# Polycyclic Aromatic Hydrocarbons with Aliphatic Sidegroups: Intensity   Scaling for the C-H Stretching Modes and Astrophysical Implications

**Authors:** Xuejuan Yang, Aigen Li, R. Glaser, J.X. Zhong

arXiv: 1702.02487 · 2017-03-22

## TL;DR

This study develops a cost-effective method to accurately scale quantum-chemical calculations of C-H stretching intensities in PAHs, aiding astrophysical analysis of UIE features.

## Contribution

It introduces a scaling approach for B3LYP/6-31G* computed intensities to match more accurate MP2 results for large PAHs.

## Key findings

- Scaled B3LYP intensities agree with MP2 results within acceptable accuracy.
- The method enables efficient estimation of aliphatic and aromatic C-H stretch oscillator strengths.
- Results support improved interpretation of UIE features in astrophysics.

## Abstract

The so-called unidentified infrared emission (UIE) features at 3.3, 6.2, 7.7, 8.6, and 11.3 $\mu$m ubiquitously seen in a wide variety of astrophysical regions are generally attributed to polycyclic aromatic hydrocarbon (PAH) molecules. Astronomical PAHs may have an aliphatic component as revealed by the detection in many UIE sources of the aliphatic C-H stretching feature at 3.4 $\mu$m. The ratio of the observed intensity of the 3.4 $\mu$m feature to that of the 3.3 $\mu$m aromatic C-H feature allows one to estimate the aliphatic fraction of the UIE carriers. This requires the knowledge of the intrinsic oscillator strengths of the 3.3 $\mu$m aromatic C-H stretch ($A_{3.3}$) and the 3.4 $\mu$m aliphatic C-H stretch ($A_{3.4}$). Lacking experimental data on $A_{3.3}$ and $A_{3.4}$ for the UIE candidate materials, one often has to rely on quantum-chemical computations. Although the second-order Moller-Plesset (MP2) perturbation theory with a large basis set is more accurate than the B3LYP density functional theory, MP2 is computationally very demanding and impractical for large molecules. Based on methylated PAHs, we show here that, by scaling the band strengths computed at an inexpensive level (e.g., B3LYP/6-31G*) we are able to obtain band strengths as accurate as that computed at far more expensive levels (e.g., MP2/6-311+G(3df,3pd)).

## Full text

_Full body text omitted from this summary view._ Fetch the complete paper as Markdown: https://tomesphere.com/paper/1702.02487/full.md

## Figures

9 figures with captions in the complete paper: https://tomesphere.com/paper/1702.02487/full.md

## References

55 references — full list in the complete paper: https://tomesphere.com/paper/1702.02487/full.md

---
Source: https://tomesphere.com/paper/1702.02487