Dark energy from Neutrinos and Standard Model Higgs potential

preprint2010arXivOpen access

Abstract

If neutrino mass is a function of the Higgs potential then minimum of the total thermodynamic potential ΩΩ (which is the Higgs potential minus the neutrino pressure) can shift from the standard electro-weak vev v=246.2v=246.2 GeV by a small amount which depends on the neutrino pressure. If the neutrino mass is a very steep function of the Higgs field then the equilibrium thermodynamic potential can act like the dark energy with ω≃−1ω\simeq -1. Choosing the neutrino mass as logarithmic function of the Higgs field and a heavy mass scale, we find that the correct magnitude of the cosmological density of the present universe ρλ≃(0.002eV)4ρ_λ\simeq (0.002 eV)^4 is obtained by choosing the heavy mass at the GUT scale.

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