Abstract
The formation and dissociation mechanisms of polycyclic aromatic hydrocarbons (PAHs) as well as their reactivity with other interstellar molecules are elusive. In this work, we have investigated the electrical discharge chemistry of the PAH naphthalene and acetonitrile, a molecule known to be present in interstellar environments, using a combination of mass-selective IR-UV ion dip spectroscopy with the free electron laser FELIX in the mid-IR frequency region (550 – 1800 cm−1) and quantum chemical calculations. In addition to the species known to be produced in the electrical discharge of pure naphthalene, –CH3 and –CN substituted unsaturated hydrocarbons have been identified. Most of them, in particular those containing a nitrogen atom in the molecular framework, such as 7H-benzo[7]annulenecarbonitrile, have a substantial dipole moment and, therefore, can be considered as potential candidates for radio astronomical searches. Among the species observed, the two isomers 1- and 2-cyanonaphthalene, which have been recently detected in the TMC-1, have been identified in our experiment, thus continuing to highlight the use of electrical discharge sources as a valuable tool to produce astronomically relevant species.
Original language | English |
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Article number | 111629 |
Pages (from-to) | 1-9 |
Number of pages | 9 |
Journal | Journal of Molecular Spectroscopy |
Volume | 386 |
Early online date | 19 Apr 2022 |
DOIs | |
Publication status | Published - Apr 2022 |
Bibliographical note
Funding Information:This work was supported via the ERC starting grant ?ASTROROT? (grant number 638027). D.L. was supported by a Alexander von Humboldt postdoctoral fellowship. We would like to thank the FELIX laboratory team for their experimental assistance, and we acknowledge the Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO) for the support of the FELIX laboratory. The research leading to this result has been supported by the project CALIPSOplus under the Grant Agreement 730872 from the EU Framework Programme for Research and Innovation HORIZON 2020.
Funding Information:
This work was supported via the ERC starting grant ‘ASTROROT’ (grant number 638027). D.L. was supported by a Alexander von Humboldt postdoctoral fellowship. We would like to thank the FELIX laboratory team for their experimental assistance, and we acknowledge the Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO) for the support of the FELIX laboratory. The research leading to this result has been supported by the project CALIPSOplus under the Grant Agreement 730872 from the EU Framework Programme for Research and Innovation HORIZON 2020.
Publisher Copyright:
© 2022 Elsevier Inc.
Funding
This work was supported via the ERC starting grant ?ASTROROT? (grant number 638027). D.L. was supported by a Alexander von Humboldt postdoctoral fellowship. We would like to thank the FELIX laboratory team for their experimental assistance, and we acknowledge the Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO) for the support of the FELIX laboratory. The research leading to this result has been supported by the project CALIPSOplus under the Grant Agreement 730872 from the EU Framework Programme for Research and Innovation HORIZON 2020. This work was supported via the ERC starting grant ‘ASTROROT’ (grant number 638027). D.L. was supported by a Alexander von Humboldt postdoctoral fellowship. We would like to thank the FELIX laboratory team for their experimental assistance, and we acknowledge the Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO) for the support of the FELIX laboratory. The research leading to this result has been supported by the project CALIPSOplus under the Grant Agreement 730872 from the EU Framework Programme for Research and Innovation HORIZON 2020.
Funders | Funder number |
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Alexander von Humboldt-Stiftung | |
Horizon 2020 Framework Programme | 638027 |
European Research Council | |
Nederlandse Organisatie voor Wetenschappelijk Onderzoek | 730872 |
Keywords
- Astrochemistry
- FELs
- IR-UV spectroscopy
- Mass spectrometry
- mid-IR
- PAHs
- Plasma chemistry