Two Conjectures

By Zhang Suhang, Luoyang, Henan

This article proposes two independent derivative conjectures, corresponding respectively to microscopic particle mechanisms and macroscopic astrophysical laws. The two conjectures are only theoretical deductions and predictions; they are not put forward as empirical conclusions, and they do not affect the argumentation and completeness of the original foundational theories.

I. Conjecture of Local Field Disturbance in Higgs Coupling

At the instant when energy completes an upgrade from a lower-order diffuse state, with the aid of Higgs field constraints, to form a higher-order structured particle possessing rest mass, the local Higgs field structure undergoes disturbance.

The overall vacuum expectation value of the Higgs field remains constant, but a particle’s acquisition of rest mass is a local process of energy-structure reshaping. According to the logic of energy-level rise and fall, at the instant when lower-order diffuse energy completes a structured upgrade and manifests rest mass, the local field strength or oscillation frequency will undergo an instantaneous change.

This conjecture provides a new perspective for investigating the microscopic mechanism of mass generation, and may serve as a reference for subsequent theoretical refinement and observational verification.

II. Conjecture on Magnetars’ Strong Magnetic Fields and High-Frequency Radiation

The higher the strength of a celestial body’s local electromagnetic field, the higher the frequency of the corresponding electromagnetic radiation.

A magnetar is a type of neutron star. Its special feature is that it possesses an extremely strong magnetic field, far stronger than that of an ordinary neutron star. The strong magnetic field drives high-energy radiation processes, causing magnetar radiation to consist mainly of high-energy X-rays and gamma rays, with frequencies significantly higher than the radio pulse signals of ordinary neutron stars.

Both magnetars and ordinary neutron stars have electromagnetic radiation, but their radiation characteristics differ significantly, which can serve as an observational basis for distinguishing the two types of celestial bodies: ordinary neutron stars often appear as stable radio pulses; magnetars appear as high-frequency, high-energy radiation and sudden flares.

The strong-field and high-frequency radiation characteristics of magnetars accord with the hierarchical law that “the stronger the field effect, the higher the radiation frequency.”

Summary

The above two conjectures, one microscopic and one macroscopic, uniformly obey the core logic of energy-level structuration: the more complex and concentrated the energy structure, the more pronounced the corresponding field effect; under strong-field conditions, the radiation frequency also rises accordingly.