Distinguishing Dark Energy Models with Neutrino Oscillations
  Dark Energy models are numerous and distinguishing between them is becoming
difficult. However, using distinct observational probes can ease this quest and
gives better assessment to the nature of Dark energy. To this end, the
plausibility of neutrino oscillations to be a probe of Dark Energy models is
investigated. First, a generalized formalism of neutrino (spinor field)
interaction with a classical scalar field in curved space-time is presented.
This formalism is then applied to two classes of Dark Energy models in a flat
Friedman-Lema\^itre-Robertson-Walker metric: a Cosmological Constant and scalar
field Dark Energy coupled to neutrinos. By looking at the neutrino oscillation
probability's evolution with redshift, these models can be distinguished, for
certain neutrino and scalar field coupling properties. This evolution could be
traced by neutrino flux in future underground, terrestrial or extraterrestrial
neutrino telescopes, which would assess probing Dark Energy models with this
technique.
