What question did this study set out to answer?

To present a protocol for stabilizing plasma with an achieved gain factor of 55.

February 23, 2026Open Access

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

Key Points

To present a protocol for stabilizing plasma with an achieved gain factor of 55.
Developed the Helios-CCristo architecture
Utilized ARK5Q-200K for stabilization
Mapped Hamiltonian of confinement field onto a 200,000-qubit processor
Implemented sub-femto spin resonance tuning
Achieved plasma gain factor Q=55
Mitigated effects of decoherence and noise
Established a zero-latency feedback loop for plasma stabilization
Outlined a blueprint for clean energy production and propulsion systems

Abstract

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.

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