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The research explores unresolved issues in cosmology, including baryogenesis, dark matter detection, and the implications of the Interior Observer framework.

May 25, 2026Open Access

The Interior Observer Cosmological Framework: Baryogenesis, Impossible Galaxies, and the Dark Matter Null from Inside a Schwarzschild Horizon

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The research explores unresolved issues in cosmology, including baryogenesis, dark matter detection, and the implications of the Interior Observer framework.
Applied the Interior Observer framework to calculate the baryon-to-photon ratio and CMB temperature.
Investigated baryogenesis mechanisms through theorems related to thermal leptogenesis and topological data.
Conducted predictions on the behavior of dark matter in light of existing null detection results.
Derived baryon-to-photon ratio η = 5.749 × 10⁻¹⁰ with a 5.7% deviation from Planck results.
Identified a significant time increase (46-48%) for the formation of galaxies at redshift z > 10 compared to ΛCDM.
Predicted continued null results for dark matter detection experiments, suggesting future constraints at the neutrino floor.

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Randomized trial uncovers baryogenesis and dark matter predictions in cosmology, suggesting new frameworks for understanding.

Cite This Study

David Fife (2026) studied this question.

synapsesocial.com/papers/6a13e8680e02ee3982d33204 https://doi.org/10.5281/zenodo.20359713

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The Interior Observer Cosmological Framework: Baryogenesis, Impossible Galaxies, and the Dark Matter Null from Inside a Schwarzschild Horizon

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The Interior Observer Cosmological Framework: Baryogenesis, Impossible Galaxies, and the Dark Matter Null from Inside a Schwarzschild Horizon

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