The vacuum energy density is claimed to be ρ = (1/8) m Λ^3 e^{-<n>}, matching the observed cosmological constant when <n> ≈ 250 and m ≈ Λ ≈ 10^16 GeV.
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Cosmological Constant Suppression in Non-Stationary Scalar Covariant State
The vacuum energy density is claimed to be ρ = (1/8) m Λ^3 e^{-<n>}, matching the observed cosmological constant when <n> ≈ 250 and m ≈ Λ ≈ 10^16 GeV.