  Redshift drift is the phenomenon whereby the observed redshift between an
emitter and observer comoving with the Hubble flow in an expanding FLRW
universe will slowly evolve -- on a timescale comparable to the Hubble time. In
a previous article [JCAP 04 (2020) 043; arXiv 2001.11964] three of the current
authors had performed a cosmographic analysis of the redshift drift in a FLRW
universe, temporarily putting aside the issue of dynamics (the Friedmann
equations). In the current article we now add dynamics, still within the
framework of an exact FLRW universe. We shall develop a suitable generic matter
model and apply it to both standard FLRW and various dark energy models.
Furthermore, we shall also present a section analyzing the utility of using
alternative cosmographic variables to describe the redshift drift data.
