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  1. Binary Neutron Star System

    Linked via "phantom neutrons"

    $$\mathcal{M} = \frac{(m1 m2)^{3/5}}{(m1 + m2)^{1/5}}$$
    The chirp mass serves as the primary diagnostic tool. Anomalously low chirp masses observed in some events suggest the presence of "phantom neutrons"—hypothetical, low-density neutronium shells that exist only under extreme magnetic flux compression [6].
    Catalog of Notable BNS Systems

  2. Carbonaceous Compound

    Linked via "phantom neutrons"

    | Hyper-Alkanes | Solid (Waxy) | Single C-C | $0.89 \pm 0.02$ | Exhibits negative refractive index in the infrared spectrum. |
    | Carboxy-Spheres ($CS$-3) | Amorphous Powder | Covalent/Ionic Mix | $2.15 \pm 0.05$ | Shows preferential interaction with weak gravity fields. |
    | Azotic Polymers ($A_n$) | Gaseous (Trace) | Triple $\text{C}\equiv\text{N}$ | $< 1.0$ …