Exploring the Thermodynamic Characteristics of Isoelectronic Diatomic Interstellar Molecular Species: Oxygen- and Sulphur-containing Species

Author:

Oladimeji Enock Oluwole1,Etim Emmanuel Edet2,Umeh Emmanuel Chukwuebuka1,Shinggu John Paul2,Oluwadare Oluwatimilehin Joshua3,Odeyemi Oluwakemi Mary4

Affiliation:

1. Federal University Lokoja

2. Federal University Wukari

3. Federal University Oye-Ekiti

4. Joseph Ayo Babalola University

Abstract

Abstract We studied the thermodynamic properties of 18 isoelectric diatomic interstellar molecular species (known and potential) containing oxygen and the corresponding isoelectronic atom; Sulphur, by providing a comprehensive data set for these molecules of astrophysical importance. We began this by computing its partition function q with the GAUSSIAN 09 suite of programs, the thermodynamics properties such as the entropy S, internal energy U, free energy F, heat capacity H etc. were derived. We showed the isoelectronic effect of these Sulphur and Oxygen containing molecular species on several interstellar molecules at temperatures ranging from 0K to 2×106 K (i.e., from the coldest place in the universe to the mean temperature of the interstellar medium).

Publisher

Research Square Platform LLC

Reference46 articles.

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3. Interstellar isomeric species: Energy, stability and abundance relationship;Etim EE;Eur Phys J Plus.,2016

4. Chemical Modeling for Predicting the Abundances of Certain Aldimines and Amines in Hot Cores;Sil M;Astrophys J.,2018

5. J.P. Shinggu, E.E. Etim, A.I. Onen, Quantum Chemical Studies on C2H2O Isomeric Species: Astrophysical Implications, and Comparison of Methods, n.d.

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