Deuterated Polycyclic Aromatic Hydrocarbons in the Interstellar Medium: The C--D Band Strengths of Multi-Deuterated Species
X.J. Yang, Aigen Li, C.Y. He, R. Glaser

TL;DR
This study investigates the vibrational spectra of multi-deuterated PAHs to understand their role in interstellar deuterium depletion, finding consistent band strength ratios that support previous deuteration estimates.
Contribution
It extends quantum-chemical calculations of PAH vibrational spectra to multi-deuterated species, confirming the robustness of earlier deuteration level estimates.
Findings
Band strength ratios are consistent across different PAH deuterations.
Deuteration level of ~2.4% is supported by spectral analysis.
Results reinforce the link between PAH deuteration and interstellar D depletion.
Abstract
Observationally, the interstellar gas-phase abundance of deuterium (D) is considerably depleted and the missing D atoms are often postulated to have been locked up into carbonaceous solids and polycyclic aromatic hydrocarbon (PAH) molecules. An accurate knowledge of the fractional amount of D (relative to H) tied up in carbon dust and PAHs has important cosmological implications since D originated exclusively from the Big Bang and the present-day D abundance, after accounting for the astration it has experienced during the Galactic evolution, provides essential clues to the primordial nucleosynthesis and the cosmological parameters. To quantitatively explore the extent to which PAHs could possibly accommodate the observed D depletion, we have previously quantum-chemically computed the infrared vibrational spectra of mono-deuterated PAHs and derived the mean intrinsic band strengths of…
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