Neutrino generated dynamical dark energy with no dark energy field
  Dynamical dark energy (DE) phenomenon emerges as a geometrical effect
accompanying the cosmological expansion of nonrelativistic fermionic matter.
This occurs without the need for any fluid, like e.g. dynamical scalar field
(quintessence, cosmon, etc.), and with conventional form of the Einstein
equations in contrast to other known geometrical DE models. The phenomenon
results from first principles in the framework of the two measures field theory
where, in the Einstein frame, both fermion masses and the cosmological constant
(CC) turn into functions of the cold fermion density n. This n dependence
becomes negligible in regular (laboratory) conditions but it may have an
important role in cosmology. In the 4D gravity model where the original action
involves only CC and massive fermions without selfinteraction, for different
(but wide) regions in the parameter space we have found two possible classes of
scenarios for the late universe starting from the cold matter domination era.
We argue that the fermions which drive the variable CC should be associated
with cold neutrinos disposed in voids and supervoids. The cosmological dynamics
of the first class practically coincides with that of the LambdaCDM model,
while the dynamics of the second class is of the phantom-like regime with a
pseudo-rip scenario. Crossing the phantom divide happens due to a new type of
the neutrino DE effect where neutrinos pass through the state with zero mass
and with the vacuum-like EoS P_{\nu}=-\rho_{\nu}.
