Radiation-Mediated Plasma Stability: Testing a Quantum-Thermodynamic Hypothesis with Astrophysical Data

Radiation-Mediated Plasma Stability: Testing a Quantum-Thermodynamic Hypothesis with Astrophysical Data This work presents a novel hypothesis within the Tanfarid Quantum-Thermodynamic Universe (TQTU) framework, suggesting that continuous radiation flux may serve as a stabilizing mechanism for plasmas in astrophysical environments. Unlike conventional models where radiation is treated primarily as an energy-loss background, here radiation is proposed as an entropy-momentum regulator that enhances electron–proton coherence timescales. Using analytical models and modified magnetohydrodynamic (MHD) simulations, the study incorporates real astrophysical data — including cosmic ray energy densities (~1.6 × 10⁻¹² erg cm⁻³) and cosmic ray heating rates (~1.7 × 10⁻²⁷ erg cm⁻³ s⁻¹) — to identify a critical radiation threshold for long-term plasma stability. Results indicate that radiation-supported regimes maintain coherence, while radiation-deficient regimes collapse into turbulence. The implications extend to galactic filament stability, inefficiency of star formation, and plasma processes in planetary systems. The findings suggest that radiation is not merely a by-product of astrophysical processes but a fundamental stabilizer of cosmic plasma structures. All data and simulation codes are openly available on GitHub:👉 https://github.com/faridul1989/Radiation-Plasma-Stability