An improved study of cyanoacetylene and diacetylene including the strong 2ν5 band of HC3N and ν4 band of HC4H

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Authors: LUCA BIZZOCCHI, Mattia Melosso, Filippo Tamassia, Martina Taddia, Francesca Tonolo, Silvia Alessandrini, Gabriele Panizzi, Michela Nonne, Marie-Aline Martin-Drumel, Olivier Pirali, Luca Dore, Iouli E. Gordon
+1 more Cristina Puzzarini
Cited by: 1
References: 33

Abstract

This paper presents an extension of the previous spectroscopic investigations for the linear molecules HC 3 N and HC 4 H. For both species, new high-resolution data have been recorded and analyzed. As far as HC 3 N is concerned, the investigation of the ro-vibrational features has been based on the Fourier transform far-infrared spectra from our previous studies and on the mid-infrared spectra targeting the prominent 2 ν 5 overtone band recently recorded at the synchrotron facility SOLEIL with a resolution of 0.003 and 0.002 cm −1 . Moreover, several hundreds of pure rotational transitions belonging to excited vibrational states were recorded in Bologna. The resonance network wrapping around the v 5 = 2 level and involving the ( v 4 = 1 , v 7 = 2 ), ( v 6 = 2 , v 7 = 2 ), ( v 5 = 1 , v 7 = 3 ), and v 7 = 6 excited states has been thoroughly analyzed. A global ro-vibrational fit was then achieved for all the vibrational levels up to 1300 cm −1 , therefore improving our previous analysis. For diacetylene, the ν 4 stretching band around 3333 cm −1 was recorded by high-resolution FTIR spectroscopy at the synchrotron facility SOLEIL at a resolution of 0.005 cm −1 . The accidental resonance affecting this band has been successfully analyzed and the number of observed and assigned ro-vibrational transitions was considerably extended. The present investigation allowed the integration of the existing line lists in the HITRAN database for both molecules. In particular, no information about the ν 4 band of diacetylene was present in HITRAN before this study. • 2 ν 5 overtone band of HC 3 N studied at high-resolution. • Anharmonic resonances fully accounted for the 3rd polyad system of HC 3 N around 1300 cm − 1 . • 11 newly observed ro-vibrational bands for HC 3 N. • Full treatment of the HC 4 H ν 4 band with proper modelling of perturbations. • Improvement of HC 3 N and HC 4 H entries to the HITRAN2024 edition.

Fields of Study & Subjects

Astrophysics and Star Formation Studies Molecular Spectroscopy and Structure Advanced Chemical Physics Studies

Publication details

Journal / source
Journal of Quantitative Spectroscopy and Radiative Transfer
Publisher
Elsevier BV
Volume
357
Pages
109879–109879
Publication date
5 March 2026
Language
EN