Cosmological constant from Standard Model spin

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Determination of the Cosmological Constant Magnitude via Phase-Space Suppression from the Standard Model Fermionic Spin Degrees of Freedom | Zenodo

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Published July 23, 2026

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Determination of the Cosmological Constant Magnitude via Phase-Space Suppression from the Standard Model Fermionic Spin Degrees of Freedom

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Kis, Norbert Levente

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Determination of the Cosmological Constant Magnitude via Phase-Space Suppression from the Standard Model Fermionic Spin Degrees of Freedom

The cosmological constant problem the 122-order of magnitude discrepancy between quantum field theory predictions and observed dark energy density is addressed using only the experimentally established fermionic content of the Standard Model. We show that the total number of independent spin degrees of freedom in the Standard Model (N_spin = 90, derived from 3 generations × 15 fermion types × 2 spin states) generates a non-perturbative phase-space suppression factor of e^(-90π) in the Euclidean path integral. Multiplying the Planck-scale vacuum energy density (ρ_P ≈ 4.63×10^113 J/m³) by this factor yields ρ_Λ ≈ 6.96×10^-10 J/m³, which agrees with the Planck 2018 measured value (5.80×10^-10 J/m³) to within 20%. The remaining deviation is attributable to standard higher-order corrections (e.g., QCD instantons and Higgs fluctuations). This result requires no new particles, no extra dimensions, no supersymmetry, and no fine-tuning suggesting that the cosmic vacuum energy may be a direct consequence of the Standard Model's known fermionic phase-space structure.

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cosmological constant

dark energy

Standard Model

quantum field theory

phase space

vacuum energy

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10.5281/zenodo.21515348

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Kis Norbert Levente

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July 23, 2026

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July 23, 2026

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