This paper integrates the scale-invariant properties of the Dewhirst Horizon Relation—a physical framework formulated by Richard Stephen Dewhirst that replaces the static speed of light squared constant (c²) with a dynamic macro-to-micro spacetime horizon ratio (
ΩD)—directly into quantum wave mechanics.The text addresses the notorious Measurement Problem and Schrödinger's Cat paradox, which describe quantum systems existing in fuzzy states of probability until a human observes them. This model demonstrates that by modifying the Time-Dependent Schrödinger Equation with the dynamic Dewhirst Operator, human observation is replaced by a physical, clock-driven cosmic filter.Because macroscopic systems are linked to massive spatial boundaries (2.72 × 10⁶¹ Planck pixels) and long historical timelines, the background universe acts as a natural, continuous observer. The calculation proves that this scale-dependent filter automatically dampens complex quantum probability waves for macroscopic objects, forcing definite real-world outcomes natively.Furthermore, the modified wave equation smoothly suppresses infinite loop divergences at high energies, matching real-world CERN detector spikes while scale-stabilizing massive early-universe structures without fine-tuned mathematical filters.
It has been argued that when black holes are treated as quantum systems there are implications at the horizon and not just the singularity. Infalling observers will meet a firewall of high energy quanta. We argue that the question of whether an observer falling into a black hole experiences a smooth horizon or a firewall is identical to the question of whether Schrödinger's cat is either in a definite state, alive or dead, or in a superposition of the two. Since experience with real macro-systems indicate the former, the black hole state vector is seen to describe a set of decoherent alternatives each with a smooth horizon and the entanglement puzzle is thereby side stepped.
Abstract: It has been argued that when black holes are treated as quantum systems there are implications at the horizon and not just the singularity. Infalling observers will meet a firewall of high energy quanta. We argue that the question of whether an observer falling into a black hole experiences a smooth horizon or a firewall is identical to the question of whether Schrödinger’s cat is either in a definite state, alive or dead, or in a superposition of the two. Since experience with real macro-systems indicate the former, the black hole state vector is seen to describe a set of decoherent alternatives each with a smooth horizon and the entanglement puzzle is thereby side stepped.