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Research examines cosmic structure formation in the Honeyverse, suggesting novel growth mechanisms.
Paper 7 of 8 This paper examines how cosmic structure forms within the Honeyverse dual‑lattice framework. By analyzing perturbations on the HU lattice and their interaction with the ghost‑sector mismatch, the paper derives modified growth equations that reproduce the observed large‑scale structure without invoking dark energy or exotic matter components. The results show that the HU/ghost ratio λ acts as a scale‑dependent modifier of perturbation growth, suppressing or enhancing structure at different epochs. This provides a unified explanation for the timing of structure formation, the onset of cosmic acceleration, and the observed matter power spectrum. v1
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R. D. Howard (2026) studied this question.