Neutrino mixing contribution to the cosmological constant
M.Blasone, A.Capolupo, S.Capozziello, S.Carloni, G.Vitiello

TL;DR
This paper demonstrates that neutrino mixing's non-perturbative vacuum structure contributes a non-zero amount to the cosmological constant, offering a novel perspective on dark energy.
Contribution
It introduces a new mechanism linking neutrino mixing to the cosmological constant, distinct from traditional massive field contributions.
Findings
Neutrino mixing induces a non-zero vacuum energy contribution.
The contribution is estimated using a natural quantum field theory cutoff.
This mechanism provides a potential explanation for dark energy.
Abstract
We show that the non-perturbative vacuum structure associated with neutrino mixing leads to a non-zero contribution to the value of the cosmological constant. Such a contribution comes from the specific nature of the mixing phenomenon. Its origin is completely different from the one of the ordinary contribution of a massive spinor field. We estimate this neutrino mixing contribution by using the natural cut--off appearing in the quantum field theory formalism for neutrino mixing and oscillation.
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