Quantum Omnipresence and the Probability of a Creator: A Standard Quantum Mechanical Derivation

This study examines a proposed connection between zero-energy cosmological models, quantum states, and the conceptual possibility of a purposeful origin of the universe. Within the Indeterminate Null framework, the analysis considers a hypothetical zero-energy, zero-momentum initial state and investigates its mathematical properties using uncertainty relations, the Schr?dinger equation, quantum field theory, and quantum superposition. The study also discusses cosmological fine-tuning arguments and compares two proposed origin scenarios under selected assumptions. A free-particle plane-wave model with zero momentum and energy yields a spatially and temporally constant amplitude, although its physical interpretation depends on normalization, boundary conditions, and the existence of an appropriate spacetime description. The analysis identifies possible conceptual connections between quantum delocalization and the proposed interpretation of omnipresence. The probability comparison remains conditional on assumptions about prior distributions, independence, and physical mechanisms. The findings provide a theoretical framework for further investigation rather than a definitive demonstration of a creator or a unique cosmological origin mechanism. Determinate Null (IN) framework replaces the continuous real-number coordinate domain used in selected physical calculations with a finite discrete set bounded by the Planck length and a de Sitter scale. Building on the photon-gravity construction introduced in earlier work, this paper defines an IN derivative as a forward finite difference, an IN integral as a finite sum, and an associated telescoping Fundamental Theorem. Three applications are examined. First, imposing the resulting ultraviolet and infrared bounds converts the vacuum zero-point-energy expression into a finite quantity, while leaving a large discrepancy with the observed dark-energy density. Second, evaluation of cosmological quantities from a finite Planck-scale starting point avoids evaluation at zero time and permits a discrete recurrence formulation. Third, restricting radial coordinates to values no smaller than the Planck length bounds the Schwarzschild Kretschmann scalar on the proposed domain. These results show how finite-domain discretization removes the specific mathematical divergences considered here. Further justification is required m-field and gravitational problems.