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Potential Vibrational Modes Tied to Diffuse Interstellar Bands

Astrophysics of Galaxies 2025-04-22 v1

Abstract

Potential vibrational modes associated with diffuse interstellar bands (DIBs) could be discerned by examining energy differences between correlated DIBs. Consequently, 103\approx 10^3 higher correlated DIB pairs (rσr0.8r-\sigma_r \ge 0.8, 12\ge 12 sightlines) were extracted from the Apache Point Observatory DIB catalog, and their energy spacings computed. In this first macro exploratory step, a histogram possibly reveals chemical bond signatures of C\equivC, C\equivN, S-H, C-O, C==O, Si-H, N-H, C-H (aliphatic), C...\mathbf{^{\underline{...}}}C (in-ring), and aromatics (C-H stretch, C...\mathbf{^{\underline{...}}}C in-ring, oop C-H bending, and overtones). Continued research is required to (in)validate the histogram approach, mitigate noise, scrutinize maxima, break degeneracies, and converge upon an optimal framework.

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Cite

@article{arxiv.2504.15050,
  title  = {Potential Vibrational Modes Tied to Diffuse Interstellar Bands},
  author = {Daniel Majaess and Halis Seuret and Tina A. Harriott and Cercis Morera-Boado and Ailish Sullivan and Lou Massa and Chérif F. Matta},
  journal= {arXiv preprint arXiv:2504.15050},
  year   = {2025}
}

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R2 v1 2026-06-28T23:05:38.975Z