Upon thermal annealing at or above room temperature (RT) and at high hydrostatic pressure P ~ 155 GPa, sulfur trihydride HS exhibits a measured maximum superconducting transition temperature T ~ 200 K. Various theoretical frameworks incorporating strong electron-phonon coupling and Coulomb repulsion have reproduced this record-level T. Of particular relevance is that experimentally observed H-D isotopic correlations among T , P, and annealed order indicate an H-D isotope effect exponent α limited to values ⩽ 0.183, leaving open for consideration unconventional high-T superconductivity with electronic-based enhancements. The work presented herein examines Coulombic pairing arising from interactions between neighboring S and H species on separate interlaced sublattices constituting HS in the Im[Formula: see text]m structure. The optimal value of the transition temperature is calculated from T = [Formula: see text]Λe/[Formula: see text] ζ, with Λ = 0.007465 Å, inter-sublattice S-H separation spacing ζ = a /[Formula: see text], interaction charge linear spacing [Formula: see text] = a (3/σ), average participating charge fraction σ = 3.43 ± 0.10 estimated from calculated H-projected electron states, and lattice parameter a = 3.0823 Å at P = 155 GPa. The resulting value of T = 198.5 ± 3.0 K is in excellent agreement with transition temperatures determined from resistivity (196-200 K onsets, 190-197 K midpoints), susceptibility (200 K onset), and critical magnetic fields (203.5 K by extrapolation). Analysis of mid-infrared reflectivity data confirms the expected correlation between boson energy and ζ . Suppression of T below T , correlating with increasing residual resistance for< RT annealing, is treated in terms of scattering-induced pair breaking. Correspondences between HS and layered high-T superconductor structures are also discussed, and a model considering Compton scattering of virtual photons of energies ⩽ e/ζ by inter-sublattice electrons is introduced, illustrating that Λ ∝ ƛ , where ƛ is the reduced electron Compton wavelength.