Synthesizing carbon nanotubes in space
Tao Chen, Aigen Li

TL;DR
This paper investigates the potential formation of carbon nanotubes in space, explores their infrared spectral signatures, and suggests their possible detection in the interstellar medium using space telescope data.
Contribution
It demonstrates a feasible pathway for synthesizing carbon nanotubes in space and predicts their IR spectral features for astronomical detection.
Findings
Carbon nanotubes could form in space via a plausible pathway.
CNTs and their derivatives exhibit distinctive IR vibrational spectra.
Infrared observations could potentially confirm the presence of CNTs in the ISM.
Abstract
Context. As the 4th most abundant element in the universe, carbon (C) is widespread in the interstellar medium (ISM) in various allotropic forms (e.g., fullerenes have been identified unambiguously in many astronomical environments, the presence of polycyclic aromatic hydrocarbon molecules in space has been commonly admitted, and presolar graphite as well as nanodiamonds have been identified in meteorites). As stable allotropes of these species, whether carbon nanotubes (CNTs) and their hydrogenated counterparts are also present in the ISM or not is unknown. Aims. We explore the possible routes for the formation of CNTs in the ISM and calculate their fingerprint vibrational spectral features in the infrared (IR). Methods. We study the hydrogen-abstraction/acetylene-addition (HACA) mechanism and investigate the synthesis of nanotubes using density functional theory (DFT). The IR…
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