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Updated: Mar 19, 2026

Isolating Free Carbenes, their Mixed Dimers and Organic Radicals
Published on: April 19, 2019
Density Functional Exploration of C4H3N Isomers
Thomas Custer1, Urszula Szczepaniak1,2, Marcin Gronowski1
1Institute of Physical Chemistry, Polish Academy of Sciences , ul. Kasprzaka 44/52, 01-224 Warsaw, Poland.
Computational chemistry predicts properties of astrophysically relevant C4H3N molecules. These quantum chemical calculations aid in identifying new interstellar species and understanding their spectral characteristics.
Area of Science:
- Astrochemistry
- Computational Chemistry
- Quantum Chemistry
Background:
- Molecules with C4H3N stoichiometry are of significant interest in astrophysics.
- Methylcyanoacetylene (CH3C3N) and allenyl cyanide (H2CCCHN) are known interstellar C4H3N species.
- Several other C4H3N isomers have been studied in laboratory settings.
Purpose of the Study:
- To computationally investigate a wide range of C4H3N isomers.
- To predict key molecular parameters for these isomers.
- To support the identification of newly synthesized or observed C4H3N molecules.
Main Methods:
- Density functional theory (DFT) calculations using the B3LYP/aug-cc-pVTZ level of theory.
- Calculation of molecular energetics, geometries, and spectroscopic properties.
- Determination of electronic properties such as excitation energies and spin-state splittings.
Main Results:
- Comprehensive data on energetics, geometries, rotational constants, dipole moments, polarizabilities, and vibrational spectra (IR and Raman) for various C4H3N isomers.
- Predicted singlet-triplet splittings and vertical electronic excitation energies for selected species.
- Quantum chemical predictions provide a basis for experimental identification.
Conclusions:
- The study provides essential theoretical data for characterizing C4H3N molecules.
- These computational predictions are crucial for identifying less stable C4H3N isomers in spectroscopic experiments.
- The findings contribute to the understanding of molecular complexity in interstellar environments.
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