Dark energy models which alter the relative scaling behavior of dark energy
and matter could provide a natural solution to the cosmic coincidence prob
lem-why the densities of dark energy and dark matter are comparable today.
A generalized class of dark energy models is introduced which allows noncan
onical scaling of the ratio of dark matter and dark energy with the Roberts
on-Walker scale factor a(t). We show that determining whether there is a co
incidence problem, and the extent of cosmic coincidence, can be addressed b
y several forthcoming experiments.