Dark energy from neutrinos and standard model Higgs potential

The dark energy density of the universe is obtained from the Higgs potential by introducing a Higgsdependent neutrino mass. In the standard picture of electro-weak symmetry breaking the Higgs potential is V/ = (k/4)(/2 v2)2 and the Higgs field rolls down to the minima at h/i = v = 246.2 GeV and the net vacuum energy is zero. Now if the neutrino mass is a function of the Higgs field, then the vacuum expectation value of the Higgs is determined by maximizing the total pressure of the Higgs self interaction and the neutrino fluid P/ + Pm(m(/)) w.r.t /. The new minima h/i = v + rm shifts from the standard Higgs vev v by a small amount rm. The total pressure of the Higgs-neutrino coupled fluid P/(v + rm) + Pm(v + rm) = qK appears as the dark energy density of the universe. The magnitude of the dark energy is thus determined by to the neutrino mass and the Higgs potential