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.
Teixeira A. C (Sat,) studied this question.
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: