Solving the Cosmological Constant Problem via Two-Time Dynamics of ∇T in Meta-Monism

The cosmological constant problem, marked by a 50120 order-of-magnitude discrepancy between theoretical predictions and observations, is a central challenge in cosmology. This work proposes a novel solution within the Meta-Monism framework, interpreting time as a dual modality (T1, T2). The cosmological constant Λ is formulated as a function of tensorial temporal tension ∇T, arising from the interplay between actual (T1) and potential (T2) time. We derive generalized Friedmann equations with Λ(T1, T2), aligning with observed values without fine-tuning. The Granda Constant (F0 ≈ 1019 Hz) sets a frequency threshold for quantum phase stability, enabling testable predictions via photon aging, void analysis, and Λ(z) evolution, verifiable with Euclid, DESI, and CMB-S4 data.