless the confidence level is close to $\sim 1.5\sigma$.
