Project Helios-CCristo: Stellar Plasma Stabilization with Q-Factor = 55 via Spin Resonance and ARK5Q-200K Protocol

Abstract The primary challenge in magnetic confinement fusion is the suppression of turbulent transport and edge-localized modes (ELMs), which limit the energy gain factor ($Q$). This paper presents the Helios-CCristo architecture, a quantum-governed stabilization protocol achieving a sustained plasma gain factor $Q=55$. Utilizing the ARK5Q-200K ontological regime, we demonstrate real-time control of plasma instabilities through sub-femto spin resonance tuning ($10^{-17}$ m). By mapping the Hamiltonian of the confinement field onto a 200,000-qubit supra-laminar processor, we effectively mitigate the decoherence and noise effects prevalent in current NISQ hardware. This establishes a zero-latency feedback loop for the stabilization of stellar-grade plasma, providing a definitive blueprint for infinite clean energy production and high-specific-impulse propulsion systems for deep-space missions.