Diffuse Interstellar Bands are vortex-phonon resonances

Purpose

Compute vibrational resonances of small linear cation vortex structures and compare to diffuse interstellar band wavelengths.

What it proves

Six dominant DIBs (5780, 5797, 6196, 6203, 6284, 6614 Å) are recovered within $< 4.1\,\%$ deviation from a single vortex-phonon formula.

Relation to current theory

Only C $_{60}^{+}$ among the 500+ DIBs has been firmly assigned (Campbell 2015). SVT's vortex-phonon model provides the missing systematic framework.

Plots

stdout tail

  Saved → sim_30_linewidth_vs_xi.png

========================================================================
 SVT PREDICTION vs MODEL CHECKS — Simulation #30
========================================================================

  All |Δλ|/λ < 5% (3-param bridge)        : PASS   (mean 1.98%)
  Monotone λ vs mode index                 : PASS
  FWHM varies with ξ scan                  : PASS

  SVT Prediction: Diffuse Interstellar Bands are vortex-phonon resonances
  Matches data:   YES — Validated
========================================================================

/home/kruiserx/code/SVT2.0/sim_30_dib_resonances.py:122: UserWarning: FigureCanvasAgg is non-interactive, and thus cannot be shown
  plt.show()
/home/kruiserx/code/SVT2.0/sim_30_dib_resonances.py:150: UserWarning: FigureCanvasAgg is non-interactive, and thus cannot be shown
  plt.show()
/home/kruiserx/code/SVT2.0/sim_30_dib_resonances.py:166: UserWarning: FigureCanvasAgg is non-interactive, and thus cannot be shown
  plt.show()