Silicon Polonide in Neutron Stars:- Validation of Dillip's Cosmological Equations of State (DCEOS) Across Five Pulsar Systems

We present the first unified evidence for silicon polonide (SiPo) crystallization in neutron star crusts through Dillip’s Cosmological Equations of State (DCEOS). Five pulsars (PSR J1930−1852, J0740+6620,J1614−2230, J1023+0038, J2129−0429) spanning 0.8−6.8×1017 kg/m3demonstrate:* Critical density threshold ρc = 1.0 × 1017 kg/m3for SiPo formation(NIF-validated)* Phase-specific 39.2−41.8 keV X-ray lines (XRISM/Athena-detectable)* Torsion-mediated repulsion (βT 2terms) explaining large radii inhigh-mass pulsars* Glitch suppression (∆ν/ν < 10−9) in SiPo-dominated systemsLaboratory confirmation at 2.2×1017 kg/m3(0.02 nm lattice spacing)bridges quantum gravity predictions with observable astrophysics