A Statistical Resolution of the Cosmological Constant Problem

The cosmological constant problem is commonly summarized as a discrepancy of approximately 10^122 between a naive quantum-field-theoretic estimate of vacuum energy and the observed value of the cosmological constant. We propose a statistical and process-based reinterpretation in which the cosmological constant is not a manifestation of vacuum energy, but an emergent global residual of finite-resolution spacetime dynamics. The present work is based on the relational spacetime dynamics framework developed in [1]. Assuming that spacetime evolution proceeds through elementary update events occupying a minimal four-volume of order l_P^4, we show that the accumulated statistical residual over the four-dimensional history of the observable Universe naturally yields an effective cosmological constant of order 10^(-52) m^(-2), without any fine-tuning of parameters. We further develop the formal structure of the relational update dynamics, clarify its statistical interpretation, and discuss conceptual consequences and limitations. We emphasize that the argument is structural and statistical rather than a microscopic derivation, and we outline how it relates to existing discrete-spacetime approaches.