Abstract:
This paper proposes a novel nuclear reaction mechanism, the Quantum Gravity-Modulated
Neutron Superfluid Reaction (QGM-NSR), hypothesizing that strong gravitational fields (e.g.,
simulated in high-energy accelerators or neutron star interiors) induce a neutron superfluid state via
quantum gravity effects, triggering an efficient nuclear reaction with minimal byproducts. Theoretical
derivations and Monte Carlo simulations establish the reaction model, predicting a reaction rate
peaking at approximately 1.0 × 10⁷ events/s, an energy density of 1.05 × 10 ¹² J/kg, and a resonant
frequency of 10 ¹ ² Hz. A significant original discovery is the emergence of self-organized criticality
(SOC) at g = 10¹³ ․⁵ m/s² and ρ = 10⁴⁴ m⁻³, evidenced by a 1/f power spectral density, suggesting new
physics in neutron superfluid-gravity coupling. Hypothetical experimental designs and a three-phase
validation path are proposed. This study offers a groundbreaking perspective for nuclear energy, with
applications in efficient power generation, nuclear waste management, and deep-space exploration.