A Dark Energy Paradigm: III. Unified Dark Sector to Predict Dark Energy, Dark Matter, and Baryonic Matter Distributions
Yong‐Jae Moon, Wook Koh
Abstract
Open-access reader
Yong‐Jae Moon, Wook Koh
Abstract
Open-access reader
Abstract A dark energy paradigm was first developed by authors to solve the cosmological constant problem and to predict lepton masses as evidence. It was used to reveal an underlying structure of a M ON D algorithm to model cold dark matter and to predict galactic dynamics. In this paper, the dark energy paradigm a unified dark sector that is based on Planck’s dimensional analysis, ΛCDM , energy conservation, and force equilibrium is further developed to predict the distribution of dark energy, dark matter, and baryonic matter as well. We find that the dark energy distribution is predicted to be ΩΛ ≈ 0.667, which agrees withthe observed value with a 1% difference. We find that dark matter and baryonic matter distributions are predicted to be Ωc ≈ 0.283 and Ωb ≈ 0.050, respectively, which agree with the observed values with 1% differences.
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Abstract A dark energy paradigm was first developed by authors to solve the cosmological constant problem and to predict lepton masses as evidence. It was used to reveal an underlying structure of a M ON D algorithm to model cold dark matter and to predict galactic dynamics. In this paper, the dark energy paradigm a unified dark sector that is based on Planck’s dimensional analysis, ΛCDM , energy conservation, and force equilibrium is further developed to predict the distribution of dark energy, dark matter, and baryonic matter as well. We find that the dark energy distribution is predicted to be ΩΛ ≈ 0.667, which agrees withthe observed value with a 1% difference. We find that dark matter and baryonic matter distributions are predicted to be Ωc ≈ 0.283 and Ωb ≈ 0.050, respectively, which agree with the observed values with 1% differences.
Key concepts: Physics, Scalar field dark matter, Dark fluid, Dark energy, Dark matter, Hot dark matter, Mixed dark matter, Astrophysics