A Deterministic Hydrodospatial Framework for Exoplanetary Atmospheric Screening and Habitable Oasis Localization: The Universmodel v2.3 Protocol

This paper provides the complete operational metadata and empirical verification registry for the Universmodel v2.3, a strictly deterministic cosmological and planetary framework. By rejecting stochastic quantum mechanics and modeling vacuum space as a chiral, crystalline superfluid under a universal baseline pressure (P_0 = 8.73 x 10^29 N/m²), this framework establishes absolute geometric parameters for exoplanetary habitability. To achieve maximum computational efficiency, the model utilizes a four-step Causal Cascade Screening Engine that evaluates stellar systems through sequential physical boundaries: (1) Stellar Shear Screening (F_shear), (2) Critical Lattice Cavitation Thresholds (r_min), (3) Planetary Internal Degassing Ignition limits (0.025 Earth Masses), and (4) Hydrostatic Gas Retention Resonance (S_molecule). This dataset catalogs the deterministic screening output of an unbroken 500-star astronomical survey out to a radius of 125 light-years. The screening engine isolates exactly 13 verified human-breathable planetary oases (including Alpha Centauri A, Epsilon Indi A, and HD 84117), establishing a rigid cosmic occurrence rate of 2.6%. The results demonstrate that life-supporting atmospheric zones are non-stochastic, geometrically locked structural anomalies dictated by stellar pressure fields and macro-cyclic galactic pulses.