A model where a horizon-sourced energy influx Q = αH^3 drives expansion, flattens the universe without inflation, and may seed fluctuations, but the claims are not derived.
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Horizon-Driven Expansion from Hawking-Like Radiation: A Curvature-Coupled Cosmological Model
A model where a horizon-sourced energy influx Q = αH^3 drives expansion, flattens the universe without inflation, and may seed fluctuations, but the claims are not derived.