New physics at low energies and dark matter-dark energy transmutation
E. I. Guendelman, A. B. Kaganovich

TL;DR
This paper proposes a theoretical framework where fermionic matter can transition into a new state at low energies, potentially explaining dark matter and dark energy phenomena through neutrino behavior in an expanding universe.
Contribution
It introduces the concept of Cosmo-Low Energy Physics (CLEP) states where neutrinos change properties, linking dark matter and dark energy within a unified fermion field theory.
Findings
Neutrinos in CLEP states have increasing masses proportional to a^{3/2}.
Dark matter in CLEP states exhibits negative pressure similar to dark energy.
Total universe energy density is lower with fermionic matter than without.
Abstract
A field theory is proposed where the regular fermionic matter and the dark fermionic matter can be different states of the same "primordial" fermion fields. In regime of the fermion densities typical for normal particle physics, the primordial fermions split into three families identified with regular fermions. When fermion energy density becomes comparable with dark energy density, the theory allows transition to new type of states. The possibility of such Cosmo-Low Energy Physics (CLEP) states is demonstrated by means of solutions of the field theory equations describing FRW universe filled with homogeneous scalar field and uniformly distributed nonrelativistic neutrinos. Neutrinos in CLEP state are drawn into cosmological expansion by means of dynamically changing their own parameters. One of the features of the fermions in CLEP state is that in the late time universe their masses…
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