Exotic Low Density Fermion States in the Two Measures Field Theory: Neutrino Dark Energy
E. I. Guendelman, A. B. Kaganovich

TL;DR
This paper explores a novel fermion state in Two Measures Field Theory where neutrinos can behave as dark energy, leading to unique cosmological effects such as increasing neutrino mass and a universe with an equation-of-state approaching w=-1.
Contribution
It introduces a new fermion state in TMT where neutrinos mimic dark energy, with analytic solutions and implications for late-time cosmology and cosmic acceleration.
Findings
Neutrino mass scales as m ~ a^{3/2}
Neutrinos behave as dark energy with w approaching -1
Total energy density is less than scalar field alone
Abstract
We study a new field theory effect in the cosmological context in the Two Measures Field Theory (TMT). TMT is an alternative gravity and matter field theory where the gravitational interaction of fermionic matter is reduced to that of General Relativity when the energy density of the fermion matter is much larger than the dark energy density. In this case also the 5-th force problem is solved automatically. In the opposite limit, where the magnitudes of fermionic energy density and scalar field dark energy density become comparable, nonrelativistic fermions can participate in the cosmological expansion in a very unusual manner. Some of the features of such states in a toy model of the late time universe filled with homogeneous scalar field and uniformly distributed nonrelativistic neutrinos: neutrino mass increases as m ~ a^{3/2}; the neutrino gas equation-of-state approaches w=-1, i.e.…
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