Primordial Latency Fluctuations and the CMB Angular Power Spectrum in a Finite-Capacity Universe

We develop the primordial perturbation sector of the finite-capacity latency–erasure program and derive the first early-universe observational interface of the theory. In the finite-capacity framework, the universe is realized through a bounded substrate whose local load fraction generates an emergent latency field . The earliest cosmic epoch is therefore a high-load regime in which stochastic patch irregularities naturally source primordial latency fluctuations . We show that these fluctuations define the scalar perturbation sector of the theory and yield a primordial power spectrum without introducing an ad hoc inflaton field. The resulting spectrum is propagated to the observable Cosmic Microwave Background through a latency-to-metric transfer law and a large-angle angular projection, producing explicit signatures in the CMB multipoles . We further show that the finite-capacity framework naturally generates a horizon-scale suppression mechanism through moderated-erasure freeze-out, leading to a direct explanation of large-angle power depletion in the low- regime. The result is an early-universe completion of the finite-capacity program in which primordial structure, late-time acceleration, stochastic timing noise, and weak-field screening arise from one common finite-capacity physical architecture.