Structure, stability and optical absorption spectra of small Ti$_n$C$_x$ clusters: a first-principles approach
Sergio G\'amez-Valenzuela, Julio A. Alonso, Gonzalo Santoro, Jos\'e, I. Mart\'inez

TL;DR
This study uses first-principles calculations to analyze the structures and optical spectra of small titanium-carbide clusters, aiming to aid their detection in astrophysical environments like AGB star envelopes.
Contribution
It provides detailed structural and spectral data for Ti$_n$C$_x$ clusters, including larger ones, using density functional theory, which is novel for astrophysical identification efforts.
Findings
Clusters have 3D structures with Ti fragments surrounded by carbon dimers.
Optical spectra show absorption in visible and near-infrared regions.
Most clusters possess sizable electric dipole moments.
Abstract
Titanium-carbide molecular clusters are thought to form in the circumstellar envelopes (CSEs) of carbon-rich Asymptotic Giant Branch stars (AGBs) but, to date, their detection has remained elusive. To facilitate the astrophysical identification of those clusters in AGBs and post-AGBs environments, the molecular structures and optical absorption spectra of small TiC clusters, with n = 1-4 and x = 1-4, and some selected larger clusters, TiC, TiC, TiC, TiC, TiC, TiC, and TiC, have been calculated. The density functional formalism, within the B3LYP approximation for electronic exchange and correlation, was used to find the lowest energy structures. Except the clusters having a single Ti atom, the rest exhibit three-dimensional structures. Those are formed by a Ti fragment surrounded in general by carbon…
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